Tufail Ali Zubedi Taught EN-501: Introduction to Environmental Engineering at NED University of Engineering and Technology during Aug - Dec 2015.
This is the set of lectures and handout used by him. feel free to contact him at zubeditufail@yahoo.com
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En 501-2015-original
1. NED University of Engineering and Technology
Department of Environmental Engineering
EN501: Introduction to Environmental Engineering - Fall 2015 semester
Course Plan
Week Topic
1 Introduction to Subject, distribution of marks, Natural Resource and its
characteristics,
Global Environmental Issues, Pakistan Environmental Issues
2 Ecology, Ecosystems and Economic Growth
3 Cycles in Nature
4 Brief introduction to Air Pollution and its Management
5 Brief introduction to Water Pollution and its Management
6 Brief introduction to Solid waste and its Management
7 Brief Introduction to Noise Pollution, Radiation and its Management
8 Interrelations of air, water pollution and solid waste management, radiation,
noise pollution
9 Effects of Pathogen and Chemicals on Health
10 Economics of Environmental Pollution Control
11 Environmental Quality Objectives
12 Environmental Legislation
13 Brief Introduction to Environmental Impact Assessment
14 Environmental Standards and Technologies,
An Introduction to ISO 14001:2004
15 Student Presentation
16 Student Presentation,
Distribution of Course
Marks
Marks
1. Exams 60
2. Sessional 40
a. Class Test
Best 2 of 3
2 x 10 = 20
b. Class Report 10
c. Class Presentation 10
Class Teacher
Tufail Ali Zubedi
Cell: 0300-3538024
Email: info@SPMCpk.com; Zubeditufail@yahoo.com
http://www.SPMCpk.com/
2. Engr.TufailAli Zubedi, PE
BE Civil, ME Environmental Engg
Environmental Consultant
http://www.SPMCpk.com/
EN 501
Introduction to
Environmental Engineering
3. Today’s Talk
Round of Introduction
Class etiquettes
Course Syllabus
Distribution of Marks
Introduction to subject
5. Class Etiquettes
Student –Teacher relationship
While in class:
Smoking , Eating, Drinking, especially sleeping is not allowed
Mobile / iPod / iPads switched off
Lecture will be provided
Open to suggestions
“Learn by doing”
Language of instruction = English
6. Week Topic
1 Introduction to Subject, distribution of marks, Natural Resource and its
characteristics,
Global Environmental Issues, Pakistan Environmental Issues
2 Ecology, Ecosystems and Economic Growth
3 Cycles in Nature
4 Brief introduction to Air Pollution and its Management
5 Brief introduction to Water Pollution and its Management
6 Brief introduction to Solid waste and its Management
7 Brief Introduction to Noise Pollution, Radiation and its Management
8 Interrelations of air, water pollution and solid waste management,
radiation, noise pollution
9 Effects of Pathogen and Chemicals on Health
10 Economics of Environmental Pollution Control
11 Environmental Quality Objectives
12 Environmental Legislation
13 Brief Introduction to Environmental Impact Assessment
14 Environmental Standards and Technologies,
An Introduction to ISO 14001:2004
15 Student Presentation
16 Student Presentation,
Course Syllabus
7. Marks Distribution
Distribution of Course
Marks
Marks
1. Exams 60
2. Sessional 40
a. Class Test
Best 2 of 3
2 x 10 = 20
b. Class Report 10
c. Class Presentation 10
8. Introduction to
Environmental Engineering
The application of
Science and engineering knowledge and
concepts
To care for / restore our natural environment &
To resolve environmental problems
9. Who does it affect?
Everyone and Everything!
Plants
Insects
Animals
Humans
Ecosystems
Our planet ..
10. What to Environmental Engineer do?
Environmental Engineers are
Concerned with the negative impacts of human activity on the
environment
Also concerned with the positive impacts on the environment
Scale = micro to macro
Individual and holistic activities
Individual and cumulative impacts
Within and outside the project boundaries
11. Natural Resources
Natural resources occur naturally
within environments that exist
relatively undisturbed by humanity, in
a natural form.
A natural resource is often
characterized by amounts of
biodiversity and geodiversity existent
in various ecosystems.
Natural resources are derived from the
environment.
Some of them are essential for our
survival while most are used for
satisfying our desires.
12. A natural resource may exist as a separate entity such as
Fresh water, and air, as well as a living organism such as a fish,
or
it may exist in an alternate form which must be processed to
obtain the resource such as
metal ores, oil, and most forms of energy.
13. Classification
On the basis of origin, natural resources may be divided into:
Biotic – Biotic resources are obtained from the biosphere (living and
organic material), such as forests and animals, and the
materials that can be obtained from them.
(Oil / coal)
Abiotic – Abiotic resources are those that come from nonliving,
inorganic material.
(land, fresh water, air and heavy metals including ores)
14. Considering their stage of development,
natural resources may be:
Potential resources – Potential resources are those that exist in a region and may be
used in the future.
(petroleum but until the time it is actually drilled out and put into use,
itremains a potential resource.)
Actual resources – Actual resources are those that have been surveyed, their quantity
and quality determined and are being used in present times.
(The development of an actual resource, such as wood processing depends upon
the technology available and the cost involved.)
Reserve resources –The part of an actual resource which can be developed profitably in
the future is called a reserve resource.
Stock resources – Stock resources are those that have been surveyed but cannot be used
by organisms due to lack of technology.
(hydrogen. Shale gas)
15.
16. natural resources can be categorized as either renewable or
nonrenewable:
Renewable resources – Renewable resources can be replenished
naturally.
(sunlight, air, wind, etc.)
Resources from a human use perspective are classified as
renewable only so long as the rate of replenishment/recovery
exceeds that of the rate of consumption.
Nonrenewable resources – Nonrenewable resources either form
slowly or do not naturally form in the environment.
(fossil fuel)
17.
18. World Charter for Nature
In 1982 the UN developed theWorld Charter for Nature,
which recognized the need to protect nature from further
depletion due to human activity.
It states that measures need to be taken at all societal levels,
from international to individual, to protect nature
READ “UN-World Charter for Nature”
It outlines the need for sustainable use of natural resources
and suggests that the protection of resources should be
incorporated into national and international systems of law.
19. Reading Assignment
IUCN-Pakistan Conservation Strategy
IUCN- State of Environment and Development (SoED) of
Sindh
IUCN-Sindh Strategy for Sustainable Development
21. FINAL WORDS
There is much debate worldwide over natural resource
allocations, this is partly due to increasing scarcity (depletion
of resources) but also because the exportation of natural
resources is the basis for many economies (particularly for
developed nations).
Next Class
Global and Pakistan Environmental Issues and solutions
22. TIP
Some natural resources such as sunlight and air can be found
everywhere, and are known as ubiquitous resources.
However, most resources only occur in small sporadic areas,
and are referred to as localized resources.
There are very few resources that are considered
inexhaustible (will not run out in foreseeable future) – these
are solar radiation, geothermal energy, and air (though access
to clean air may not be).The vast majority of resources are
exhaustible, which means they have a finite quantity, and can
be depleted if managed improperly.
24. 11/20/2015 A/RES/37/7. World Charter for Nature
http://www.un.org/documents/ga/res/37/a37r007.htm 1/5
United Nations A/RES/37/7
General Assembly
Distr. GENERAL
28 October 1982
ORIGINAL:
ENGLISH
A/RES/37/7
48th plenary meeting
28 October 1982
37/7. World Charter for Nature
The General Assembly,
Having considered the report of the Secretary‐General on the revised
draft World Charter for Nature,
Recalling that, in its resolution 35/7 of 30 October 1980, it expressed
its conviction that the benefits which could be obtained from nature depended
on the maintenance of natural processes and on the diversity of life forms and
that those benefits were jeopardized by the excessive exploitation and the
destruction of natural habitats,
Further recalling that, in the same resolution, it recognized the need
for appropriate measures at the national and international levels to protect
nature and promote international co‐operation in that field,
Recalling that, in its resolution 36/6 of 27 October 1981, it again
expressed its awareness of the crucial importance attached by the
international community to the promotion and development of co‐operation aimed
at protecting and safeguarding the balance and quality of nature and invited
the Secretary‐General to transmit to Member States the text of the revised
version of the draft World Charter for Nature contained in the report of the
Ad Hoc Group of Experts on the draft World Charter for Nature, as well as
any further observations by States, with a view to appropriate consideration
by the General Assembly at its thirty‐seventh session,
Conscious of the spirit and terms of its resolutions 35/7 and 36/6, in
which it solemnly invited Member States, in the exercise of their permanent
sovereignty over their natural resources, to conduct their activities in
recognition of the supreme importance of protecting natural systems,
maintaining the balance and quality of nature and conserving natural
resources, in the interests of present and future generations,
Having considered the supplementary report of the Secretary‐General,
Expressing its gratitude to the Ad Hoc Group of Experts which, through
its work, has assembled the necessary elements for the General Assembly to be
able to complete the consideration of and adopt the revised draft World
Charter for Nature at its thirty‐seventh session, as it had previously
recommended,
30. NATURAL RESOURCES
Soil
Mountains
Rivers and Canals
Forests
Animals
Minerals
The resources gifted by the nature to the
country and the people are called National
Resources.
SOHAIL AHMED 2
31. SOIL
• Fertile Plains and deserts are important part
of natural resources.
• More fertile plain a country has means more
Agricultural department.
• Allah has gifted many fertile plains to
Pakistan.
• Pakistan Can Cultivate a number of different
foods.
SOHAIL AHMED 3
32. MOUNTAINS
• Mountains are the gift of the nature.
• They protect from the cool winds
• Mountains are rich in minerals.
• Mountain provide water to our rivers.
• Mountains of Pakistan are rich in minerals
especially the Western Mountain Ranges.
SOHAIL AHMED 4
33. RIVERS AND CANALS
• The underground water, rivers and oceans are
natural resources
• The river system of Pakistan is consisted of
Indus and other associated rivers.
• We use water for drinking purposes and store
the water of the rivers and use it for different
purposes like irrigation, for hydroelectricity etc.
SOHAIL AHMED 5
34. FORESTS
• They are helpful in improvement of weather
• Protect against windstorms
• Help in slow melting of snow to stop floods.
• Much More to explain
• Normally 25 percent area of a country should
be covered with forest. But in Pakistan it is
only 4 to 5 percent.
SOHAIL AHMED 6
35. ANIMALS
• Animals provide milk, meat, hide and skins,
wool etc.
• They are also used for agriculture and
transportation.
• They are a source of foreign exchange.
• Pakistan is Gifted by Nature a lot of Different
types of Animals
SOHAIL AHMED 7
36. MINERAL RESOURCES
The term Mineral Resource is used to refer to
any of a class of naturally occurring solid
inorganic substances with a characteristic
crystalline form and a homogeneous chemical
composition.
SOHAIL AHMED 8
37. MINERALS OF PAKISTAN
In Pakistan there is wide scale availability of
mineral resources, but these resources remained
unexploited for years. It is due to lack of
technical skill, finance and technology.
SOHAIL AHMED 9
38. IMPORTANT MINERALS OF PAKISTAN
• Coal
• Natural Gas
• Iron ore
• Chromite
• Gypsum
• Sulphur
• Oil
• Uranium
SOHAIL AHMED 10
39. COAL
• The annual coal production of Pakistan is 3.2
million tones.
• Coal is used in power generation. It is basically
used as fuel.
• It is mostly found in Sindh (Thatta, Tharparkar,
Manara) Balochistan (Deegari, Maach), Punjab
(Makarwal, Dandot),NWFP (Cherat and Noshera).
SOHAIL AHMED 11
40. NATURAL GAS
• It is itself a source of energy and fuel.
• Used as a source of power generation.
• It is found in Sui, Mari, Uch, Khairpur,
Jacobabad etc.
• Now some new discoveries are also found.
SOHAIL AHMED 12
41. IRON ORE
• Iron Ore is used for industry, especially steel
industry.
• Its deposits are found in Chitral, Chaghai,
Kohat, Kurram Agency, Mardan, Hazara,
Mianwali (Kalabagh) and DG Khan.
SOHAIL AHMED 13
42. CHROMITE
• Chromite is used in preparing other metals,
leather tanning, making of steel products,
armament and stainless steel.
• Found in Zoab (Muslim Bagh), Chaghai,
Malakand, Mahmand, Waziristan, Fort
Sandaman etc.
SOHAIL AHMED 14
43. GYPSUM
• Gypsum is used for plaster of Paris, Paints
and Cement.
• It is found in Jhelum, Mianwali, DG Khan,
Kohat and Loralai.
SOHAIL AHMED 15
44. SULPHUR
• Sulphur is used by chemical industry.
• Its deposits are found in Kalat, Khairpur,
Mardan, and Jacobabad etc.
SOHAIL AHMED 16
45. OIL
• It is a major source of energy.
• It is mostly imported from Iran and Gulf
states.
• Now some valuable reserves are found in
Jhelum, Mianwali, Attock, Balkasar, Mial,
Chakwal, and Dhodak.
SOHAIL AHMED 17
46. URANIUM
• It is the basic element for atomic power,
indispensable for the defence.
• Its deposits are in DG Khan, Hazara and
Kohat.
SOHAIL AHMED 18
47. Pakistan is blessed with considerable
mineral resources. Some of them are
explored but much remains to be done for
the search for more
SOHAIL AHMED 19
49. EN 501
Introduction to
Environmental Engineering
Engr.TufailAli Zubedi, PE
BE Civil, ME Environmental Engg
o e ta g ee g
Environmental Consultant
http://www.SPMCpk.com/
51. In March 1992, the Government of Pakistan adopted the National
Conservation Strategy (NCS)Conservation Strategy (NCS).
It addresses the issues of conservation and sustainable use of
natural resources for economic development.
IUCN Pakistan supported the Federal Government for the
development of relevant provincial level strategies.
IUCN's Sindh Programme was established in 2002.IUCN s Sindh Programme was established in 2002.
IUCN Sindh Programme initiated the process of developing a
report on the State of Environment and Development of Sindh (SoED)
to bridge the existing information gap and to cater to the needs ofto bridge the existing information gap and to cater to the needs of
a wide range of stakeholders, who have been striving for the
sustainable development of Sindh.
52. The report may also serve as a baseline for policy makers,
planners, and development practitioners.
The next logical step to the SoED is to develop a Sustainable
Development Strategy for SindhDevelopment Strategy for Sindh.
The SoED is intended to provide the basis for devising this
Strategy, which aims to provide an overall framework togy, p
address the Province's environmental and development issues
in a holistic manner.
53. SINDH IN THE NATIONAL CONTEXTSINDH IN THE NATIONAL CONTEXT
Sindh is located in the south-east of Pakistan.
Throughout history it has been known by many names;
Sindh comprises of Lower Indus Basin.
Is the second-most populous province after the Punjab and
Covers 140,914 square kilometre (km), with a northsouth
l th f b t 540 k d b dth f b t 250 klength of about 540 km and a breadth of about 250 km.
lies between 23° and 28 ° North latitudes and 66° and 71°
East longitudesEast longitudes.
54. TopographyTopography
Sindh can be divided into four distinct parts
dry and barren Kirthar Range in the west,
a central alluvial plain bisected by the River Indus,
a desert belt in the east anda desert belt in the east, and
the Indus delta in the south.
55. Mountainous RangesMountainous Ranges
Western Sindh is the only region which is mountainous
It includes the hill ranges of
Kirthar,
P bPab,
Laki, and
Kohistan.Kohistan.
Small hilly tract in the southeast corner of theTharparkary p
District known as Nagarparkar.
56. The Kirthar RangeThe Kirthar Range
Kirthar has a simple, anticlinal structure with flanks gently
dipping towards west and south.
These ranges run north to south like a crescent turned
towards the low lands and extend up to the northerntowards the low lands and extend up to the northern
extremity of the province.
The highest altitude known as Kutay-jee- Kabar (Dog'sg y j ( g
Grave) is in the Kirthar Range and is 2072.64 meters high.
57. The Laki RangeThe Laki Range
The Laki Range, is mainly composed of tertiary rocks and
contains a large number of thermal springs.
58.
59. The hilly region of western Sindh consists almost entirely of rocks belonging to
the tertiary system of geological nomenclature.y y g g
Only along the Laki Range and in its neighborhood that there are some
exposures of rocks belonging to the next older system, the Cretaceous.
With the exception of some volcanic beds associated with these Cretaceous
strata, all the rock formations of western Sindh are of sedimentary origin.
All of the more important hill masses consist of limestone.
A great majority of these limestone deposits belong to the Nummultic periodA great majority of these limestone deposits belong to the Nummultic period
and are largely built up of the accumulated shells of foraminifera, principally
those belonging to the genus Nummulites.
The isolated hills of Nagarparkar on the northern border of the Rann of Kutch
belong to quite a different system both geographically and geologically.
60. A large part of Sindh lies in the deltaic plain of the Lower
IndusValley. Most of this region consists of plains overlain by
alluvium, trenched with river channels in some places and
overridden by raised terraces in othersoverridden by raised terraces in others.
A few isolated low limestone hills are the only relieving
features in the plains which are otherwise at one level.p
The plains may be subdivided into three parts:
the western valley,
the eastern valley, and
The deltaic area.
61. The western valley section is distinguished from the eastern
valley by the presence of old alluvium(wind-borne sand) and
seasonal nala flowing from the Kirthar mountain range into
the Manchar Lakethe Manchar Lake.
The deltaic area largely consists of mangrove swamps and
sandbars.The chief characteristic of the region is the creeks,g
which serve as the changing outlets of the Indus and as inlets
for the sea.
62. The eastern part of Sindh consists of theThar Desert which
continues into Rajputana (India).
The landscape is sandy and rough with sand dunes covering
more than 56 percent of the areamore than 56 percent of the area.
The sand dunes are mostly longitudinal with a north-east-
south-west trend and are stabilized by shrub vegetation andy g
grass.
63.
64. VegetationVegetation
characteristic features indicative of a rainless climate, dry
atmosphere and sandy soil largely impregnated with salt.
Another feature of the vegetation in the province is the
prominence and variety of grassesprominence and variety of grasses.
65.
66. The most striking characteristic is the predominance of
l t ith ll l t ll lik th l flplants with small leaves, or none at all, like the leafless caper,
milkbush and the cactus (Euphorbia nereifolia).The large leaved
Banyan tree,like the pipal,was introduced later.
Except for the irrigated Indus valley, the province is arid and
with little vegetation.The dwarf palms, Kher (Acacia rupestris),
and Lohirro (Tecoma undulata) trees are typical of the western hilland Lohirro (Tecoma undulata) trees are typical of the western hill
region.
In the central valley, the babul (known as Babur in Sindhi) tree is
the most dominant and occurs in thick forests along the Indus
banks.
67. The neem (Azadirachta indica),ber (Zizyphys vulgaris) or jojoba,
lai (Tamarix orientalis) and kirirr (Capparis decidua) are among the
more common vegetation types.
Mango date palms and the more recently introducedMango, date palms, and the more recently introduced
banana, guava, orange and chiku are the common fruit-bearing
trees of the irrigated areas.g
68. The coastal strip and the creeks abound in semi-aquatic and
aquatic plants and the in-shore Indus deltaic islands support
forests of timmer (Avicennia marina) (timmer ja bela) and
chaunir (Ceriops tagal) treeschaunir (Ceriops tagal) trees.
Water lilies grow in abundance in the numerous lakes and
ponds, particularly in the Lower Sindh region.p p y g
82. Sustainable Solid Waste Management-
Application of Modern Landfill Concept
Presenter: Mubashir Saleem
NED University of Engineering & Technology
August 13, 2015
83. - Name: Mubashir Saleem
- Professional Experiance: 2 years in the Design and drawing of water
and wastewater conveayance and treatment systems + 1.5 year of
Teaching
- Academic Qualification:
• BE (Civil Engineering), NED University (2009)
• ME (Environmental Engineering), NED University + University of
Padua ,(2013)
- Current Affiliation:
• Doctoral Research Fellow at The University of Padua, Italy.
About Me
85. WHAT IS POLLUTION ?
• Some sort of contamination
• Unbalanced in the natural system
• Accumulation of something bad or
unwanted
86. POLLUTION, the other side of the Coin
POLLUTION is actually a RESOURCE in the WRONG
QUANTITY at the WRONG PLACE
An IDEA can change life
87. The Hypocrisy: (Fertilizer application)
Fertilizers contain:
• Plant Nutrients (Nitrate and Phosphates)
• Resource when applied in the field
• Becomes a pollutant when they infiltrate into the ground water
88. Definition of solid waste: Difficult !
“Waste is a left-over, a redundant product or material
of no or marginal value for the owner
and which the owner wants to discard”
Courtesy Prof.Christensen
•No universally accepted definition exists
92. The underestimated side :
Energy Potential from waste in Pakistan
The European Paradigm:
UK produces 28 million tones (around 77000 tones per day) of household waste every
year.. Currently, UK only 11% of this is utilized for energy production, producing, around
190MW, enough for 300,000 households.
Where we are standing:
• Only Karachi produce around 12000 tons/ day of solid waste out of which
• 20% is collected by the intermediate waste pickers,
• 20% is left on the streets at the mercy of nature and
• the rest (almost 60%) is picked up and dump in official and/or unofficial dustbins of the
city, then transported to the uphill areas located 30-35 km away from the city and
disposed in open air
• Apart from the Municipal waste the country has an enormous potential of recovering
energy through Anaerobic Digestion of agricultural waste, poultry waste, animal
manure etc.
(Nayyer Alam Zaigham, Proceedings of COMSATS Conference2004 on Renewable Energy Technologies & Sustainable
Development, 2005)
93. Quality is a problem!
And you about
landfill gas?
Do you know
anything about
parachutes?
94. Elementary Composition of MSW
1
Werte aus : NEUPERT, 1989, Stoffl. Zussammensetzung von Haus- u. Gewerbemüll
Bayr. Landesamt für Umweltschutz (Hrsg.): Zusammensetzung und Schadstoffgehalt von Siedlungsabfällen, 2003
Zeschmar- Lahl, 2003
Bidlingmeyer, 1990, Schwermetalle im Hausmüll
El Dawi, 1997, Vergleich der Müllzusammensetzungen in Abfallbehandlungsanlagen
2 Werte aus: Neumayer, 1999
Döberl, 2004
Substance Ratio 2
[% FS]
Lignin 6
Cellulose 16
Hemicellulose 7
Hydrocarbons 9
Proteins 3
Fats, Resins, Waxes 2
Paper additives (org.+anorg.) 8
Plastics 18
Plastic additives (anorg.) 3
Minerals 13
Ash 4
Hazardous substances 1
Metals 10
Summe 100
Microscopical picture of slag from
thermal waste treatment
Quelle: ise.uni-karlsruhe.de
Substance Ratio 1
[Gew.% FS]
Water 35 -37
Glass/Minerals 7- 11,2
O2 13,6
H2 2,4
C ges 20 - 22
Zn 0,04 - 0,3
Fe 2,8
Pb 0,011 - 0,063
Cd 0,0006 - 0,001
Hg 0,0004
Cu 0,024
Cr 0,0031 - 0,021
Mn 0,018
Ni 0,0024
Sn 0,002
Al 0,64
As 0,0007 - 0,0009
Ti 0,16
F 0,012
Cl 0,5
S 0,2
N 0,9
P 0,1
Na 0,5
K 0,4
Mg 0,3
Ca 2,1
95. eere.energy.gov
Biomass Composition and Degradability
Readily degradable
under anaerobic landfill
conditions
Slowly degradable under
anaerobic landfill conditionsPersistent under
anaerobic landfill
conditions
A hemicellulose can be
any of several different
heteropolymers (matrix
polysaccharides, most
pentose sugars) present
in almost all plant cell
walls along with cellulose.
Hemicellulose is a
branched polymer, while
cellulose is unbranched.
In contrast to cellulose
that is crystalline, strong,
and resistant to
hydrolysis, hemicellulose
has a random, amorphous
structure with little
strength.
500-3000 sugar units
7,000 - 15,000 glucose molecules
96. Lignin structure
Lignin is an organic substance binding
the cells, fibres and vessels which
constitute wood and the lignified
elements of plants. After cellulose, it is
the most abundant renewable carbon
source on Earth. It is not possible to
define the precise structure of lignin as
a chemical molecule. All lignins show a
certain variation in their chemical
composition. However the definition
common to all is a network polymer of
phenyl propene basic units.
102. Modern waste management strategy
• Waste production minimisation
• Efficient waste management
• Recovery of valuable material resources
• Global climate changes issues
• Reduction of landfilling
• Energy balance optimisation
• Emissions minimisation, ecotoxilogical control
• Health risk minimisation
• Environmental sustainability (long term impacts)
• Economical and social sustainability
Boh!!!
114. Waste Management
Traditional
• low population
• harmony with nature
Low amount of waste
Today
• explosion of population
• increasing standard of living
huge amount of waste
Traditional
methods
do not
fulfill
the new
requirements!
Himba-
People /
Namibia
Pictures: GEO 2001; Greenpeace, Smid 1996
Sao Paulo / Brasil
117. Global Warming
• Landfills are significant sources (6-
13% of global CH4 emission)
• CH4 more GWP than CO2 (28-34 from
2013 IPCC AR5 p714)
• Methane oxidation important
• Less organic waste in landfills in the
future
(TH Christensen)
118. Loss of Natural Resources
Loss of aestetics and landscaping
Water Contamination
Environmental
damages
AIT, Thailand
119. Collection of waste
in developing countries
- irregular
- not efficient
- not existing
In many cases:
Lixeira / Brasil
Thailand
Thailand Thailand
Kampala/ Uganda
Kampala/ Uganda
Kampala/ Uganda
Pakistan
121. Ampang Jaya Landfill Site (Kuala Lumpur)
Source: UPM, Malaysia, Dawn news paper
Disposal of collected waste
- dumps / landfills / open burning -
Jam Chakro (Karachi)
122. Disposal of waste –
if no collection system is existing
- open fires
- wild dumps
- dump in waterbodies
Ilhabela / Brasil
Pictures: Santen, 2000; Kraus 2001 and Dawn news paper
Kampala/ Uganda
Jam Chakro, Karachi
123. Health issues
Risk to community
Illness
Disease
- Breeding ground for vermin, insects and scavenging animals
chances of illness and disease
-waste pickers: contact with syringes, hospital wastes and other
hazardous waste
- Burning causes air pollution, and serious health effects
- Where these sites are located very close to densely populated
areas, or support substantial communities of waste pickers,
there are particular public health risks
124. Dumpsite Collapsed in Philippines
On 10 July 2000, more than 200 people died and hundreds more were
injured when the Payatas dumpsite in Quezon City, the Philippines,
collapsed in heavy rains. The collapse buried shanty homes of the
nation's poorest. Most of the victims were children, at home on a day
declared a holiday because of an impending typhoon.
Source: AIT, Thailand
1999: Shacks close to the mountain of
garbage which subsided
After the Collapse in July 2000 Payatas
dumpsite in Quezon City, Philippines
125. Waste as a resource
- Waste paper for new paper production
- Separated plastics for (like PE, PVC, PP) as a source
for new plastic production
- Mixed plastic and paper as an energy source (RDF)
- Metal recovery for new metal production (including
electronic waste)
- Kitchen and yard waste as soil conditioner
- Sewage sludge and agricultural waste as soil
conditioner or fuel
126. Waste as a resource
New products from waste
- organic waste as a source for the production of fuel,
CO2, CH4, alcohol)
- organic waste as a source for the production of food
for animals
- organic waste as a source for the production of e.g.
biodegradable plastic
127. Hierarchy of utilisation of waste
Direct recycling Downcycling
Actual material use Raw material use
(as a resource)
Material use Energetic use
(thermal use)
Utilisation for
136. What about the Organics/ Organic
Fraction of Municipal Solid waste /
Putrescible waste ?
137. Aerobic stabilisation: Composting
Biological degradation and transformation process for organic substances by
a variety of microbes, in aerobic conditions and in solid state. The process is
exergonic, results in heating up of the stabilizingmaterial, and it leads to the
formation of carbon dioxide and water. A humus rich material is generated.
Under specific quality control of the substrate and of the process the final product
may be classified as Compost: a stabilized and sanitised product which is
beneficial to plant growth.
138. Mechanism Of Biological Treatment?
Aerobic treatment is a biochemical process carried out in the
presence of O2 (dissolved). The process uses organic matter, nutrients,
and dissolved oxygen, and produces stable solids, carbon dioxide, and more
organisms.
Organic materials+ Nutrients +O2 CO2+NH3+New Cells
Aerobic microbes
Organics
O2
CO2
Nutrients
Stable
Solids
Growth
Microbes
139. Aims of Composting
Reduction of volume and mass of organic waste
Recirculation of organics into the natural cycle
Increasing of the Carbon Sink pool
Energy recovery (if anaerobic digestion is adopted as a
treatment before composting)
Stabilisation and hygienization of organic waste as a
pretreatment before landfilling
Fulfilment of regulations and laws
144. • Zero waste is a new planning
approach for the 21st Century that
seeks to redesign the way resources
and materials flow through society,
taking a ‘whole system’ approach
(Zero waste kuvalum, 2004).
• Zero waste maximises recycling,
minimises waste, reduces
consumption and ensures that
products are made to be reused,
repaired or recycled back into nature
or the market place (Grass Roots
Recycling Network, 2004).
(Cristina Trois, 2008)
Zero waste option
145. Zero waste perspectives
Zero waste
• Waste minimisation
• Personal behaviour
• Education
• Composting, MBT
• Thermal treatment
• Landfilling
Zero illness
• Prevention
• Personal behaviour
• Education
• Medicine
• Surgeries
• Graveyards
147. E: extracted raw material
ΔR: recycled and reused material (secondary raw materials)
ΔL: recovered material from landfill mining (secondary raw materials)
di: diffuse mass emissions/loss associated to the specific steps and
processes
I: immobilized material. (inert material)
The Concept of Urban Mining
148. Dispersion of Materials with Time
Raw Material Dispersed Material
100%
100%
Cycle of Utilization/Time
Raw Materials: i.e. steel, paints , textiles, tires, asphalt
Processes : i.e. corrosion, abrasion, dissolution, evaporation,
149. E = ∆R ∆L+ I∑di
Mass Balance: Flow of Resources
+ +
Sustainability and Urban Mining
The diffuse emissions should be carefully controlled and minimised as
they are the cause for the progressive deterioration of the global
environmental quality.
E= ∆R ∆L- I∑di - -
• Minimise raw material extraction
• Maximize recovery, recycling and reuse of secondary raw
materials
• Increase the immobilisation of materials in final sinks/geological
repositories
152. Mechanism Of Biological Treatment?
Anaerobic treatment is a biochemical process carried out in the
absence of O2 for the stabilization of organic materials by conversion
to CH4 and inorganic end-products such as CO2 and NH3
Organics
Nutrients
Growth
Stable
Solids
CO2 CH4+
Microbes
Energy Value:
Methane can be
used as fuel
Organic materials+ Nutrients CH4+CO2+NH3+New Cells
Anaerobic microbes
153. Biodegradation of organic waste: Process choice
green waste
rural biowaste
municipal biowaste
kitchen waste
food waste
restaurant waste
slaughterhouse waste
sewage sludge
slurry
Composting Digestion
Moisture
Structure
159. By definition a sanitary landfill is:
• a fully engineered disposal option.
• It avoids the harmful effects of uncontrolled dumping by
• spreading,
• compacting and
• Covering the waste on land that has been carefully
engineered before use.
• Through careful site selection, preparation and management,
operators can minimize risks from leachate and gas production
both in the present and the future.
• Site design and plans consider not only waste disposal but
aftercare and ultimate land use once the site closes
Sanitary landfill
161. Objectives
To prevent or reduce as far as possible
negative effects from the landfilling of
waste on
• the environment
• the global environment
• human health
162. LANDFILL TYPE
1. Mound
leachate migration by gravity out
of the landfill (long term)
long term landfill identification
2. Pit
closer to groundwater
leachate control more difficult
(eternal pumping)
side walls to be lined (avoiding
gas and leachate migration)
163. Concept I
• Open dump
– High impact during operation
• Dry tomb landfilling
– No air in landfill body
→Anaerobic degradation
– No water, no leachate
→Very low organic waste degradation
(mummification)
→Long term impacts due to high organic content in
landfill body
164. Concept II
• Contained landfill (today design)
– Controll of biogas and leachate emissions by physical
barriers (what will happen when they loose
efficiency?)
– Some lined landfill could became dry tomb – it
depends on top cover and the allowance of leachate
recirculation
• Sustainable landfill (tomorrow design)
– Waste pre-treatment
– Aerobic landfilling
– Open cover
– High ratio Liquid/Solid
167. Long term landfill impact
Open dump
Dry tomb landfill
Contained landfill
Sustainable landfill
time
OPERATION
ea
e30
300
AFTERCARE
tc
emax
I
II
III
169. amino acids,
saccharid, glycerin,
fatty acids
Anaerobic Processes (Contained Landfills)
fractions and
solved polymeres
protein
carbohydrate
fat
H2
alcohol
CO2
acetic acid
Biogas
CH4, CO2
organic acids
Hydrolysis Acidification Acetogenic
phase
Methane formation
H2
CO2
acetic acid
propionic acid,
butyric acid
Complex &
Particulate
OM
170. • Particulates made soluble and large polymers
converted to simpler monomers
– Carbohydrates, fats, and proteins
• Large molecules (polymers) broken down into
smaller molecules (monomers)
– Allow passage through bacterial cell wall
• Facultative anaerobes and anaerobes
• May be rate limiting step in process for high
concentrations of particulate organic matter.
Step 1: Hydrolysis
171. Molecule composed of
fatty acids and alcohols
R — C
O — H
O
R — C
O — H
O
Fatty Acids: Long-chain hydrocarbon
molecule capped by a carboxyl group
(COOH)
O
C
H — CH — CH — CH — H
O
R
O
C
O
R
O
C
O
R
H — CH — CH — CH — H
O
R
O
C
O
R
O
C
O
R
O
C
O
R
O
C
O
R
Fats (Lipids)
Protein
A macromolecule (polymer)
C — C
O — H
O
—
NH2
H
R
amino acid
C — C
O — H
O
—
NH2
H
R C — C
O — H
O
—
NH2
H
R
amino acid
C — C
O — H
O
—
NH2
H
R — N — C — C
O
H H
R’
peptide bond
C — C
O — H
O
—
NH2
H
R — N — C — C
O
H H
R’
peptide bond
Step 1: Hydrolysis (Examples)
172. Step 2: Acidogenesis
• Glucose, amino acids,
and fatty acids converted
to C3 and C4 volatile fatty
acids (76%), H2 (4%), and
acetic acid (20%)
• Optimum growth rate
occurs near pH 6
• Volatile fatty acids
generally not significant
consumer of alkalinity
• NH3 produced from
amino acids
Volatile Fatty Acids
"short-chain" or volatile fatty acids are 2 to
4-carbon molecules
CH3 — C
O — H
O
CH3 — C
O — H
O
ethanoic acid
(acetic acid / vinegar)
propionic acid
CH3 — CH2 — C
O — H
O
CH3 — CH2 — C
O — H
O
O — H
butanonic acid
(butyric acid)
CH3 — CH2 — CH2 — C
O
butanonic acid
(butyric acid)
CH3 — CH2 — CH2 — C
O
173. Step 3: Acetogenesis
Example:
C2H5OH + H2O acetate (CH3COO-) + H+ + 2H2
Go' = +9.6 kJ/mol
• Volatile fatty acids converted to acetic acid
(68%) and H2 (32%)
• Sensitive to H2 concentration
• Syntrophic (mutually beneficial) relationship with
the methanogens
174. Step 4: Methanogenesis
• Obligate anaerobes – methanogens
– Tend to have slower growth rates
• H2 utilizing methanogens use H2 to produce
methane removing H2 from system
• Limited pH range 6.7 to 7.4
– importance of alkalinity in system
• Sensitive to temperature change
175. Mechanisms of Methane Formation
2. Reduction of carbon dioxide CO2 + 4H2 => CH4 + 2H2O
1. Splitting of acetic acid CH3COOH => CH4 + CO2
Acetotrophic methanogens
4 CH3COOH 4 CO2 + 2 H2
Methylotrophic methanogens
4 CH3OH + 6 H2 3 CH4 + 2 H2O
Hydrogenotrophic methanogens
CO2 + 4 H2 CH4 + 2 H2O
1.
2.
176. Sample Methane Yield, m3
/kg VS
Mixed MSW 0.186 - 0.222
Mixed Yard Waste 0.143
Office Paper 0.369
Newsprint 0.084
Magazine 0.203
Food Board 0.343
Milk Carton 0.318
Wax Paper 0.341
*
From Owens, J.M. and D.P. Chynoweth
Biogas Potentials of Different Materials
179. Leachate is a wastewater produced by the infiltration of water in
the landfill.
The water percolating through the waste removes organic
compounds, metals and salts.
The QUALITY of the leachate depends on:
• the quality and type of the waste (MSW, Industrial waste,
bottom ashes).
• it depends by the conditions of the degradation of waste
in the landfill (anaerobic condition, aerobic conditions,
semi-aerobic condtions)
• and finally it depends by the age of the landfill (new
landfill or old landfill).
What is leachate?
180. The QUANTITY of leachate depends on:
• Characteristics of the site
• Climatic & meteorological conditions of the site
• Physical characteristics of the waste
• Characteristics of the barrier systems
What is leachate?
183. Leachate management options
• A. In situ : recirculation
• B. On site: leachate treatment plant
• C. Off site: co-treatment at external
facilities (industrial or domestic)
C
A B
C
184. Selection criteria for treatment
Young Medium Old
COD (mg/l) > 10.000 500-10.000 < 500
COD/TOC 2,7 2,0-2,7 2,0
BOD5/COD > 0,4 0,1-0,4 < 0,1
Biological treatment
Chemical precipitation
Ozone
Reverse osmosis
Activated carbon
Ion exchange
good good-fair fair fair-poor poor
186. 2nd Barriere = quality of the site
3rd Barriere = landfill concept
Multi Barrier Concept
1st Barrier = quality of the waste
4th Barrier = landfill drainage & liner
187. Landfill siting
The following criteria have to be respected in the course
of landfill siting:
Geological barrier: thickness > 3 m with kf < 1*10-7 m/s
Groundwater: Baseline of the liner 1m above the highest
groundwater table, soil should have a low permeability
No drinking water catchment area, no nature conservation
areas, no floading areas
> 300 m distance to residential areas, appropriate traffic
location
193. Today
Evolution of the Solar System
Evolution of Life on Earth
Evolution of Life on Earth
Periodic Extinctions
194. Evolution of the Solar System
The standard model for the formation of the Solar System (including the Earth)
is the solar nebula hypothesis.
In this model, the Solar system formed from a large, rotating cloud of
interstellar dust and gas called the solar nebula.
It was composed of hydrogen and helium created shortly after the Big Bang
13.8 Ga (billion years ago) and heavier elements ejected by supernovae.
About 4.5 Ga, the nebula began a contraction that may have been triggered by
the shock wave of a nearby supernova.
A shock wave would have also made the nebula rotate.
As the cloud began to accelerate, its angular momentum, gravity and inertia
flattened it into a protoplanetary disk perpendicular to its axis of rotation.
Small perturbations due to collisions and the angular momentum of other large
debris created the means by which kilometer-sized protoplanets began to form,
orbiting the nebular center.
195. The center of the nebula, not having much angular momentum,
collapsed rapidly.
The compression heating it until nuclear fusion of hydrogen into
helium began.
After more contraction, aTTauri star ignited and evolved into the
Sun.
The solar wind of the newly formedTTauri star cleared out most
of the material in the disk that had not already condensed into
larger bodies.
The same process is expected to produce accretion disks around
virtually all newly forming stars in the universe, some of which
yield planets
196. In the outer part of the nebula, gravity caused matter to
condense around density perturbations and dust particles.
The rest of the protoplanetary disk began separating into
rings.
Successively larger fragments of dust and debris clumped
together to form planets (called runaway accretion)
197. Earth formed in this manner about 4.54 billion years ago
(with an uncertainty of 1%) and was largely completed
within 10–20 million years
The proto-Earth grew by accretion until its interior was hot
enough to melt the heavy, siderophile metals.
Having higher densities than the silicates, these metals sank.
This so-called iron catastrophe resulted in the separation of a
primitive mantle and a (metallic) core
Only 10 million years after the Earth began to form,
producing the layered structure of Earth and setting up the
formation of Earth's magnetic field.
199. Evolution of Life on Earth
Biologists reason that all living organisms on Earth must
share a single universal ancestor.
The earliest organisms fossil is available of bacteria.
The lack of fossil or geochemical evidence for earlier
organisms has left plenty of scope for hypotheses.
Two main groups:
1) that life arose spontaneously on Earth or
2) that it was "seeded" from elsewhere in the Universe
200. Life "seeded" from elsewhere
There are three main versions of the "seeded from
elsewhere" hypothesis:
from elsewhere in our Solar System via fragments knocked into
space by a large meteor impact, in which case the most credible
sources are Mars andVenus;
by alien visitors, possibly as a result of accidental contamination
by microorganisms that they brought with them;
and from outside the Solar System but by natural means.
Greek philosopher Anaximander, physical chemist Svante
Arrhenius, astronomers Fred Hoyle and Chandra
Wickramasinghe, and by molecular biologist Francis Crick
and chemist Leslie Orgel.
201. Independent emergence on Earth
Life on Earth is based on carbon and water. Carbon provides
stable frameworks for complex chemicals and can be easily
extracted from the environment, especially from carbon
dioxide
Water is an excellent solvent
Research on how life might have emerged from non-living
chemicals focuses on three possible starting points:
self-replication, an organism's ability to produce offspring that
are very similar to itself;
metabolism, its ability to feed and repair itself; and
external cell membranes, which allow food to enter and waste
products to leave, but exclude unwanted substances
203. Evolution of Life on Earth
Timeline of evolution of life represents the current scientific
theory outlining the major events during the development
of life on planet Earth.
In biology, evolution is any change across successive
generations in the heritable characteristics of biological
populations.
Evolutionary processes give rise to diversity at every level of
biological organization, from kingdoms to species, and
individual organisms and molecules, such as DNA and
proteins.
204. Basic Timeline
In its 4.6 billion years circling the Sun, the Earth has harbored an
increasing diversity of life forms:
1. for the last 3.6 billion years, simple cells (prokaryotes);
2. for the last 3.4 billion
years, cyanobacteria performing photosynthesis;
3. for the last 2 billion years, complex cells (eukaryotes);
4. for the last 1.2 billion years, eukaryotes which sexually
reproduce
5. for the last 1 billion years, multicellular life;
6. for the last 600 million years, simple animals;
7. for the last 550 million years, bilaterians, water life forms with a
front and a back;
8. for the last 500 million years, fish and proto-amphibians;
9. for the last 475 million years, land plants;
205. Basic Timeline
10. for the last 400 million years, insects and seeds;
11. for the last 360 million years, amphibians;
12. for the last 300 million years, reptiles;
13. for the last 200 million years, mammals;
14. for the last 150 million years, birds;
15. for the last 130 million years, flowers;
16. for the last 60 million years, the primates,
17. for the last 20 million years, the family Hominidae (great apes);
18. for the last 2.5 million years, the genus Homo (including
humans and their predecessors);
19. for the last 250,000 years, anatomically modern humans.
207. Periodic Extinctions
Periodic extinctions have temporarily reduced diversity,
eliminating:
2.4 billion years ago, many obligate anaerobes (Obligate
anaerobes are poisoned by oxygen), in the Great
Oxygenation Event;
252 million years ago, the trilobites (Trilobites (3 lobes) are
a fossil group of extinct marine arthropods that form the
class Trilobita.), in the Permian–Triassic extinction event;
65 million years ago, the pterosaurs (Pterosaurs ("winged
lizard") were the earliest vertebrates flying reptiles known
to have evolved powered flight and of order Pterosauria.
Pterosaurs), non-avian dinosaurs, in the Cretaceous–
Paleogene extinction event.
231. TAZ/NED/Fall2015En501/20150822/v1
Handout
Accretion In astrophysics, accretion is the growth of particles into a massive object by
gravitationally attracting more matter, typically gaseous matter in an accretion
disc.
This attracted matter accelerates the growth of the particles into boulder-sized
planetesimals. The more massive planetesimals accrete some smaller ones, while
others shatter in collisions.
Some dynamics in the disc are necessary to allow orbiting gas to lose angular
momentum and fall onto the central massive object. Occasionally, this can result
in stellar surface fusion.
accretion disc An accretion disk is a structure (often a circumstellar disk) formed by diffused
material in orbital motion around a massive central body. The central body is
typically a star.
Gravity causes material in the disc to spiral inward towards the central body.
Gravitational and frictional forces compress and raise the temperature of the
material causing the emission of electromagnetic radiation.
The frequency range of that radiation depends on the central object's mass.
Accretion discs of young stars and protostars radiate in the infrared; those around
neutron stars and black holes in the X-ray part of the spectrum.
The study of oscillation modes in accretion discs is referred to as diskoseismology
Big Bang The Big Bang theory is the prevailing cosmological model for the universe from
the earliest known periods through its subsequent large-scale evolution.
It states that the universe expanded from a very high density state
The Big Bang theory offers a comprehensive explanation for a broad range of
observed phenomena, including the abundance of light elements, the cosmic
microwave background, large scale structure, and Hubble's Law. The framework
for the Big Bang model relies on Albert Einstein's theory of general relativity and
on simplifying assumptions such as homogeneity and isotropy of space.
circumstellar disk A circumstellar disk is a torus, pancake or ring-shaped accumulation of matter
composed of gas, dust, planetesimals, asteroids or collision fragments in orbit
around a star. Around the youngest stars, they are the reservoirs of material out
of which planets may form. Around mature stars, they indicate that planetesimal
formation has taken place and around white dwarfs, they indicate that planetary
material survived the whole of stellar evolution. Such a disk can manifest itself in
various ways.
Herbig Ae/Be star A Herbig Ae/Be star (HABe) is a pre-main-sequence star – a young (<10Myr) star
of spectral types A or B. These stars are still embedded in gas-dust envelopes and
are sometimes accompanied by circumstellar disks.
They are 2-8 Solar mass (M☉) objects
Hydrogen and calcium emission lines are observed in their spectra
Luminosity In astronomy, luminosity is the total amount of energy emitted by a star, galaxy,
or other astronomical object per unit time.
It is related to the brightness, which is the luminosity of an object in a given
spectral region.
Milky Way The Milky Way is the galaxy that contains our Solar System.
Its name "milky" is derived from its appearance as a dim glowing band arching
across the night sky whose individual stars cannot be distinguished by the naked
eye.
232. TAZ/NED/Fall2015En501/20150822/v1
The Milky Way is a barred spiral galaxy that has a diameter usually considered to
be roughly 100,000–120,000 light-years but may be 150,000–180,000 light-years.
The Milky Way is estimated to contain 100–400 billion stars, although this number
may be as high as one trillion.
There are probably at least 100 billion planets in the Milky Way.
The Solar System is located within the disk, about 27,000 light-years from the
Galactic Center, on the inner edge of one of the spiral-shaped concentrations of
gas and dust called the Orion Arm.
Nebula A nebula (Latin for "cloud";[2] pl. nebulae, nebulæ, or nebulas) is an interstellar
cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a
name for any diffuse astronomical object, including galaxies beyond the Milky
Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda
Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature
of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin
Hubble and others.
pre-main sequence
stars
A pre-main-sequence star (also known as a PMS star and PMS object) is a star in
the stage when it has not yet reached the main sequence.
A protostar grows by accretion, acquiring mass from its surrounding envelope of
interstellar dust and gas. By the time it is visible, the main accretion phase has
ended and it has acquired virtually all of its mass but has not yet started hydrogen
burning (i.e. nuclear fusion of hydrogen). The end of the main accretion phase to
the start of hydrogen burning (i.e. zero age main sequence) is the pre-main
sequence stage.
Protoplanetary disk A protoplanetary disk is a rotating circumstellar disk of dense gas surrounding a
young newly formed star, a T Tauri star, or Herbig Ae/Be star.
The protoplanetary disk may also be considered an accretion disc for the star
itself, because gasses or other material may be falling from the inner edge of the
disk onto the surface of the star. But this process should not be confused with the
accretion process thought to build up the planets themselves.
Protoplanets Protoplanets are large planetary embryos that originate within protoplanetary
discs and have undergone internal melting to produce differentiated interiors.
runaway accretion
Siderophile Siderophile (from sideron, "iron", and philia, "love") elements are the high-density
transition metals which tend to sink into the core because they dissolve readily in
iron either as solid solutions or in the molten state.
The siderophile elements include gold, cobalt, iron, iridium, manganese,
molybdenum, nickel, osmium, palladium, platinum, rhenium, rhodium and
ruthenium.
Stars vs planets
Stellar relating to a star or stars
supernova remnant This shock wave sweeps up an expanding shell of gas and dust called a supernova
remnant.
Supernovae A supernova is a stellar explosion that briefly outshines an entire galaxy, radiating
as much energy as the Sun or any ordinary star is expected to emit over its entire
life span, before fading from view over several weeks or months.
233. TAZ/NED/Fall2015En501/20150822/v1
The extremely luminous burst of radiation expels much or all of a star's material
at a velocity of up to 30,000 km/s (10% of the speed of light), driving a shock wave
into the surrounding interstellar medium.
This shock wave sweeps up an expanding shell of gas and dust called a supernova
remnant.
Supernovae are potentially strong galactic sources of gravitational waves
Supernovae are more energetic than novae. Nova means "new" in Latin, referring
to what appears to be a very bright new star shining in the celestial sphere; the
prefix "super-" distinguishes supernovae from ordinary novae, which are far less
luminous.
Supernovae can be triggered in one of two ways: by the sudden re-ignition of
nuclear fusion in a degenerate star; or by the gravitational collapse of the core of
a massive star
The last directly observed supernova in the Milky Way was Kepler's Star of 1604
(SN 1604); remnants of two more recent supernovae have been found
retrospectively
T Tauri star T Tauri stars (TTS) are a class of variable stars named after their prototype – T
Tauri. They are found near molecular clouds and identified by their optical
variability and strong chromospheric lines. T Tauri stars are pre-main sequence
stars in the process of contracting to the main sequence along the Hayashi track, a
luminosity-temperature relationship obeyed by infant stars of less than 3 solar
masses (M☉) in the pre-main-sequence phase of stellar evolution.
234. HANDOUT-Timeline of natural history
In the earliest solar system history, the Sun, the planetesimals and the jovian planets were formed.
The inner solar system aggregated more slowly than the outer, so the terrestrial planets were not yet
formed, including Earth and Moon.
c. 4,570 Ma: A supernova explosion (known as the primal supernova) seeds our galactic
neighborhood with heavy elements that will be incorporated into the Earth, and results in
a shock wave in a dense region of the Milky Way galaxy. The Ca-Al-rich inclusions, which
formed 2 million years before the chondrules,[1]
are a key signature of a supernova explosion.
4,567±3 Ma: Rapid collapse of hydrogen molecular cloud, forming a third-generation Population
I star, the Sun, in a region of the Galactic Habitable Zone(GHZ), about 25,000 light years from
the center of the Milky Way Galaxy.[2]
4,566±2 Ma: A protoplanetary disc (from which Earth eventually forms) emerges around the
young Sun, which is in its T Tauri stage.
4,560–4550 Ma: Proto-Earth forms at the outer (cooler) edge of the habitable zone of the Solar
System. At this stage the solar constant of the Sun was only about 73% of its current value, but
liquid water may have existed on the surface of the Proto-Earth, probably due to the greenhouse
warming of high levels ofmethane and carbon dioxide present in the atmosphere. Early
Bombardment Phase begins: because the solar neighbourhood is rife with large planetoids and
debris, Earth experiences a number of giant impacts that help to increase its overall size
Hadean Eon[edit]
4,533 Ma: Hadean Eon, Precambrian Supereon and unofficial Cryptic era start as the Earth–
Moon system forms, possibly as a result of a glancing collision between proto–Earth and the
hypothetical protoplanet Theia. (The Earth was considerably smaller than now, before this
impact.) This impact vaporized a large amount of the crust, and sent material into orbit around
Earth, which lingered as rings, similar to those of Saturn, for a few million years, until they
coalesced to become the Moon. The Moon geology pre-Nectarian period starts. Earth was
covered by a magmatic ocean 200 kilometres (120 mi) deep resulting from the impact energy
from this and other planetesimals during the early bombardment phase, and energy released by
the planetary core forming. Outgassing from crustal rocks gives Earth a reducing atmosphere
of methane, nitrogen, hydrogen, ammonia, and water vapour, with lesser amounts of hydrogen
sulfide, carbon monoxide, then carbon dioxide. With further full outgassing over 1000–1500 K,
nitrogen and ammonia become lesser constituents, and comparable amounts of methane,
carbon monoxide, carbon dioxide, water vapour, and hydrogen are released.
235. 4,500 Ma: Sun enters main sequence: a solar wind sweeps the Earth-Moon system clear of
debris (mainly dust and gas). End of the Early Bombardment Phase.Basin Groups Era begins on
Earth
4,450 Ma: 100 million years after the Moon formed, the first lunar crust, formed of
lunar anorthosite, differentiates from lower magmas. The earliest Earth crust probably forms
similarly out of similar material. On Earth the pluvial period starts, in which the Earth's crust
cools enough to let oceans form.
4,300 Ma: Nectarian Era begins on Earth
4,404 Ma: First known mineral, found at Jack Hills in Western Australia. Detrital zircons show
presence of a solid crust and liquid water. Latest possible date for a secondary atmosphere to
form, produced by the Earth's crust outgassing, reinforced by water and possibly organic
molecules delivered by comet impacts andcarbonaceous chondrites (including type CI shown to
be high in a number of amino acids and polycyclic aromatic hydrocarbons (PAH)).
4,250 Ma: Earliest evidence for life, based on unusually high amounts of light isotopes of
carbon, a common sign of life, found in Earth's oldest mineral deposits located in the Jack
Hills of Western Australia.[3]
4,100 Ma: Early Imbrian Era begins on Earth. Late heavy bombardment of the Moon (and
probably of the Earth as well) by bolides and asteroids, produced possibly by the planetary
migration of Neptune into the Kuiper belt as a result of orbital
resonances between Jupiter and Saturn.[4]
4,030 Ma: Acasta Gneiss of Northwest Territories, Canada, first known oldest rock, or aggregate
of minerals.
Archean Eon[edit]
Main article: Archean
Eoarchean Era[edit]
Main article: Eoarchean
4,000 Ma: Archean Eon and Eoarchean Era start. Possible first appearance of plate tectonic
activity in the Earth's crust as plate structures may have begun appearing. Possible beginning
of Napier Mountains Orogeny forces of faulting and folding create first metamorphic rocks.
Origins of life.
3,930 Ma: Possible stabilization of Canadian Shield begins
3,920–3,850 Ma: Final phase of Late Heavy Bombardment
3,850 Ma: Greenland apatite shows evidence of 12
C enrichment, characteristic of the presence of
photosynthetic life.[5]
236. 3,850 Ma: Evidence of life: Akilia Island graphite off Western Greenland contains evidence
of kerogen, of a type consistent with photosynthesis.[citation needed]
3,800 Ma: Oldest banded iron formations found.[citation needed]
. First complete continental masses
or cratons, formed of granite blocks, appear on Earth. Occurrence of initial felsic igneous activity
on eastern edge of Antarctic craton as first great continental mass begins to coalesce. East
European Craton begins to form - first rocks of the Ukrainian Shield and Voronezh Massif are
laid down
3,750 Ma: Nuvvuagittuq Greenstone Belt forms
3,700 Ma: Graphite found to be biogenic in 3.7 billion-year-old metasedimentary
rocks discovered in Western Greenland[6]
Stabilization of Kaapval cratonbegins: old tonaltic
gneisses laid down
Paleoarchean Era[edit]
3,600 Ma: Paleoarchean Era starts. Possible assembly of the Vaalbara supercontinent: Oldest
cratons on Earth (such as the Canadian Shield, East European Craton and Kaapval) begin
growing as a result of crustal disturbances along continents coalescing into Vaalbara - Pilbara
Craton stabilizes. Formation ofBarberton greenstone belt: Makhonjwa Mountains uplifts on the
eastern edge of Kaapval craton, oldest mountains in Africa - area called the "genesis of life" for
exceptional preservation of fossils. Narryer Gneiss Terrane stabilizes: these gniesses become
the "bedrock" for the formation of the Yilgarn Craton in Australia - noted for the survival of
the Jack Hills where the oldest mineral, a zircon was uncovered
3,500 Ma: Lifetime of the last Universal ancestor: split between bacteria and archaea occurs as
"tree of life" begins branching out - varieties of Eubacteria begin to radiate out globally. Fossils
resembling cyanobacteria, found at Warrawoona, Western Australia.[citation needed]
3,480 Ma: Fossils of microbial mat found in 3.48 billion-year-old sandstone discovered
in Western Australia.[7][8]
First appearance of stromatolitic organisms that grow
at interfaces between different types of material, mostly on submerged or moist surfaces
3,460 Ma: Fossils of bacteria in chert.[citation needed]
Zimbabwe Craton stabilizes from the suture of
two smaller crustal blocks, the Tokwe Segment to the south and the Rhodesdale Segment or
Rhodesdale gneiss to the north
3.400 Ma: Eleven taxa of prokaryotes are preserved in the Apex Chert of the Pilbara craton in
Australia. Because chert is fine-grained silica-rich microcrystalline,cryptocrystalline or
microfibrious material, it preserves small fossils quite well. Stabilization of Baltic Shield begins
3.340 Ma: Johannesburg Dome forms in South Africa: located in the central part of Kaapvaal
Craton and consists of trondhjemitic and tonalitic granitic rocks intruded into mafic-ultramafic
greenstone - the oldest granitoid phase recognised so far.
237. 3,300 Ma: Onset of compressional tectonics[9]
Intrusion of granitic plutons on the Kaapvaal
Craton
3,260 Ma: One of the largest recorded impact events occurs near the Barberton Greenstone
Belt, when a 58 km (36 mi) asteroid leaves a hole almost 480 km (300 mi) across – two and a
half times larger in diameter than the Chicxulub crater.[10]
Mesoarchean Era[edit]
3,200 Ma: Mesoarchean Era starts. Onverwacht series in South Africa form - contain some of
the oldest microfossils mostly spheroidal and carbonaceous alga-like bodies
3,200–2600 Ma: Assembly of the Ur supercontinent to cover between 12–16% of the
current continental crust. Formation of Limpopo Belt
3.1 Ma: Fig Tree Formation: second round of fossilizations including Archaeosphaeroides
barbertonensis and Eobacterium. Gneiss and greenstone belts in the Baltic Shield are laid down
in Kola Peninsula, Karelia and northeastern Finland
3 Ma: Humboldt Orogeny in Antarctica: possible formation of Humboldt Mountains in Queen
Maud Land. Photosynthesizing cyanobacteria evolve; they use water as a reducing agent,
thereby producing oxygen as a waste product. The oxygen initially oxidizes dissolved iron in the
oceans, creating iron ore - over time oxygen concentration in the atmosphere slowly rises, acting
as a poison for many bacteria. As Moon is still very close to Earth and causes tides 1,000 feet
(305 m) high, the Earth is continually wracked by hurricane-force winds - these extreme mixing
influences are thought to stimulate evolutionary processes. Rise ofStromatolites: microbial mats
become successful forming the first reef building communities on Earth in shallow warm tidal
pool zones (to 1.5 Gyr). Tanzania Craton forms
2.940 Ma: Yilgarn Craton of western Australia forms by the accretion of a multitude of formerly
present blocks or terranes of existing continental crust
2,900 Ma: Assembly of the Kenorland supercontinent, based upon the core of the Baltic shield,
formed at 3100 Ma. Narryer Gniess Terrane (including Jack Hills) of Western Australia
undergoes extensive metamorphism
Neoarchean Era[edit]
2,800 Ma: Neoarchean Era starts. Breakup of the Vaalbara: Breakup of supercontinent Ur as it
becomes a part of the major supercontinent Kenorland. Kaapvaal and Zimbabwe cratons join
together
2,770 Ma: Formation of Hamersley Basin on the southern margin of Pilbara Craton - last stable
submarine-fluviatile environment between the Yilgarn and Pilbara prior to rifting, contraction and
assembly of the intracratonic Gascoyne Complex
2,750 Ma: Renosterkoppies Greenstone Belt forms on the northern edge of the Kaapvaal Craton
238. 2,736 Ma: Formation of the Temagami Greenstone Belt in Temagami, Ontario, Canada
2,707 Ma: Blake River Megacaldera Complex begins to form in present-
day Ontario and Quebec - first known Precambrian supervolcano - first phase results in creation
of 8km long, 40km wide, east-west striking Misema Caldera - coalescence of at least two large
mafic shield volcanoes
2,705 Ma: Major komatiite eruption, possibly global[9]
- possible mantle overturn event
2.704 Ma: Blake River Megacaldera Complex: second phase results in creation of 30 km long,
15 km wide northwest-southeast trending New Senator Caldera - thick massive mafic sequences
which has been inferred to be a subaqueous lava lake
2,700 Ma: Biomarkers of cyanobacteria discovered, together
with steranes (sterols of cholesterol), associated with films of eukaryotes, in shales located
beneath banded iron formation hematite beds, in Hamersley Range, Western
Australia[11]
Skewed sulfur isotope ratios found in pyrites shows a small rise in oxygen
concentration in the atmosphere[12]
Sturgeon Lake Caldera, forms in Wabigoon greenstone belt:
contains well perserved homoclinal chain of greenschist facies, metamorphosed intrusive,
volcanic and sedimentary layers - Mattabi pyroclastic flow considered third most voluminous
eruptive event. Stromatolites of Bulawayo series in Zimbabwe form: first verified reef community
on Earth. Skewed sulfur isotope ratios found in pyrites shows a small rise in oxygen
concentration in the atmosphere
2,696 Ma: Blake River Megacaldera Complex: third phase of activity constructs classic east-
northeast striking Noranda Caldera which contains a 7-to-9-km-thick succession of mafic and
felsic rocks erupted during five major series of activity. Abitibi greenstone belt in present-day
Ontario and Quebec begins to form: considered world's largest series of Archean greenstone
belts, appears to represent a series of thrusted subterranes
2,690 Ma: Formation of high pressure granulites in the Limpopo Central Region
2,650 Ma: Insell Orogeny: occurrence of a very-high grade discrete tectonothermal event (a
UHT metamorphic event)
2,600 Ma: Oldest known giant carbonate platform.[9]
Saturation of oxygen in ocean sediments is
reached as oxygen now begins to dramatically appear in Earth's atmosphere
Proterozoic Eon[edit]
Main article: Proterozoic
Paleoproterozoic Era[edit]
Main article: Paleoproterozoic
Siderian Period[edit]
239. 2,500 Ma: Proterozoic Eon, Paleoproterozoic Era, and Siderian Period start. Oxygen saturation
in the oceans is reached: Banded iron formations form and saturate ocean floor deposits -
without an oxygen sink, Earth's atmosphere becomes highly oxygenic. Great Oxygenation
Event led by cyanobacteria's oxygenic photosynthesis - various forms of Archaea and anoxic
bacteria become extinct in first great extinction event on Earth. Algoman Orogeny or Kenoran:
assembly of Arctica out of the Canadian Laurentian Shield and Siberian craton - formation
of Angaran Shield and Slave Province
2,440 Ma: Formation of Gawler Craton in Australia
2,400 Ma: Huronian glaciation starts, probably from oxidation of earlier methane greenhouse
gas produced by burial of organic sediments of photosynthesizers. First cyanobacteria.
Formation of Dharwar Craton in southern India
2,400 Ma: Suavjarvi impact structure forms. This is the oldest known impact crater whose
remnants are still recognizable. Dharwar Craton in southern India stabilizes
Rhyacian Period[edit]
2,300 Ma: Rhyacian period starts.
2,250 Ma: Bushveld Igneous Complex forms: world's largest reserves of platinum-group
metals (platinum, palladium, osmium, iridium, rhodium and ruthenium) as well as vast quantities
of iron, tin chromium titanium and vanadium appear - formation of Transvaal Basin begins
2,200–1800 Ma: Continental Red Beds found, produced by iron in weathered sandstone being
exposed to oxygen. Eburnean Orogeny, series of tectonic, metamorphic and plutonic events
establish Eglab Shield to north of West African Craton and Man Shield to its south - Birimian
domain of West Africa established and structured
2,200 Ma: Iron content of ancient fossil soils shows an oxygen built up to 5–18% of current
levels[13]
End of Kenoran Orogeny: invasion of Superior and Slave Provinces by basaltic dikes
and sills - Wyoming and Montana arm of Superior Province experiences intrusion of 5 km thick
sheet of chromite-bearing gabbroic rock as Stillwater Complex forms
2,100 Ma: Huronian glaciation ends. Earliest known eukaryote fossils found. Earliest
multicellular organisms collectively referred to as the "Gabonionta" (Francevillian Group
Fossil), Wopmay orogeny along western margin of Canadian Shield
2,090 Ma: Eburnean Orogeny: Eglab Shield experiences syntectonic trondhjemitic pluton
intrusion of its Chegga series - most of the intrusion is in the form of a plagioclase called
oligoclase
2.070 Ma: Eburnean Orogeny: asthenospheric upwelling releases large volume of post-orogenic
magmas - magma events repeatedly reactivated from the Neoproterozoic to the Mesozoic
Orosirian Period[edit]
240. 2,050 Ma: Orosirian Period starts. Significant orogeny in most continents.
2,023 Ma: Vredefort impact structure forms.
2,005 Ma: Glenburgh Orogeny (2,005–1,920 Ma) begins: Glenburgh Terrane in western
Australia begins to stabilize during period of substantial granite magmatism and deformation;
Halfway Gneiss and Moogie Metamorphics result. Dalgaringa Supersuite (2,005–1,985 Ma),
comprising sheets, dykes and viens of mesocratic and leucocratic tonalite, stabilizes.
2,000 Ma: The lesser supercontinent Atlantica forms. The Oklo natural nuclear
reactor of Gabon produced by uranium-precipitant bacteria.[14]
First acritarchs.
1,900 - 1,880 Ma: Gunflint chert biota forms flourishes including prokaryotes
like Kakabekia, Gunflintia, Animikiea and Eoastrion
1,850 Ma: Sudbury impact structure. Penokean orogeny. First eukaryotes. Bacterial viruses
(bacteriophage) emerge before, or soon after, the divergence of the prokaryotic and eukaryotic
lineages.[15]
1,830 Ma: Capricorn Orogeny (1.83 - 1.78 Gyr) stabilizes central and northern Gascoyne
Complex: formation of pelitic and psammitic schists known as Morrissey Metamorphics and
depositing Pooranoo Metamophics an amphibolite facies
Statherian Period[edit]
1,800 Ma: Statherian Period starts. Supercontinent Columbia forms, one of whose fragments
being Nena. Oldest ergs develop on several cratons[9]
Barramundi Orogeny (ca. 1.8 Gyr)
influences MacArthur Basin in Northern Australia.
1,780 Ma Colorado Orogeny (1.78 - 1.65 Gyr) influences southern margin of Wyoming craton -
collision of Colorado orogen and Trans-Hudson orogen with stabilized Archean craton structure
1,770 Ma Big Sky Orogeny (1.77 Gyr) influences southwest Montana: collision between Hearne
and Wyoming cratons
1,765 Ma As Kimban Orogeny in Australian continent slows, Yapungku Orogeny (1.765 Gyr)
begins effecting Yilgarn craton in Western Australia - possible formation of Darling Fault, one of
longest and most significant in Australia
1,760 Ma Yavapai Orogeny (1.76 - 1.7 Gyr) impacts mid to south western United States
1.750 Ma Gothian Orogeny (1.75 - 1.5 Gyr): formation of tonalitic-granodioritic plutonic rocks
and calc-alkaline volcanites in the East European Craton
1,700 Ma Stabilization of second major continental mass, the Guiana Shield in South America
1,680 Ma Mangaroon Orogeny (1.68 - 1.62 Gyr), on the Gascoyne Complex in Western
Australia: Durlacher Supersuite, granite intrusion featuring a northern (Minnie Creek) and
southern belt - heavily sheared orthoclase porphyroclastic granites
241. 1.650 Ma Kararan Orogeny (1.65 Gyr) uplifts great mountains on the Gawler Craton in Southern
Australia - formation of Gawler Range including picturesque Conical Hill Track and "Organ
Pipes" waterfall
Mesoproterozoic Era[edit]
Main article: Mesoproterozoic
Calymmian Period[edit]
1,600 Ma: Mesoproterozoic Era and Calymmian Period start. Platform covers expand. Major
orogenic event in Australia: Isan Orogeny (1,600 Ma) influences Mount Isa Block of Queensland
- major deposits of lead, silver, copper and zinc are laid down. Mazatzal Orogeny (1,600 Ma -
1,300 Ma) influences mid to south western United States: Precambrian rocks of the Grand
Canyon, Vishnu Schist and Grand Canyon Series, are formed establishing basement of Canyon
with metamorphosed gniesses that are invaded by granites
1,500 Ma: Supercontinent Columbia collapses: associated with continental rifting along western
margin of Laurentia, eastern India, southern Baltica, southeastern Siberia, northwestern South
Africa and North China Block - formation of Ghats Province in India First structurally
complex eukaryotes (Hododyskia, colonial formamiferian).
Ectasian Period[edit]
1,400 Ma: Ectasian Period starts. Platform covers expand. Major increase
in Stromatolite diversity with widespread blue-green algae colonies and reefs dominating tidal
zones of oceans and seas
1,300 Ma: Break-up of Columbia Supercontinent completed: widespread anorogenic magmatic
activity, forming anorthosite-mangerite-charnockite-granite suites in North America, Baltica,
Amazonia and North China - stabilization of Amazonian Craton in South America Grenville
orogeny(1,300 - 1,000 Ma) in North America: globally associated with assembly of
Supercontinent Rodinia establishes Grenville Province in Eastern North America - folded
mountains from Newfoundland to North Carolina as Old Rag Mountain forms
1,270 Ma Emplacement of Mackenzie granite mafic dike swarm - one of three dozen dike
swarms, forms into Mackenzie Large Igneous Province - formation of Copper Creek deposits
1,250 Ma Sveconorwegian Orogeny (1,250 Ma - 900 Ma) begins: essentially a reworking of
previously formed crust on the Baltic Shield
1,240 Ma Second major dike swarm, Sudbury dikes form in Northeastern Ontario around the
area of the Sudbury Basin
Stenian Period[edit]