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LESSON 2. Salient Features of the Sun

Sun- is the largest body in our solar
system.
- it is the nearest star to our
planet.
- it is only one of the many
billions of stars in the galaxy and a
typical main-sequence star.
Table 14.1: Data of the Sun
Distance

93 million miles

Diameter

864,400 miles

Volume

1,250,000 times greater than te earth

Mass

2 x 10 kg

Density

1.41 g/cm

Inclination

7 degrees - 10 degrees

Surface Temperature

6,000 degrees celsius

Equatorial

15,000,000 degrees celsius

Rotation Polar

Once every 33 days

Equatorial

Once every 25 days

Life span

11 billion years

Solar constant

1.94 calories/cm/min

Age

4.6 billion years

Type

Yellow dwarf
The Sun's Atmosphere
- the most familiar sight as we

observed the sun at early dawn or
during sunset.
- it consists of four layers:
photosphere, chromosphere,
corona, and reversing layers.
Photosphere
- is the light sphere and the main body of
the sun.
- this layer is 150 miles thick and with a
temperature of 6,000 degrees celsius.
- this layer of the sun is characterized
with various disturbances: granules,
faculae, and sunspots.
1. Granules- are bubbles of hot gases
that appear in cycles of bright and dark
spots reaching up to 621 miles.
2. Faculae- (small torches) are small, but
sharp eruptions which last for about 15
minutes to one hour.
3. Sunspots- are darker, cooler areas in
the atmosphere. They range size from
800 to 80,000 km in diameter.
Chromosphere
- is the color sphere.
- it extends from 5,000 to 8,000 miles
thick.
- when observed during total solar
eclipse or with the use of an
instrument.
- it appears in a rose pink in color.
- it also characterized with disturbances
also referred to as "storms".
• Solar Flares- are gigantic eruptions that
bombard the earth electromagnetic
waves (X-rays, gamma rays, ultraviolet
rays, infrared rays) and particles.
• they occur near sunspots and may
spread up to 100,000 miles or more in
space.
• The Electromagnetic waves reach Earth
eight minutes after the initial burst.
• These waves cause interference in
radio and telecommunication
operations.
• The particles are the protons and
electrons that are released from
hydrogen atoms that are shattered to
pieces.
- they are driven by the earth's
magnetic field to the southern and
northern hemisphere.
Aurora- the colliding with the particles of
our atmosphere, causing the formation
of brilliant displays of light.
- it is also purely electrical charges
that look like neon lights in the sky that
may last for days or weeks.
Prominences- are billowing arches of
rose-colored flame, which also occur
near sunspots.
- they may go up to about
500,000 to one million miles in space.
Corona- is the outer most layer of the
sun's atmosphere.
- this layer is also visible only
during solar eclipse.
- its shape varies with the elevenyear period of sunspots.
- its formed by the vapors emitted
by the bubbling gases in the
photosphere.
- the temperature of corona
ranges from 1 to 2 million degrees
celsius.
PLANETISIMAL THEORY
COMPANION STAR THEORY
NEBULAR HYPOTHESIS
Lesson 3: Characteristics of the Eight
Planets of the Solar System
• Eight planets revolve around the sun
with remarkable precision.
• Speed, Eccentricity and Distance from
the sun characterize the orbits of the
planets.
• Possibility of their crossing, allowing
collision of planets and satellites to
occur
- these are the numbers and variety of
orbits in the solar system suggest this
possibility.
• Mercury- has a small magnetic field.
• Venus and Mars- have very weak
magnetic fields.
• Earth- has a very significant magnetic
field.
• Jupiter- has a very large and strong
magnetic field.
• Warning process in the atmosphere of
Jupiter, Saturn, Uranus, and Neptune- is
much similar to that of the earth, but
their absorbing materials are different.
• Earth- is warmed by the heat
developed in the absorption of
ultraviolet rays by the ozone layer in
the atmosphere while the outer
planets are warmed by the heat
developed by the absorption of solar
radiation of methane and the smog of
some particles.
• Jupiter, Saturn, and Neptune- are
found to be emitting more heat than
they receive from the sun
• Planets- are grouped according to
size.
• Terrestrial planets- are small and
they have high densities due to
their bodies made up of rocks and
heavy elements.
• Mercury, Venus, Earth, And Marsare considered terrestrial planets.
• Jovian planets- are larger and
massive and they have low
densities and have dense
Characteristics of the Eight Planets of the Solar System
Number
of
Satellite

Distance from
the sun

Inclination

Rotation

MERCURY

58 million km

7 degrees
14 minutes

About 58.7
days

88 days

0

Heavily
cratered
planet

VENUS

67 million miles

3 degrees
39 minutes

243 days

225 days

o

Veiled planet

EARTH

93 million miles

23 degrees
30 minutes

24 hours

365 days

1

Blue planet

MARS

141,700,000 0
miles

25 degrees

1.37

1.88 years

2

Red planet

3 degrees

10 hours

19

Largest planet

23

Pale
yellow,ringed
planet

5

Bluish-green
with righs

2

Planet with a
clear
atmosphere

Planet

JUPITER

Revolution

SATURN

URANUS
NEPTUNE

1.79 billion miles

98 degrees
30 degrees

17.24 hours
14 hours

84 years
165 years

Description
Lesson 4. Asteroids, Comets, and
Meteors
• Asteroids- are small chunks of
irregularly shaped objects that occupy
the 350 million miles space between
Mars and Jupiter.
• They orbit the sun in a belt following
the same direction as those of the
planets.
- the asteroid belt range in size.
If all the asteroids were put together
they would form a body no more than
1,500 km in diameter.
• Their number is estimated to
be about 30,000 but only about
7,000 have been identified..
• They vary in size, shape,
color, and composition.
• A German astronomer Johan Bode
accidentically discovered the
existence of these miniature
planets in 1800.
• Ceres- is the largest asteroids, 940
km in diameter.

Giuseppe Piazzi discovered it
on January 1, 1801. Ceres was named
after
the
Roman
goddess
of
agriculture and also known as the
protecting goddess of Sicily.
 Pallas- is the second largest, 540 km
in diameter.
 Vesta- which is 510 km in diameter.
 About
500
other
asteroids
are
between 50 to 100 km in diameter
and the rest are smaller than 50 km.
3 types of asteroids as their color and
composition

• C-type asteroids- are very dark
and carbonaceous. There are
75% of known asteroids.
• S-type asteroids- are rusty red in
color and they are composed of
iron and magnesium silicate.
• M-type asteroids- are rich with
metallic substances.
3 types of asteroids according to
position:
1.Athensis
the
first
type
of
asteroids.They lie near the orbit of
Mars. Some examples are Ceres, Pallas,
Juno, and Vesta.
2.Apollosis
the
second
type
of
asteroids. They lie near Jupiter and
they have highly elliptical orbits.
Eros,
Geographos,
and
Icarus
are
examples. These asteroids constantly
cross the earth's orbit.

Icarus reached the earth about 6
million km.
 Geographos- reached the earth at a
distance of about 9 km.
 Eros- at about 485,000 miles.
3.Trojans- are the third type. They
lie within the main asteroid belt
and they circle the sun for 12
years.

Examples are Hector, Diomedes,
Agamemnon, and Petrocius.
COMETS
it is known since ancient times.
they were once associated to bad
omens and disaster.
Oort Cloud- comet originated
from a dense shell of material
surrounding the outer edge of
the solar system.
Jan Oort- Dutch Astronomer.
Comets- orbits are big and
• As they revolved around the
sun some can reach the outer
edge of the solar system and
then
back,
moving
closer
towards the sun.
• As they get closer to the sun,
they become very bright and
start forming a tail.
3 Basic Parts of Comets
1. NUCLEUS- which is believed to be
solid and composed of frozen gases,
water vapor, and dust particles.
2. COMA- a cloudlike structure that
surrounds the nucleus which is
composed of gas and small bits of
rocks and dust.
3. TAIL- that is composed of gas or
dust particles or both. Comets may
have one or several tails.
• When the comet is away from the
sun, it has no tail.
• Comets appear in the sky from time
to time.
• Some comets return on a cycle every
few years.
2 Groups of Comets according to their
order of appearance:
1. Short-period comets- have orbits
that take less than 200 years.
2. Long-period comets- have orbits
that take more than 200 years.
• Haley's comet appears every 76 years
.
• Edmund Haley- predicted its
appearance in 1910.
• The last time it reappeared was in
1986 and it is predicted to reappear
again in the year 2062.
• Kuiper Belt Objects(KBO)
- this is the name given to many
small bodies found orbiting the sun
from beyond Neptune and Pluto.
• Oort Cloud- is a theoretical, spherical
gathering of rocks at the outer edge
of the solar system.
• Meteors- are the bright streak of
light that dart the night sky which
are referred to as "shooting star".
• In reality meteors are "space debris"
or stray pieces of stony or metallic
rocks that pass through the earth's
atmosphere.
• Meteors travel in great speed that sometimes
exceeds 100,000 miles per hour.
• Friction with the earth's atmosphere caused
them to glow and vaporize completely in
space.
• Meteorites- the large ones reach the earth's
surface.
• Meteor shower- is a celestial event in which
a number of meteors are observed to radiate
from one point in the night sky.
- it is a regular sight sometime in the midmonth of
August because in this month Earth crosses the
path of comets and meteors are seen in the
Esrth's atmosphere.
Summary in lesson 2;
• The sun is the largest celestial body in the solar
system.It has a various characteristics.
• The sun's atmosphere is the most prominent
layer that we see in the sky. The solar
atmosphere
consists
of
four
layers:
Photosphere, Chromosphere, Reversing layer,
and Corona.
• The
photosphere
is
characterized
by
disturbances. The most familiar to us are the
sunspots.
• The chromosphere is likewise characterized by
disturbances. The solar flares are disturbances
that have profound effect on Earth's
atmosphere.
Summary in lesson 3:
• The planets are classified according
to size. The terrestrial planets are
Mercury, Venus, Earth, and Mars,
while Jovian Planets are Jupiter,
Saturn, Neptune, and Uranus.
• The eight planets differ in terms of
distance from the sun, rotation,
revolution,inclination,and number of
satellites.
Summary in lesson 4:
• Impact of asteroids larger than 500 meters on
the earth's surface can cause global
devastation. But this is an extremely rare
phenomenon.
• Astronomers consider all three celestial
objects as space debris.
• Comets have large and elliptical orbits and
return on a predictable cycle of few years.
• Asteroids are chunks of irregularly shaped
objects that occupy the space between Mars
and Jupiter.
• Meteors are stray pieces of objects that
appear in the night sky as shooting stars.
THANK YOU
GEMINI FOR
LISTENING!!!
"have a nice day
everyone"...

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Features of the Sun.

  • 1. LESSON 2. Salient Features of the Sun Sun- is the largest body in our solar system. - it is the nearest star to our planet. - it is only one of the many billions of stars in the galaxy and a typical main-sequence star.
  • 2. Table 14.1: Data of the Sun Distance 93 million miles Diameter 864,400 miles Volume 1,250,000 times greater than te earth Mass 2 x 10 kg Density 1.41 g/cm Inclination 7 degrees - 10 degrees Surface Temperature 6,000 degrees celsius Equatorial 15,000,000 degrees celsius Rotation Polar Once every 33 days Equatorial Once every 25 days Life span 11 billion years Solar constant 1.94 calories/cm/min Age 4.6 billion years Type Yellow dwarf
  • 3. The Sun's Atmosphere - the most familiar sight as we observed the sun at early dawn or during sunset. - it consists of four layers: photosphere, chromosphere, corona, and reversing layers.
  • 4. Photosphere - is the light sphere and the main body of the sun. - this layer is 150 miles thick and with a temperature of 6,000 degrees celsius. - this layer of the sun is characterized with various disturbances: granules, faculae, and sunspots.
  • 5.
  • 6. 1. Granules- are bubbles of hot gases that appear in cycles of bright and dark spots reaching up to 621 miles. 2. Faculae- (small torches) are small, but sharp eruptions which last for about 15 minutes to one hour. 3. Sunspots- are darker, cooler areas in the atmosphere. They range size from 800 to 80,000 km in diameter.
  • 7. Chromosphere - is the color sphere. - it extends from 5,000 to 8,000 miles thick. - when observed during total solar eclipse or with the use of an instrument. - it appears in a rose pink in color. - it also characterized with disturbances also referred to as "storms".
  • 8.
  • 9. • Solar Flares- are gigantic eruptions that bombard the earth electromagnetic waves (X-rays, gamma rays, ultraviolet rays, infrared rays) and particles. • they occur near sunspots and may spread up to 100,000 miles or more in space. • The Electromagnetic waves reach Earth eight minutes after the initial burst.
  • 10.
  • 11. • These waves cause interference in radio and telecommunication operations. • The particles are the protons and electrons that are released from hydrogen atoms that are shattered to pieces. - they are driven by the earth's magnetic field to the southern and northern hemisphere.
  • 12. Aurora- the colliding with the particles of our atmosphere, causing the formation of brilliant displays of light. - it is also purely electrical charges that look like neon lights in the sky that may last for days or weeks.
  • 13.
  • 14. Prominences- are billowing arches of rose-colored flame, which also occur near sunspots. - they may go up to about 500,000 to one million miles in space.
  • 15.
  • 16. Corona- is the outer most layer of the sun's atmosphere. - this layer is also visible only during solar eclipse. - its shape varies with the elevenyear period of sunspots. - its formed by the vapors emitted by the bubbling gases in the photosphere. - the temperature of corona ranges from 1 to 2 million degrees celsius.
  • 17.
  • 21. Lesson 3: Characteristics of the Eight Planets of the Solar System • Eight planets revolve around the sun with remarkable precision. • Speed, Eccentricity and Distance from the sun characterize the orbits of the planets. • Possibility of their crossing, allowing collision of planets and satellites to occur - these are the numbers and variety of orbits in the solar system suggest this possibility.
  • 22. • Mercury- has a small magnetic field. • Venus and Mars- have very weak magnetic fields. • Earth- has a very significant magnetic field. • Jupiter- has a very large and strong magnetic field. • Warning process in the atmosphere of Jupiter, Saturn, Uranus, and Neptune- is much similar to that of the earth, but their absorbing materials are different.
  • 23. • Earth- is warmed by the heat developed in the absorption of ultraviolet rays by the ozone layer in the atmosphere while the outer planets are warmed by the heat developed by the absorption of solar radiation of methane and the smog of some particles. • Jupiter, Saturn, and Neptune- are found to be emitting more heat than they receive from the sun
  • 24. • Planets- are grouped according to size. • Terrestrial planets- are small and they have high densities due to their bodies made up of rocks and heavy elements. • Mercury, Venus, Earth, And Marsare considered terrestrial planets. • Jovian planets- are larger and massive and they have low densities and have dense
  • 25. Characteristics of the Eight Planets of the Solar System Number of Satellite Distance from the sun Inclination Rotation MERCURY 58 million km 7 degrees 14 minutes About 58.7 days 88 days 0 Heavily cratered planet VENUS 67 million miles 3 degrees 39 minutes 243 days 225 days o Veiled planet EARTH 93 million miles 23 degrees 30 minutes 24 hours 365 days 1 Blue planet MARS 141,700,000 0 miles 25 degrees 1.37 1.88 years 2 Red planet 3 degrees 10 hours 19 Largest planet 23 Pale yellow,ringed planet 5 Bluish-green with righs 2 Planet with a clear atmosphere Planet JUPITER Revolution SATURN URANUS NEPTUNE 1.79 billion miles 98 degrees 30 degrees 17.24 hours 14 hours 84 years 165 years Description
  • 26. Lesson 4. Asteroids, Comets, and Meteors • Asteroids- are small chunks of irregularly shaped objects that occupy the 350 million miles space between Mars and Jupiter. • They orbit the sun in a belt following the same direction as those of the planets. - the asteroid belt range in size. If all the asteroids were put together they would form a body no more than 1,500 km in diameter.
  • 27. • Their number is estimated to be about 30,000 but only about 7,000 have been identified.. • They vary in size, shape, color, and composition. • A German astronomer Johan Bode accidentically discovered the existence of these miniature planets in 1800.
  • 28. • Ceres- is the largest asteroids, 940 km in diameter.  Giuseppe Piazzi discovered it on January 1, 1801. Ceres was named after the Roman goddess of agriculture and also known as the protecting goddess of Sicily.  Pallas- is the second largest, 540 km in diameter.  Vesta- which is 510 km in diameter.  About 500 other asteroids are between 50 to 100 km in diameter and the rest are smaller than 50 km.
  • 29. 3 types of asteroids as their color and composition • C-type asteroids- are very dark and carbonaceous. There are 75% of known asteroids. • S-type asteroids- are rusty red in color and they are composed of iron and magnesium silicate. • M-type asteroids- are rich with metallic substances.
  • 30. 3 types of asteroids according to position: 1.Athensis the first type of asteroids.They lie near the orbit of Mars. Some examples are Ceres, Pallas, Juno, and Vesta. 2.Apollosis the second type of asteroids. They lie near Jupiter and they have highly elliptical orbits. Eros, Geographos, and Icarus are examples. These asteroids constantly cross the earth's orbit.  Icarus reached the earth about 6 million km.
  • 31.  Geographos- reached the earth at a distance of about 9 km.  Eros- at about 485,000 miles. 3.Trojans- are the third type. They lie within the main asteroid belt and they circle the sun for 12 years.  Examples are Hector, Diomedes, Agamemnon, and Petrocius.
  • 32. COMETS it is known since ancient times. they were once associated to bad omens and disaster. Oort Cloud- comet originated from a dense shell of material surrounding the outer edge of the solar system. Jan Oort- Dutch Astronomer. Comets- orbits are big and
  • 33. • As they revolved around the sun some can reach the outer edge of the solar system and then back, moving closer towards the sun. • As they get closer to the sun, they become very bright and start forming a tail.
  • 34. 3 Basic Parts of Comets 1. NUCLEUS- which is believed to be solid and composed of frozen gases, water vapor, and dust particles. 2. COMA- a cloudlike structure that surrounds the nucleus which is composed of gas and small bits of rocks and dust. 3. TAIL- that is composed of gas or dust particles or both. Comets may have one or several tails.
  • 35. • When the comet is away from the sun, it has no tail. • Comets appear in the sky from time to time. • Some comets return on a cycle every few years. 2 Groups of Comets according to their order of appearance: 1. Short-period comets- have orbits that take less than 200 years. 2. Long-period comets- have orbits that take more than 200 years.
  • 36. • Haley's comet appears every 76 years . • Edmund Haley- predicted its appearance in 1910. • The last time it reappeared was in 1986 and it is predicted to reappear again in the year 2062. • Kuiper Belt Objects(KBO) - this is the name given to many small bodies found orbiting the sun from beyond Neptune and Pluto.
  • 37. • Oort Cloud- is a theoretical, spherical gathering of rocks at the outer edge of the solar system. • Meteors- are the bright streak of light that dart the night sky which are referred to as "shooting star". • In reality meteors are "space debris" or stray pieces of stony or metallic rocks that pass through the earth's atmosphere.
  • 38. • Meteors travel in great speed that sometimes exceeds 100,000 miles per hour. • Friction with the earth's atmosphere caused them to glow and vaporize completely in space. • Meteorites- the large ones reach the earth's surface. • Meteor shower- is a celestial event in which a number of meteors are observed to radiate from one point in the night sky. - it is a regular sight sometime in the midmonth of August because in this month Earth crosses the path of comets and meteors are seen in the Esrth's atmosphere.
  • 39. Summary in lesson 2; • The sun is the largest celestial body in the solar system.It has a various characteristics. • The sun's atmosphere is the most prominent layer that we see in the sky. The solar atmosphere consists of four layers: Photosphere, Chromosphere, Reversing layer, and Corona. • The photosphere is characterized by disturbances. The most familiar to us are the sunspots. • The chromosphere is likewise characterized by disturbances. The solar flares are disturbances that have profound effect on Earth's atmosphere.
  • 40. Summary in lesson 3: • The planets are classified according to size. The terrestrial planets are Mercury, Venus, Earth, and Mars, while Jovian Planets are Jupiter, Saturn, Neptune, and Uranus. • The eight planets differ in terms of distance from the sun, rotation, revolution,inclination,and number of satellites.
  • 41. Summary in lesson 4: • Impact of asteroids larger than 500 meters on the earth's surface can cause global devastation. But this is an extremely rare phenomenon. • Astronomers consider all three celestial objects as space debris. • Comets have large and elliptical orbits and return on a predictable cycle of few years. • Asteroids are chunks of irregularly shaped objects that occupy the space between Mars and Jupiter. • Meteors are stray pieces of objects that appear in the night sky as shooting stars.
  • 42. THANK YOU GEMINI FOR LISTENING!!! "have a nice day everyone"...