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by Megan Koehn...Basic needs of plants (Kindergarten)
Basic Needs Of Plants
Basic Needs Of Plants
guesta178af0
What plants need?
What plants need?
What plants need?
fengchuishaster
this is a ppt for basic introduction of plants & its lifecycle.
Parts of plants
Parts of plants
anishakansagra
uses of Plants
uses of Plants
English planet
Science 3
Plant habitats
Plant habitats
YhanzieCapilitan
Plant Parts 1-2nd grade
Plant Parts 1-2nd grade
Lee De Groft
What do plants need to grow ? WATER Water is necessary for proper germination of seeds. Plants need water for growth. LIGHT Green plants need sunlight in to make their own food. NUTRIENTS Plants need the minerals found in soil for healthy growth. WARMTH Plants only grow well in the right conditions. Temperatures that are too cold or too hot may affect how the plant grows. Plants need water, air, nutrients, and sunlight to grow. References https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=plants&imgrc=zZol8-3s3BbYkM%3A https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=water https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=water&imgrc=PPFuoqF0BDb2EM%3A https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=water+plants+clipart&imgrc=b7wMWmxxPdUzQM%3A
How Plants Grow
How Plants Grow
Shin Tampus
All living things grow and change. All living things need food, water, and air to live.
Parts of a plant
Parts of a plant
subject specialist biology
Recommandé
by Megan Koehn...Basic needs of plants (Kindergarten)
Basic Needs Of Plants
Basic Needs Of Plants
guesta178af0
What plants need?
What plants need?
What plants need?
fengchuishaster
this is a ppt for basic introduction of plants & its lifecycle.
Parts of plants
Parts of plants
anishakansagra
uses of Plants
uses of Plants
English planet
Science 3
Plant habitats
Plant habitats
YhanzieCapilitan
Plant Parts 1-2nd grade
Plant Parts 1-2nd grade
Lee De Groft
What do plants need to grow ? WATER Water is necessary for proper germination of seeds. Plants need water for growth. LIGHT Green plants need sunlight in to make their own food. NUTRIENTS Plants need the minerals found in soil for healthy growth. WARMTH Plants only grow well in the right conditions. Temperatures that are too cold or too hot may affect how the plant grows. Plants need water, air, nutrients, and sunlight to grow. References https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=plants&imgrc=zZol8-3s3BbYkM%3A https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=water https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=water&imgrc=PPFuoqF0BDb2EM%3A https://www.google.com/search?q=water+cycle&source=lnms&tbm=isch&sa=X&ved=0ahUKEwjKpO6HkevNAhWCopQKHXnSBrUQ_AUICCgB&biw=1366&bih=624#tbm=isch&q=water+plants+clipart&imgrc=b7wMWmxxPdUzQM%3A
How Plants Grow
How Plants Grow
Shin Tampus
All living things grow and change. All living things need food, water, and air to live.
Parts of a plant
Parts of a plant
subject specialist biology
Plants: how are they grouped, types of roots and the function of stems and roots
Plants 3rd grade
Plants 3rd grade
Tape Ayvukue
Chapter 2 what do plants need to grow
Chapter 2 what do plants need to grow
firstgradewalks
Plant parts
Plant parts
SaintDenisSchool52
Plants and their parts - Luke - Grade 2
Lesson 1. Plants and their parts
Lesson 1. Plants and their parts
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Parts of a plant ppt
Parts of a plant ppt
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The Parts Of Plants
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Plants needs
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Plants powerpoint and interactive activities
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https://www.dropbox.com/s/y7ymozui1f5qazy/Parts%20of%20a%20Plant%20-%20PowerPoint.ppt?dl=1
Parts of a plant power point
Parts of a plant power point
REXTEC
Slides on parts of plants and characteristics of different parts of animals
Parts of Plants
Parts of Plants
THIRIPURASUNTHARIAP
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Kinds of plants
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Power point sobre les plantes i les funcions de les seves parts. Utilitzat a Cicle Mitjà PILE
Parts of the plants and their functions
Parts of the plants and their functions
Escola Mediterrania
The parts of a plant and their functions
The parts of a plant and their functions
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Plants, leaf parts, cross section of a stem, cross section of a leaf, xylem and phloem
Powerpoint plant parts for science gr 5
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Parts of the Plants
Parts of the plants
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Plant Information
Plants powerpoint
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Basic presentation of the parts of a plant and of the life cycle of plants. Pitched at about the 2nd, 3rd or 4th grade level. Lots of descriptive pictures and diagrams.
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Plants: how are they grouped, types of roots and the function of stems and roots
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https://www.dropbox.com/s/y7ymozui1f5qazy/Parts%20of%20a%20Plant%20-%20PowerPoint.ppt?dl=1
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Biological Classification BioHack (3).pdf
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muntazimhurra
Understanding circumstellar disks is of prime importance in astrophysics, however, their birth process remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, often wrapped into a sub-grid model, play a crucial role in disk formation and evolution. This calls for a combined approach in which both the protostar and circumstellar disk are studied in concert. Aims. We aim to elucidate the small scale physics and constrain sub-grid parameters commonly chosen in the literature by resolving the star-disk interaction. Methods. We carry out a set of very high resolution 3D radiative-hydrodynamics simulations that self-consistently describe the collapse of a turbulent dense molecular cloud core to stellar densities. We study the birth of the protostar, the circumstellar disk, and its early evolution (< 6 yr after protostellar formation). Results. Following the second gravitational collapse, the nascent protostar quickly reaches breakup velocity and sheds its surface material, thus forming a hot (∼ 103 K), dense, and highly flared circumstellar disk. The protostar is embedded within the disk, such that material can flow without crossing any shock fronts. The circumstellar disk mass quickly exceeds that of the protostar, and its kinematics are dominated by self-gravity. Accretion onto the disk is highly anisotropic, and accretion onto the protostar mainly occurs through material that slides on the disk surface. The polar mass flux is negligible in comparison. The radiative behavior also displays a strong anisotropy, as the polar accretion shock is shown to be supercritical whereas its equatorial counterpart is subcritical. We also f ind a remarkable convergence of our results with respect to initial conditions. Conclusions. These results reveal the structure and kinematics in the smallest spatial scales relevant to protostellar and circumstellar disk evolution. They can be used to describe accretion onto regions commonly described by sub-grid models in simulations studying larger scale physics.
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Botany krishna series 2nd semester Only Mcq type questions
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Context. Determining the size distribution of asteroids is key to understanding the collisional history and evolution of the inner Solar System. Aims. We aim to improve our knowledge of the size distribution of small asteroids in the main belt by determining the parallaxes of newly detected asteroids in the Hubble Space Telescope (HST) archive and subsequently their absolute magnitudes and sizes. Methods. Asteroids appear as curved trails in HST images because of the parallax induced by the fast orbital motion of the spacecraft. Taking into account the trajectory of this latter, the parallax effect can be computed to obtain the distance to the asteroids by fitting simulated trajectories to the observed trails. Using distance, we can obtain the absolute magnitude of an object and an estimation of its size assuming an albedo value, along with some boundaries for its orbital parameters. Results. In this work, we analyse a set of 632 serendipitously imaged asteroids found in the ESA HST archive. Images were captured with the ACS/WFC and WFC3/UVIS instruments. A machine learning algorithm (trained with the results of a citizen science project) was used to detect objects in these images as part of a previous study. Our raw data consist of 1031 asteroid trails from unknown objects, not matching any entries in the Minor Planet Center (MPC) database using their coordinates and imaging time. We also found 670 trails from known objects (objects featuring matching entries in the MPC). After an accuracy assessment and filtering process, our analysed HST asteroid set consists of 454 unknown objects and 178 known objects. We obtain a sample dominated by potential main belt objects featuring absolute magnitudes (H) mostly between 15 and 22 mag. The absolute magnitude cumulative distribution logN(H > H0) ∝ αlog(H0) confirms the previously reported slope change for 15 < H < 18, from α ≈ 0.56 to α ≈ 0.26, maintained in our case down to absolute magnitudes of around H ≈ 20, and therefore expanding the previous result by approximately two magnitudes. Conclusions. HST archival observations can be used as an asteroid survey because the telescope pointings are statistically randomly oriented in the sky and cover long periods of time. They allow us to expand the current best samples of astronomical objects at no extra cost in regard to telescope time.
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Hubble Asteroid Hunter III. Physical properties of newly found asteroids
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Context. WASP-76 b has been a recurrent subject of study since the detection of a signature in high-resolution transit spectroscopy data indicating an asymmetry between the two limbs of the planet. The existence of this asymmetric signature has been confirmed by multiple studies, but its physical origin is still under debate. In addition, it contrasts with the absence of asymmetry reported in the infrared (IR) phase curve. Aims. We provide a more comprehensive dataset of WASP-76 b with the goal of drawing a complete view of the physical processes at work in this atmosphere. In particular, we attempt to reconcile visible high-resolution transit spectroscopy data and IR broadband phase curves. Methods. We gathered 3 phase curves, 20 occultations, and 6 transits for WASP-76 b in the visible with the CHEOPS space telescope. We also report the analysis of three unpublished sectors observed by the TESS space telescope (also in the visible), which represents 34 phase curves. Results. WASP-76 b displays an occultation of 260±11 and 152±10 ppm in TESS and CHEOPS bandpasses respectively. Depending on the composition assumed for the atmosphere and the data reduction used for the IR data, we derived geometric albedo estimates that range from 0.05 ± 0.023 to 0.146 ± 0.013 and from <0.13 to 0.189 ± 0.017 in the CHEOPS and TESS bandpasses, respectively. As expected from the IR phase curves, a low-order model of the phase curves does not yield any detectable asymmetry in the visible either. However, an empirical model allowing for sharper phase curve variations offers a hint of a flux excess before the occultation, with an amplitude of ∼40 ppm, an orbital offset of ∼−30◦ , and a width of ∼20◦ . We also constrained the orbital eccentricity of WASP-76 b to a value lower than 0.0067, with a 99.7% confidence level. This result contradicts earlier proposed scenarios aimed at explaining the asymmetry observed in high-resolution transit spectroscopy. Conclusions. In light of these findings, we hypothesise that WASP-76 b could have night-side clouds that extend predominantly towards its eastern limb. At this limb, the clouds would be associated with spherical droplets or spherically shaped aerosols of an unknown species, which would be responsible for a glory effect in the visible phase curves.
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Small size (20-300 nm) / bacteria (size measured in μm) Viral genome – single type of nucleic acid: DNA – dezoxyriboviruses RNA - riboviruses Totally dependant on living cells for all metabolic processes May infect humans, animals, plants, bacteria, fungi,parasites, insects Virion = viral corpuscle = elementary, infectious unit. Only visible by electron microscopy. Laboratory diagnosis of viral infections Methods: • Cytology • Electron microscopy • Cultivation • Detection of viral proteins • Serology • Molecular diagnosis (detection of genetic material i.e. nucleic acids) PPT prepared by Dr. Prince C P
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Biopesticide (2).pptx .This slides helps to know the different types of biop...
Biopesticide (2).pptx .This slides helps to know the different types of biop...
Botany krishna series 2nd semester Only Mcq type questions
Botany krishna series 2nd semester Only Mcq type questions
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
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COST ESTIMATION FOR A RESEARCH PROJECT.pptx
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Pulmonary drug delivery system M.pharm -2nd sem P'ceutics
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Green chemistry and Sustainable development.pptx
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SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx
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Presentation Vikram Lander by Vedansh Gupta.pptx
Isotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on Io
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Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
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VIRUSES structure and classification ppt by Dr.Prince C P
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SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE
Botany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdf
Needs of plants
1.
11/18/13
2.
3.
4.
5.
6.
» Water is necessary
for proper germination of seeds. » Plants need water for growth.
7.
8.
»Green plants need sunlight in to
make their own food.
9.
10.
»Plants need the minerals found
in soil for healthy growth.
11.
12.
» Plants only
grow well in the right conditions. » Temperatures that are too cold or too hot may affect how the plant grows.
13.
14.
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18.
THE PROCESS
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2nd day 11/19/13 Planting