'Young star' diaporamas de présentation

PHYS178 2008 week 11 part-1

PHYS178 2008 week 11 part-1. Extrasolar planets Lecture 2: Planetary formation theory and detection techniques A/Prof. Quentin A Parker. Formation of a Star and proto-planetary disk. Dense cores form within a molecular cloud.

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Units to cover

Units to cover. 60-63. Homework 8 Unit 56 problems 6,7 Unit 59 problems 6, 8, 9 Unit 60 problems 6, 8, 11 Unit 61 problems 4, 7 Unit 62, problem 8. Tracking changes with the HR Diagram. As a star evolves, its temperature and luminosity change.

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Variability of young stars with LSST Gregory J. Herczeg KIAA

Variability of young stars with LSST Gregory J. Herczeg KIAA. Star Formation: ISM/Molecular Clouds. Pre-main sequence stellar evolution (low-mass case). Classical T Tauri Stars. HD141569, Clampin et al. From Visser et al., in prep. Morphology of a classical T Tauri star.

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The History of the Earth

The History of the Earth. How do we know how the solar systems are formed?. It takes a very long time for a solar system to form; therefore we cannot observe the formation of a solar system. How do we know how solar systems are formed? Lifecycle of a Frog Example:

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STAR VIDEO

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STARS

STARS. Page Keeley Where do Stars Go?. Learning goal: Explain the physical properties of stars. Think About It. When you look at the night time sky, how many stars do you see? Hundreds? Thousands? Millions?

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Designing Hydrologic Observatories as a Community Resource

Designing Hydrologic Observatories as a Community Resource. Welcome to the CUAHSI National Workshop on. John L. Wilson New Mexico Inst. Of Mining & Technology Chair, CUAHSI Board of Directors. Logan, Utah, August 24-25, 2004. CUAHSI.

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Romeo and Juliet A Play by William Shakespeare

Romeo and Juliet A Play by William Shakespeare. Characters & Summary of Acts 1 through 5. 9 th Grade English Ms. Richards. Click the image to continue. Main Menu. Plot Overview Main Characters More Characters Act 1 Act 2 Act 3 Act 4 Act 5 Review Question.

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Young stars forming

Young stars forming . Young stars forming, continued. Young stars forming, continued. Principles governing the structure of a star Figure 7.1. Evolution of a 1 solar-mass star Figure 7.2. Evolution of a high-mass star Figure 7.3. Birth of a star Figure 7.4. Protostars Figure 7.5.

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Learning Objectives: Where do the elements come from? What can we learn from telescopes?

The Origin of Chemical Elements. Learning Objectives: Where do the elements come from? What can we learn from telescopes? How do heavy elements form?. What happens in stars?. What happens to the missing mass?. Why do you think two anti-electrons are released?.

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A new luminosity and mass function for low mass stars in the Serpens cloud

A new luminosity and mass function for low mass stars in the Serpens cloud. Alain KLOTZ : C.E.S.R. Toulouse - France Nicolas LODIEU : A.I.P. Postdam - Germany Emmanuel CAUX : C.E.S.R. Toulouse - France Jean-Louis MONIN : L.A.O.G. Grenoble - France.

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Wednesday 10-1-14

Wednesday 10-1-14. WU: Compare a radio wave to a microwave. a) Which has a higher frequency? b) Which has a longer wavelength? Check Starlight Starbright worksheet Spectrum Analysis. Microwave. Radio Waves. To Do. Quizlet has been moved to Friday Grade Star Light, Star Bright

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Shakespeare

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Chandra Science Highlight

Chandra Science Highlight. DEM L 316: Two Supernova Remnants in the Large Magellanic Cloud. Chandra X-ray Observatory ACIS image.

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Chandra Science Highlight

Chandra Science Highlight. Chandra X-ray Observatory ACIS image. BP Psc: An Enigmatic Emission-line Star. The composite images show X-ray (purple) and optical data orange, green and blue) for BP Piscium (BP Psc), a peculiar star thought to be a red giant star.

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