Gemini South telescope makes the case for multiple Earth
... to capture fine detail and “freeze” the turbulence caused by Earth’s atmosphere. With this technique, the final images yield a resolution equal to what the Gemini telescope would produce if it were in space. Thus, Gemini can uniquely resolve such faint, distant objects. ...
... to capture fine detail and “freeze” the turbulence caused by Earth’s atmosphere. With this technique, the final images yield a resolution equal to what the Gemini telescope would produce if it were in space. Thus, Gemini can uniquely resolve such faint, distant objects. ...
chapter 28 pages 747-752
... • When a star’s spectra is shifting to different wavelengths, this means it is moving • If the spectra shifts towards the blue (shorter) wavelengths, the star is moving towards us • If it shift towards the red (longer) wavelengths, then the star is moving away ...
... • When a star’s spectra is shifting to different wavelengths, this means it is moving • If the spectra shifts towards the blue (shorter) wavelengths, the star is moving towards us • If it shift towards the red (longer) wavelengths, then the star is moving away ...
Sample exam 2
... 12. What are the conditions necessary to initiate star formation? Give at least three different characteristics, and how each leads to (or is needed for) star formation. 13. Globular clusters are clusters that orbit a galaxy that contain millions of M-class stars. What does this suggest about the ag ...
... 12. What are the conditions necessary to initiate star formation? Give at least three different characteristics, and how each leads to (or is needed for) star formation. 13. Globular clusters are clusters that orbit a galaxy that contain millions of M-class stars. What does this suggest about the ag ...
The life of a Star (pages 468-471)
... 2. Explain how a nebula turns into a cloud leading to a star (3 steps)? 3. What happens when a star runs out of the fuels needed to produce energy? 4. What is a supernova? During this stage, what happens to the core of the star? When our Sun eventually swells into a red giant star, its outer layer ...
... 2. Explain how a nebula turns into a cloud leading to a star (3 steps)? 3. What happens when a star runs out of the fuels needed to produce energy? 4. What is a supernova? During this stage, what happens to the core of the star? When our Sun eventually swells into a red giant star, its outer layer ...
The Life Cycle of a star
... • A supernova can light up the sky for weeks. • The temperature in one can reach 1,000,000,000 °C. • The supernova then either becomes a neutron star or a black hole. ...
... • A supernova can light up the sky for weeks. • The temperature in one can reach 1,000,000,000 °C. • The supernova then either becomes a neutron star or a black hole. ...
Global Warming_Notes_for_Test_Review[1]
... 24. Star mass is expressed in terms of solar mass. Our sun is a one solar mass star. 25. Luminosity is a measure of the total amount of energy a star radiates per second. 26. Fusion is the transformation of hydrogen into helium. ...
... 24. Star mass is expressed in terms of solar mass. Our sun is a one solar mass star. 25. Luminosity is a measure of the total amount of energy a star radiates per second. 26. Fusion is the transformation of hydrogen into helium. ...
Chapter 13 Notes – The Deaths of Stars
... of an ___________ core, happen extremely rapidly: _________ burning only lasts for about _______ day Iron core ultimately _________________, triggering an explosion that destroys the star: A __________________! Several hundreds to ________________ of years later, the ejected material from supern ...
... of an ___________ core, happen extremely rapidly: _________ burning only lasts for about _______ day Iron core ultimately _________________, triggering an explosion that destroys the star: A __________________! Several hundreds to ________________ of years later, the ejected material from supern ...
PHYS299B_Final_HudsonJustin
... a solar eclipse. The smaller dips in brightness is when the brighter star blocks out the light from the other star when passing in front of it. • From these curves, we can tell if stars follow the characteristics of an eclipsing binary or other types of variable stars. ...
... a solar eclipse. The smaller dips in brightness is when the brighter star blocks out the light from the other star when passing in front of it. • From these curves, we can tell if stars follow the characteristics of an eclipsing binary or other types of variable stars. ...
Stellar Magnitude, Distance, and Motion
... o Proper motion is not large. The star with the largest proper motion is called Barnard's Star. It moves 10.3 seconds of arc per year. o Since the moon subtends about 1/2 of a degree (which is 1/2 x 60 x 60 = 1800 seconds of arc) on the celestial sphere, it takes Barnard's star about 1800/10.3 ~ ...
... o Proper motion is not large. The star with the largest proper motion is called Barnard's Star. It moves 10.3 seconds of arc per year. o Since the moon subtends about 1/2 of a degree (which is 1/2 x 60 x 60 = 1800 seconds of arc) on the celestial sphere, it takes Barnard's star about 1800/10.3 ~ ...
I : Internal structure of main sequence stars
... The luminosity L The efficiency of the fusion η The mass of the star M The fraction of the stellar mass that can participate in the fusion reactions f ...
... The luminosity L The efficiency of the fusion η The mass of the star M The fraction of the stellar mass that can participate in the fusion reactions f ...
PowerPoint Presentation - ASTR498E High energy
... The mass of the star M The fraction of the stellar mass that can participate in the fusion reactions f ...
... The mass of the star M The fraction of the stellar mass that can participate in the fusion reactions f ...
Week 5 (10/16) – Quiz #11
... Which of the following statements most accurately describes what happens when I HOLD A PIECE OF CHALK IN MY HAND: A. B. C. D. ...
... Which of the following statements most accurately describes what happens when I HOLD A PIECE OF CHALK IN MY HAND: A. B. C. D. ...
E5 stellar processes and stellar evolution (HL only)
... Interstellar space consists of gas (74% H, 25% He by mass) and dust at a density of about 10-21 kg.m-3. This is about one hydrogen atom to every cm3 of space. ...
... Interstellar space consists of gas (74% H, 25% He by mass) and dust at a density of about 10-21 kg.m-3. This is about one hydrogen atom to every cm3 of space. ...