The Hertzsprung-Russell Diagram
... Most stars lie in the main sequence because if a star is hotter it is brighter. Thus you would expect stars of the same size but different temperatures to form a diagonal line since “hotter means brighter” That Main-Sequence is steeper than a ‘same-size diagonal” shows that larger mass ‘normal’ star ...
... Most stars lie in the main sequence because if a star is hotter it is brighter. Thus you would expect stars of the same size but different temperatures to form a diagonal line since “hotter means brighter” That Main-Sequence is steeper than a ‘same-size diagonal” shows that larger mass ‘normal’ star ...
Part 1—Stages of Human Life
... 1. Make an educated guess of the life cycle of the images of the stars. Guess the stages of life for this high mass star. 2. Shuffle the images and place them in order from youngest to oldest, but do NOT glue them down yet. 3. List the logic and the reasons for why you placed the images in the order ...
... 1. Make an educated guess of the life cycle of the images of the stars. Guess the stages of life for this high mass star. 2. Shuffle the images and place them in order from youngest to oldest, but do NOT glue them down yet. 3. List the logic and the reasons for why you placed the images in the order ...
1. Star A has a distance of 3 parsecs. What is its parallax angle? 1a
... Star I is of spectral type O2 and star II is of spectral type O3. Which star is hotter? Star I. Which of the following stars is the most massive: a) G2V b) K8V c) O1V? c) because its the hottest and hence brightest and hence most luminous. What do all the stars in question 13) have in common? They a ...
... Star I is of spectral type O2 and star II is of spectral type O3. Which star is hotter? Star I. Which of the following stars is the most massive: a) G2V b) K8V c) O1V? c) because its the hottest and hence brightest and hence most luminous. What do all the stars in question 13) have in common? They a ...
Astronomy 360 - Indiana State University
... independent of the observer's location and the time of the observation. This means that only one set of coordinates is required for each object, and that these same coordinates can be used by observers in different locations and at different times. The equatorial coordinate system is basically the p ...
... independent of the observer's location and the time of the observation. This means that only one set of coordinates is required for each object, and that these same coordinates can be used by observers in different locations and at different times. The equatorial coordinate system is basically the p ...
Student Literacy
... how some stars were always visible at night. Other stars were only visible during certain months of the year. People charted when these stars appeared and how they were positioned. They depended on these stars and star patterns for direction. Skywatchers noticed that during the spring, summer, fall ...
... how some stars were always visible at night. Other stars were only visible during certain months of the year. People charted when these stars appeared and how they were positioned. They depended on these stars and star patterns for direction. Skywatchers noticed that during the spring, summer, fall ...
CHAPTER 10, Stellar Motions
... Astronomers have now detected hundreds of planetary bodies, called exoplanets, moving in orbit around other stars. Most of these are more massive than any of the Sun's planets. These planetary-like bodies are detected because of their strong gravitational interactions with their stars. However, tech ...
... Astronomers have now detected hundreds of planetary bodies, called exoplanets, moving in orbit around other stars. Most of these are more massive than any of the Sun's planets. These planetary-like bodies are detected because of their strong gravitational interactions with their stars. However, tech ...
STAAR Review – Week Ten
... a. Stars with greater magnitudes tend to have lower temperatures. b. Stars with greater masses tend to have lower temperatures. c. Stars with greater magnitudes tend to have higher temperatures. d. Stars with greater temperatures tend to have lower magnitudes. 19. What do our Sun and the star Vega h ...
... a. Stars with greater magnitudes tend to have lower temperatures. b. Stars with greater masses tend to have lower temperatures. c. Stars with greater magnitudes tend to have higher temperatures. d. Stars with greater temperatures tend to have lower magnitudes. 19. What do our Sun and the star Vega h ...
Astronomy
... The star is now in the “prime of its life”; it is in equilibrium. Over time; temp, luminosity, color change. Our sun is in the main sequence phase It will live for about 10 billion years Our sun is now about 4.6 billion years old – Links: ...
... The star is now in the “prime of its life”; it is in equilibrium. Over time; temp, luminosity, color change. Our sun is in the main sequence phase It will live for about 10 billion years Our sun is now about 4.6 billion years old – Links: ...
Stars Crossword
... 4. a singularity whose gravity is so strong that nothing can escape - not even light 5. the area surrounding a blackhole where at that point nothing can escape 9. the middle age stage of a small star like ours 11. when a very large star's outer layer explodes outward with an amazing amount of force ...
... 4. a singularity whose gravity is so strong that nothing can escape - not even light 5. the area surrounding a blackhole where at that point nothing can escape 9. the middle age stage of a small star like ours 11. when a very large star's outer layer explodes outward with an amazing amount of force ...
Integrative Studies 410 Our Place in the Universe
... Formation of the Elements • Light elements (hydrogen, helium) formed in Big Bang • Heavier elements formed by nuclear fusion in stars and thrown into space by supernovae – Condense into new stars and planets – Elements heavier than iron form during supernovae explosions ...
... Formation of the Elements • Light elements (hydrogen, helium) formed in Big Bang • Heavier elements formed by nuclear fusion in stars and thrown into space by supernovae – Condense into new stars and planets – Elements heavier than iron form during supernovae explosions ...
Neutron Stars - Otterbein University
... Super-Massive Stars end up as Black Holes • If the mass of the star is sufficiently large (M > 25 MSun), even the neutron pressure cannot halt the collapse – in fact, no known force can stop it! • The star collapses to a very small size, with ultrahigh density • Nearby gravity becomes so strong tha ...
... Super-Massive Stars end up as Black Holes • If the mass of the star is sufficiently large (M > 25 MSun), even the neutron pressure cannot halt the collapse – in fact, no known force can stop it! • The star collapses to a very small size, with ultrahigh density • Nearby gravity becomes so strong tha ...
Stellar Evolution Test Answers
... 1. When the light from a distant galaxy is distorted by a black hole, the resulting image is a ring. We call this a) the photon sphere b) the event horizon c) gravitational lensing d) the cosmological principle 2. Once you cross the ____________________, there is no going back…light can no longer es ...
... 1. When the light from a distant galaxy is distorted by a black hole, the resulting image is a ring. We call this a) the photon sphere b) the event horizon c) gravitational lensing d) the cosmological principle 2. Once you cross the ____________________, there is no going back…light can no longer es ...
Mapping the Stars
... Do the stars appear to move at night also? Yes All the stars we see at night appear to rotate around which star? Polaris which is the North Star Where is Polaris located? Directly above the Earth’s North Pole. Stars are actually moving in space, but since they are so distant , their movement is hard ...
... Do the stars appear to move at night also? Yes All the stars we see at night appear to rotate around which star? Polaris which is the North Star Where is Polaris located? Directly above the Earth’s North Pole. Stars are actually moving in space, but since they are so distant , their movement is hard ...
hw5
... A creature’s likelyhood of surviving changes in their environment over time depends on how quickly they can adapt to those changes. An intelligent creature can adapt very quickly to changes through use of tools and rational behavior. p. 370 RQ# 3 How can astronomers use variable stars to find distan ...
... A creature’s likelyhood of surviving changes in their environment over time depends on how quickly they can adapt to those changes. An intelligent creature can adapt very quickly to changes through use of tools and rational behavior. p. 370 RQ# 3 How can astronomers use variable stars to find distan ...
Date_________________ TWINKLE, TWINKLE
... a star. The spectra of stars provide one basis for classifying stars. Stars have colors which you can notice if you let your eyes acclimate at night (red, orange, yellow, white, and blue). The major lines in a star's spectrum dictates the color. Stars of similar color share other characteristics tha ...
... a star. The spectra of stars provide one basis for classifying stars. Stars have colors which you can notice if you let your eyes acclimate at night (red, orange, yellow, white, and blue). The major lines in a star's spectrum dictates the color. Stars of similar color share other characteristics tha ...
Cassiopeia (constellation)
Cassiopeia is a constellation in the northern sky, named after the vain queen Cassiopeia in Greek mythology, who boasted about her unrivalled beauty. Cassiopeia was one of the 48 constellations listed by the 2nd-century Greek astronomer Ptolemy, and it remains one of the 88 modern constellations today. It is easily recognizable due to its distinctive 'M' shape when in upper culmination but in higher northern locations when near lower culminations in spring and summer it has a 'W' shape, formed by five bright stars. It is bordered by Andromeda to the south, Perseus to the southeast, and Cepheus to the north. It is opposite the Big Dipper.In northern locations above 34ºN latitude it is visible year-round and in the (sub)tropics it can be seen at its clearest from September to early November in its characteristic 'M' shape. Even in low southern latitudes below 25ºS is can be seen low in the North.