Astronomy Day 2006: A short presentation on eclipsing binary stars
... It is recognized as fact by astronomers that well over half of the stars in the universe belong to multiple systems. You might think of our Sun as being an exceptional system that involves only one star and you would be right. ...
... It is recognized as fact by astronomers that well over half of the stars in the universe belong to multiple systems. You might think of our Sun as being an exceptional system that involves only one star and you would be right. ...
Teacher Sheet 1. What variables does the HR Diagram compare
... 12. Why do giants differ from stars in the Main Sequence? Although they are cool [red], they are very luminous, and therefore bright. In the Main Sequence, stars that are cool are not as luminous. 13. How do white dwarf stars differ from stars in the Main Sequence? White dwarf stars are very hot [bl ...
... 12. Why do giants differ from stars in the Main Sequence? Although they are cool [red], they are very luminous, and therefore bright. In the Main Sequence, stars that are cool are not as luminous. 13. How do white dwarf stars differ from stars in the Main Sequence? White dwarf stars are very hot [bl ...
here - Lund Observatory
... The trigonometric parallax for Sirius has been determined to 0.375’’. Stars of the same spectral and luminosity class are supposed to have the same absolute magnitudes and intrinsic colour indices. The interstellar reddening of the two binary components is assumed to be the same. The two cluster sta ...
... The trigonometric parallax for Sirius has been determined to 0.375’’. Stars of the same spectral and luminosity class are supposed to have the same absolute magnitudes and intrinsic colour indices. The interstellar reddening of the two binary components is assumed to be the same. The two cluster sta ...
Consider Average Stars
... The apparent brightness of a star – that is, what we actually see – is partly an accident of location: nearby stars can look deceptively bright. (The obvious example is the Sun!) But the intrinsic (true) brightness of a star is a good measure of how much energy is being generated, how fast the fuel ...
... The apparent brightness of a star – that is, what we actually see – is partly an accident of location: nearby stars can look deceptively bright. (The obvious example is the Sun!) But the intrinsic (true) brightness of a star is a good measure of how much energy is being generated, how fast the fuel ...
Stellar Magnitude, Distance, and Motion
... 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 ~ 180 years to change its posit ...
... 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 ~ 180 years to change its posit ...
Document
... Aside from temperature (color) and luminosity (absolute magnitude), what other physical parameters are needed to characterize a star? • Chemical composition • Mass • Radius • Age These parameters can be measured directly using: • nearby/bright stars, (spectrum = composition) • binary stars, (binary ...
... Aside from temperature (color) and luminosity (absolute magnitude), what other physical parameters are needed to characterize a star? • Chemical composition • Mass • Radius • Age These parameters can be measured directly using: • nearby/bright stars, (spectrum = composition) • binary stars, (binary ...
Lives of stars
... 3. Do these pair(s) of stars have same stellar classification? explain 4. Which two stars have same luminosity? 5. Do these pair(s) have same stellar classifications? explain 6. Which letter is most similar to the current sun’s location n the diagram? 7. When the sun starts to die, the sun will star ...
... 3. Do these pair(s) of stars have same stellar classification? explain 4. Which two stars have same luminosity? 5. Do these pair(s) have same stellar classifications? explain 6. Which letter is most similar to the current sun’s location n the diagram? 7. When the sun starts to die, the sun will star ...
Making H-R Diagrams - PLC-METS
... see them the same. The apparent magnitude of a star is the amount of light received on Earth or the brightness of the star as seen from Earth. This is different than the absolute magnitude because the absolute magnitude is based upon the amount of light the star gives off. This difference is the rea ...
... see them the same. The apparent magnitude of a star is the amount of light received on Earth or the brightness of the star as seen from Earth. This is different than the absolute magnitude because the absolute magnitude is based upon the amount of light the star gives off. This difference is the rea ...
Spectra of stars
... You can see that the spectrum is basically a continuous spectrum from violet to red but it is covered with many fine dark lines. These are absorption lines and in a real stellar spectrum there would be many hundreds of these spread across the whole spectrum. A black and white version of the spectrum ...
... You can see that the spectrum is basically a continuous spectrum from violet to red but it is covered with many fine dark lines. These are absorption lines and in a real stellar spectrum there would be many hundreds of these spread across the whole spectrum. A black and white version of the spectrum ...
The Future Sun • Homework 5 is due Wed, 24 March at 6:30am
... In what ways are HR diagrams of H+χ Perseus, Pleiades, Hyades, & NGC188 different? Q Which is false a. Hottest stars in Perseus are hotter than hottest stars in Pleiades. b. Most stars are on the main sequence. c. NGC188 has small range of luminosity d. Some clusters have giants. ...
... In what ways are HR diagrams of H+χ Perseus, Pleiades, Hyades, & NGC188 different? Q Which is false a. Hottest stars in Perseus are hotter than hottest stars in Pleiades. b. Most stars are on the main sequence. c. NGC188 has small range of luminosity d. Some clusters have giants. ...
class17
... A. It would be only 1/3 as bright. B. It would be only 1/6 as bright. C. It would be only 1/9 as bright. D. It would be three times brighter. ...
... A. It would be only 1/3 as bright. B. It would be only 1/6 as bright. C. It would be only 1/9 as bright. D. It would be three times brighter. ...
Patterns in the Sky - Plano Independent School District
... stars that make up the pan or dipper and the 3 stars in the tail. You use the 2 stars on the end of the pan as the pointing stars to find Polaris the North Star in the tail of the Little Dipper. The 2 stars that are the pointers are Dubhe—the top star and Merak—the bottom star in the pan. The handle ...
... stars that make up the pan or dipper and the 3 stars in the tail. You use the 2 stars on the end of the pan as the pointing stars to find Polaris the North Star in the tail of the Little Dipper. The 2 stars that are the pointers are Dubhe—the top star and Merak—the bottom star in the pan. The handle ...
Measuring the Stars
... the main sequence, as this is where most stars are. Also indicated is the white dwarf region; these stars are hot but not very luminous, as they are quite small. ...
... the main sequence, as this is where most stars are. Also indicated is the white dwarf region; these stars are hot but not very luminous, as they are quite small. ...
PHYS 2410 General Astronomy Homework 5
... The last cycle started a Maunder minimum, and the next maximum can not be predicted. ...
... The last cycle started a Maunder minimum, and the next maximum can not be predicted. ...
Citizen Sky Epsilon Aurigae Script for Fulldome Planetariums
... it drops in brightness and mysteriously dims for nearly two years. Let’s replace our classical view of the constellation with a connect-the-dots look. The lines will help us as we leave our earthbound perspective and simulate a trip to this fascinating destination. We can now see that the “dots” of ...
... it drops in brightness and mysteriously dims for nearly two years. Let’s replace our classical view of the constellation with a connect-the-dots look. The lines will help us as we leave our earthbound perspective and simulate a trip to this fascinating destination. We can now see that the “dots” of ...
Document
... from us than 1 pc. b. Star A is closer to us than Star B. Both are closer to us than 1 pc. c. Star A is closer to us than 1 pc. Star B is farther than 1 pc. d. Star B is closer to us than 1 pc. Star A is farther than 1 pc. e. Star B is closer to us than Star A. Both are farther away than 1 pc. ...
... from us than 1 pc. b. Star A is closer to us than Star B. Both are closer to us than 1 pc. c. Star A is closer to us than 1 pc. Star B is farther than 1 pc. d. Star B is closer to us than 1 pc. Star A is farther than 1 pc. e. Star B is closer to us than Star A. Both are farther away than 1 pc. ...
Stars
... from us than 1 pc. b. Star A is closer to us than Star B. Both are closer to us than 1 pc. c. Star A is closer to us than 1 pc. Star B is farther than 1 pc. d. Star B is closer to us than 1 pc. Star A is farther than 1 pc. e. Star B is closer to us than Star A. Both are farther away than 1 pc. ...
... from us than 1 pc. b. Star A is closer to us than Star B. Both are closer to us than 1 pc. c. Star A is closer to us than 1 pc. Star B is farther than 1 pc. d. Star B is closer to us than 1 pc. Star A is farther than 1 pc. e. Star B is closer to us than Star A. Both are farther away than 1 pc. ...
Lecture 12
... These two stars have about the same luminosity— which one appears brighter (i.e. has a larger apparent brightness) ? A. Alpha Centauri B. The Sun ...
... These two stars have about the same luminosity— which one appears brighter (i.e. has a larger apparent brightness) ? A. Alpha Centauri B. The Sun ...
Merak
... How Far Away: 62 light years away How Bright: About 50 times brighter than the Sun Where to View: In the constellation Ursa Major. When to View:All year round in the Northern Hemisphere ...
... How Far Away: 62 light years away How Bright: About 50 times brighter than the Sun Where to View: In the constellation Ursa Major. When to View:All year round in the Northern Hemisphere ...
Astronomy Lecture Notes: Stellar Nomenclature I Introduction
... 1. If one star is 1 magnitude brighter than another then that star is actually about 2.5 times brighter as measured in Watts/m2 by a photometer. 2. If one star is 5 magnitudes brighter than another then that star is actually exactly 100 times brighter as measured in Watts/m2 by a photometer. 3. Exam ...
... 1. If one star is 1 magnitude brighter than another then that star is actually about 2.5 times brighter as measured in Watts/m2 by a photometer. 2. If one star is 5 magnitudes brighter than another then that star is actually exactly 100 times brighter as measured in Watts/m2 by a photometer. 3. Exam ...
Homework 5 (stellar properties)
... 6. (3 pts.) What two observations/measurements would you make to classify a star according to its luminosity (i.e., luminosity class, e.g., Ia, Ib, II, III, IV, or V)? (Hint: Look at the HR diagram.) Which equation relates these two quantities to the size (radius) of a star (after all, the luminosit ...
... 6. (3 pts.) What two observations/measurements would you make to classify a star according to its luminosity (i.e., luminosity class, e.g., Ia, Ib, II, III, IV, or V)? (Hint: Look at the HR diagram.) Which equation relates these two quantities to the size (radius) of a star (after all, the luminosit ...
I. Parallax
... _______________. Because of Earth’s orbit around the Sun, this happens when astronomers view a “nearby” star at ___ _________________________. C. An example of this is when you hold your finger ___________ ________________and view it first with ________ and then the _________. D. The term parallax i ...
... _______________. Because of Earth’s orbit around the Sun, this happens when astronomers view a “nearby” star at ___ _________________________. C. An example of this is when you hold your finger ___________ ________________and view it first with ________ and then the _________. D. The term parallax i ...
Stellar Properties
... what would be the distance to the star? A)1/5, b)1. c)5, d)25 pc 2. Star A and B have same luminosity. If star A is 4 times closer to Earth then star B, then _____ to earthly viewer.: a=A is 4 x brighter, b=B is 4x brighter, c=A is 16 times brighter d=B is 16 times brighter, e=A is 64x brighter 3. A ...
... what would be the distance to the star? A)1/5, b)1. c)5, d)25 pc 2. Star A and B have same luminosity. If star A is 4 times closer to Earth then star B, then _____ to earthly viewer.: a=A is 4 x brighter, b=B is 4x brighter, c=A is 16 times brighter d=B is 16 times brighter, e=A is 64x brighter 3. A ...
Capella
Capella is the brightest star in the constellation Auriga, the sixth brightest in the night sky and the third brightest in the northern celestial hemisphere, after Arcturus and Vega. Its name is derived from the diminutive of the Latin capra ""goat"", hence ""little goat"". Capella also bears the Bayer designation Alpha Aurigae (often abbreviated to α Aurigae, α Aur or Alpha Aur). Although it appears to be a single star to the naked eye, it is actually a star system of four stars in two binary pairs. The first pair consists of two bright, large type-G giant stars, both with a radius around 10 times that of the Sun and two and a half times its mass, in close orbit around each other. Designated Capella Aa and Capella Ab, these two stars have both exhausted their core hydrogen fuel and become giant stars, though it is unclear exactly what stage they are on the stellar evolutionary pathway. The second pair, around 10,000 astronomical units from the first, consists of two faint, small and relatively cool red dwarfs. They are designated Capella H and Capella L. The stars labelled Capella C through to G and I through to K are actually unrelated stars in the same visual field. The Capella system is relatively close, at only 42.8 light-years (13.1 pc) from Earth.