The most important questions to study for the exam
... 13. How do astronomers measure the luminosity class of a star? • From the observed size of the star • From the brightness of the star in the sky • From the absorption lines in the star's spectrum 14. Aldebaran, a star in the constellation Taurus, has a spectral-luminosity class of K5 III. This tell ...
... 13. How do astronomers measure the luminosity class of a star? • From the observed size of the star • From the brightness of the star in the sky • From the absorption lines in the star's spectrum 14. Aldebaran, a star in the constellation Taurus, has a spectral-luminosity class of K5 III. This tell ...
PDF version (two pages, including the full text)
... Southern Cross and the Pointers (Alpha and Beta Centauri). Alpha Centauri is a triple system, with two sun like stars orbiting each other every 80 years and a dim red dwarf tagging along at a much larger distance. This star was discovered by Robert Innes at the Union Observatory in Johannesburg in 1 ...
... Southern Cross and the Pointers (Alpha and Beta Centauri). Alpha Centauri is a triple system, with two sun like stars orbiting each other every 80 years and a dim red dwarf tagging along at a much larger distance. This star was discovered by Robert Innes at the Union Observatory in Johannesburg in 1 ...
Winter Stargazing - Trimble County Schools
... • Follow the line to the southeast, and you will see Sirius perched right below it. • Sirius is the nose of the dog. • His body stretches to the southeast, and his front leg is to the west of Sirius. ...
... • Follow the line to the southeast, and you will see Sirius perched right below it. • Sirius is the nose of the dog. • His body stretches to the southeast, and his front leg is to the west of Sirius. ...
1 - Quia
... 3. Spiral galaxies often appear bluish due to an abundance of a. old stars. c. young stars. b. black holes. d. white dwarfs. 4. Galaxies are classified based on their a. shape. b. color. ...
... 3. Spiral galaxies often appear bluish due to an abundance of a. old stars. c. young stars. b. black holes. d. white dwarfs. 4. Galaxies are classified based on their a. shape. b. color. ...
Exploring the Universe
... 1. H-R diagrams are used to estimate the sizes of stars and their distances, and to infer how stars change over time a. Horizontal axis=surface temperature b. Vertical axis=absolute brightness ...
... 1. H-R diagrams are used to estimate the sizes of stars and their distances, and to infer how stars change over time a. Horizontal axis=surface temperature b. Vertical axis=absolute brightness ...
Astronomy 20 Homework # 5 1.
... (a) Derive a formula for the b.h. luminosity as a function of its mass, assuming that its eective area is 4RS2 , where RS is the Schwarzschild radius. (b) By setting L = c2 dM=dt, derive and solve the dierential equation for the evaporation time of a black hole with an initial mass of M0 . (c) E ...
... (a) Derive a formula for the b.h. luminosity as a function of its mass, assuming that its eective area is 4RS2 , where RS is the Schwarzschild radius. (b) By setting L = c2 dM=dt, derive and solve the dierential equation for the evaporation time of a black hole with an initial mass of M0 . (c) E ...
Activity: Star Classification - d
... Part 1: Exploring with Classification Each group will receive 1 set of 27 stars. Every star has: a color, name, temperature, size, & luminosity value o The luminosity is compared to the sun's luminosity. If a star has a luminosity value of 5, then it is 5 times brighter than our sun. If a star h ...
... Part 1: Exploring with Classification Each group will receive 1 set of 27 stars. Every star has: a color, name, temperature, size, & luminosity value o The luminosity is compared to the sun's luminosity. If a star has a luminosity value of 5, then it is 5 times brighter than our sun. If a star h ...
Sun - TeacherWeb
... http://scifiles.larc.nasa.gov/text/kids/Problem_Board/problems/sound/sound_waves2.html ...
... http://scifiles.larc.nasa.gov/text/kids/Problem_Board/problems/sound/sound_waves2.html ...
Stellar Physics Lecture 1
... – bv /bb and bb /bu <1 with bb /bu < bv /bb hot, blue star, T >20000 K. – bv /bb and bb /bu roughly equal and ~1 cooler, white star, T ~9000 K. – bv /bb and bb /bu >1 with bb /bu > bv /bb cool, orange/red star T <4000 K. ...
... – bv /bb and bb /bu <1 with bb /bu < bv /bb hot, blue star, T >20000 K. – bv /bb and bb /bu roughly equal and ~1 cooler, white star, T ~9000 K. – bv /bb and bb /bu >1 with bb /bu > bv /bb cool, orange/red star T <4000 K. ...
Document
... radial velocity perturbations of central star. e.g. an Earth size planet orbiting Alpha Centauri B.- about 3.5ly distant; a star with a surface temperature of ~5200 K) ...
... radial velocity perturbations of central star. e.g. an Earth size planet orbiting Alpha Centauri B.- about 3.5ly distant; a star with a surface temperature of ~5200 K) ...
Document
... bright it looks from Earth, you can determine how far away it must be to look that faint. • For any star in the sky, we KNOW: – Apparent Magnitude (m) – Spectral Type (O, B, A, F, G, K, M) – Luminosity Class (Main Sequence, Giant, etc…). These are denoted by a roman numeral (V, III, I,…). ...
... bright it looks from Earth, you can determine how far away it must be to look that faint. • For any star in the sky, we KNOW: – Apparent Magnitude (m) – Spectral Type (O, B, A, F, G, K, M) – Luminosity Class (Main Sequence, Giant, etc…). These are denoted by a roman numeral (V, III, I,…). ...
powerpoint - Physics @ IUPUI
... • RR Lyrae have an average absolute magnitude of 0.75. • Why is that an advantage? • What is the disadvantage if you are looking at other galaxies? ...
... • RR Lyrae have an average absolute magnitude of 0.75. • Why is that an advantage? • What is the disadvantage if you are looking at other galaxies? ...
Ursa Minor
Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.