Star and Galaxies
... • During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
... • During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
Volcanoes and Igneous Activity Earth
... • During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
... • During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
Habitibility of Earth, in our Solar System, and Beyond
... Half again as big as Earth, 5 times more massive Surface T at 0 - 40°C. !!! Surface G is 2.2 x Earth. ...
... Half again as big as Earth, 5 times more massive Surface T at 0 - 40°C. !!! Surface G is 2.2 x Earth. ...
Name
... 1. In Hershey, PA (40 N Latitude) from which direction will the Sun rise above the horizon on the Summer Solstice? ...
... 1. In Hershey, PA (40 N Latitude) from which direction will the Sun rise above the horizon on the Summer Solstice? ...
Astronomy Exam #2 for the 10
... The hot main sequence stars appear to be mostly B and A spectral type with an absolute magnitude between +2 and -5. This range in absolute magnitudes corresponds to a range in luminosity of between 16 and 10,000 solar luminosities. These stars will have a short main sequence lifetime compared to the ...
... The hot main sequence stars appear to be mostly B and A spectral type with an absolute magnitude between +2 and -5. This range in absolute magnitudes corresponds to a range in luminosity of between 16 and 10,000 solar luminosities. These stars will have a short main sequence lifetime compared to the ...
Answers to Coursebook questions – Chapter E3
... Star B has a larger parallax, so it is closer. Hence it appears brighter. ...
... Star B has a larger parallax, so it is closer. Hence it appears brighter. ...
Name the eight planets in order by increasing distance from the sun:
... 8-Which of the geocentric, heliocentric models of our solar systems shows the sun as the center of our solar system? A: heliocentric 9-Which of the geocentric, heliocentric models of our solar systems do we support today? A: heliocentric 10-What are the four main components that make up our solar sy ...
... 8-Which of the geocentric, heliocentric models of our solar systems shows the sun as the center of our solar system? A: heliocentric 9-Which of the geocentric, heliocentric models of our solar systems do we support today? A: heliocentric 10-What are the four main components that make up our solar sy ...
Star in a Box Worksheet - Beginning with solutions
... 1. What stages of their lives are the two stars in? Deneb is between the main sequence and the Hertzsprung Gap. Betelgeuse is between the Hertzsprung Gap and core helium burning. 2. How long does each star have to live? D eneb has about 1 million years left to live and Betelgeuse has about 400 th ...
... 1. What stages of their lives are the two stars in? Deneb is between the main sequence and the Hertzsprung Gap. Betelgeuse is between the Hertzsprung Gap and core helium burning. 2. How long does each star have to live? D eneb has about 1 million years left to live and Betelgeuse has about 400 th ...
How Bright is that star?
... Relates luminosity, temperature and Radius of a star. The luminosity/meter² (l), is determined by the temperature (T) of that area ) l = σT⁴ (σ is a constant which if T is in °K, l comes out in Watts) Surface area is determined by radius(R): A = 4πR² So the total Lumnosity of star becomes L = 4πR²σT ...
... Relates luminosity, temperature and Radius of a star. The luminosity/meter² (l), is determined by the temperature (T) of that area ) l = σT⁴ (σ is a constant which if T is in °K, l comes out in Watts) Surface area is determined by radius(R): A = 4πR² So the total Lumnosity of star becomes L = 4πR²σT ...
Teaching ideas for Option E, Astrophysics
... is no interesting story behind this though; they started as A, B, etc. but were later reordered. Students find the story of the Eddington/Chandrasekhar controversy about collapsed stars interesting and it is worth spending some time on it. Freeman Dyson’s obituary of Chandrasekhar, in Nature, 438, 1 ...
... is no interesting story behind this though; they started as A, B, etc. but were later reordered. Students find the story of the Eddington/Chandrasekhar controversy about collapsed stars interesting and it is worth spending some time on it. Freeman Dyson’s obituary of Chandrasekhar, in Nature, 438, 1 ...
Name: Period : _____ Bulldog Review #9 1. The Milky Wa
... C. Gravity is the force that is formed in the crust of the planet and it holds objects to the surface of the Earth. D. Gravity is the natural force that causes objects to move toward the center of the Earth. 7. Light travels at a constant speed of about 300,000 km/s. This speed is referred to as the ...
... C. Gravity is the force that is formed in the crust of the planet and it holds objects to the surface of the Earth. D. Gravity is the natural force that causes objects to move toward the center of the Earth. 7. Light travels at a constant speed of about 300,000 km/s. This speed is referred to as the ...
the May 2017 Newsletter!
... very close, the star could quite easily be seen as double in a 6 inch telescope. Other double stars were Castor and Alpha Centauri. Both of the latter have recently opened up from a close approach as viewed from Earth – Castor closed up for about 30 years. (See footnote 1); the Alpha Centauri pair a ...
... very close, the star could quite easily be seen as double in a 6 inch telescope. Other double stars were Castor and Alpha Centauri. Both of the latter have recently opened up from a close approach as viewed from Earth – Castor closed up for about 30 years. (See footnote 1); the Alpha Centauri pair a ...
General Astronomy - Stockton University
... The components periodically eclipse one another, causing a decrease in the apparent brightness of the system as seen by the observer. The period of the eclipse, which coincides with the orbital period of the system, can range from minutes to years. ...
... The components periodically eclipse one another, causing a decrease in the apparent brightness of the system as seen by the observer. The period of the eclipse, which coincides with the orbital period of the system, can range from minutes to years. ...
Day 1212
... The outer layers expand and cool. In this late stage of its life cycle, an average star like our Sun is called a giant. ...
... The outer layers expand and cool. In this late stage of its life cycle, an average star like our Sun is called a giant. ...
Can you write numbers in scientific notation
... What determines what object will be left behind after a star dies out? What are the properties of each of those objects? How does Einstein’s model of gravity differ from Newton’s description? Why Einstein’s description taken to be “more complete” than Newton’s? What are the effects an outside obser ...
... What determines what object will be left behind after a star dies out? What are the properties of each of those objects? How does Einstein’s model of gravity differ from Newton’s description? Why Einstein’s description taken to be “more complete” than Newton’s? What are the effects an outside obser ...
Aug14Guide - East-View
... The Moon is at first quarter on the 4th, full on the 10th, at last quarter on the 17th and new on the 25th. A talk entitled ‘Great Moments in Astronomy’ will be given by Ken Kennedy of Dundee Astronomical Society on Sunday, 10th August at 1.30pm at Mills Observatory. The talk will be a personal sele ...
... The Moon is at first quarter on the 4th, full on the 10th, at last quarter on the 17th and new on the 25th. A talk entitled ‘Great Moments in Astronomy’ will be given by Ken Kennedy of Dundee Astronomical Society on Sunday, 10th August at 1.30pm at Mills Observatory. The talk will be a personal sele ...
Postgraduate Seminar Series Small Angle Neutron scattering on the anisotropic superconductor CaC6.
... By Lieke van Spaandonk A Cataclysmic Variable (CV) is a binary star system where two stars orbit each other around their centre of mass. The primary is the more massive star of the system and will have evolved into a white dwarf (compact degenerate star), while the secondary is still a main sequence ...
... By Lieke van Spaandonk A Cataclysmic Variable (CV) is a binary star system where two stars orbit each other around their centre of mass. The primary is the more massive star of the system and will have evolved into a white dwarf (compact degenerate star), while the secondary is still a main sequence ...
Astronomy
... Please do not write on this test 15. The magnitude scale a. originated just after the telescope was invented. b. can be used to indicate the apparent brightness of a celestial object. c. was devised by Newton. d. is no longer used today. 16. For an observer in the southern latitude -60o, the star P ...
... Please do not write on this test 15. The magnitude scale a. originated just after the telescope was invented. b. can be used to indicate the apparent brightness of a celestial object. c. was devised by Newton. d. is no longer used today. 16. For an observer in the southern latitude -60o, the star P ...
AST 1010 Quiz questions
... 2. Canopus, a bright star in our sky, has an apparent magnitude of -0.62. The star is located 96 pc from Earth. Would the absolute magnitude of Canopus be greater or less than the apparent magnitude? Explain. 3. The star Vega has an apparent magnitude of +0.03 and an absolute magnitude of +0.58. Is ...
... 2. Canopus, a bright star in our sky, has an apparent magnitude of -0.62. The star is located 96 pc from Earth. Would the absolute magnitude of Canopus be greater or less than the apparent magnitude? Explain. 3. The star Vega has an apparent magnitude of +0.03 and an absolute magnitude of +0.58. Is ...
Powerpoint Presentation (large file)
... By carefully examining a star’s spectral lines, astronomers can determine whether that star is a main-sequence star, giant, supergiant, or white dwarf ...
... By carefully examining a star’s spectral lines, astronomers can determine whether that star is a main-sequence star, giant, supergiant, or white dwarf ...
Study Guide: Unit 1, The Universe and its Stars, HS
... Directions: Choose the alternative that best completes the statement or answers the question. 1) HS-ESS1-2 Which of the following colors has the longest wavelength? A) violet B) red C) orange D) green E) blue 2) HS-ESS1-2 Which of the following is NOT considered a form of electromagnetic radiation? ...
... Directions: Choose the alternative that best completes the statement or answers the question. 1) HS-ESS1-2 Which of the following colors has the longest wavelength? A) violet B) red C) orange D) green E) blue 2) HS-ESS1-2 Which of the following is NOT considered a form of electromagnetic radiation? ...
Perseus (constellation)
Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.