Reach for the Stars – Div. B
... Lagoon Nebula(catalogued as Messier 8 or M8, and as NGC 6523) is a giant interstellar cloud in theconstellation Sagittarius. It is classified as an emission nebula and as a H II region. • The Lagoon Nebula was discovered by Giovanni Hodierna before 1654 and is one of only two star-forming nebulae fa ...
... Lagoon Nebula(catalogued as Messier 8 or M8, and as NGC 6523) is a giant interstellar cloud in theconstellation Sagittarius. It is classified as an emission nebula and as a H II region. • The Lagoon Nebula was discovered by Giovanni Hodierna before 1654 and is one of only two star-forming nebulae fa ...
1 - BYU Physics and Astronomy
... 26. From the earth's north pole (a) the entire celestial sphere is visible at some time during the year, (b) only half the celestial sphere is visible during a year, (c) only stars within 23.5° of the celestial equator can ever be seen, (d) only stars within 66.5° of the north pole can ever be seen. ...
... 26. From the earth's north pole (a) the entire celestial sphere is visible at some time during the year, (b) only half the celestial sphere is visible during a year, (c) only stars within 23.5° of the celestial equator can ever be seen, (d) only stars within 66.5° of the north pole can ever be seen. ...
CYGNUS CONSTELLATION, the Swan Cygnus is
... Cygnus is a very large constellation. Covering 804 square degrees and around 1.9% of the night sky, Cygnus ranks 16th of the 88 constellations in size. It is bordered by Cepheus to the north and east, Draco to the north and west, Lyra to the west, Vulpecula to the south, Pegasus to the southeast and ...
... Cygnus is a very large constellation. Covering 804 square degrees and around 1.9% of the night sky, Cygnus ranks 16th of the 88 constellations in size. It is bordered by Cepheus to the north and east, Draco to the north and west, Lyra to the west, Vulpecula to the south, Pegasus to the southeast and ...
ASTR 1101-001 Spring 2008 - Louisiana State University
... • Astronomers determine the mass of a star by examining how strong the gravitational field is around that star. (Isaac Newton’s law of universal gravitation; §4-7) • By studying the motion of planets around our Sun, astronomers have determined that the Sun has a mass of 2 x 1030 kilograms. • We cann ...
... • Astronomers determine the mass of a star by examining how strong the gravitational field is around that star. (Isaac Newton’s law of universal gravitation; §4-7) • By studying the motion of planets around our Sun, astronomers have determined that the Sun has a mass of 2 x 1030 kilograms. • We cann ...
Epsilon Aurigae Mystery and Opportunity
... • Precise measurements out of eclipse revealed a quasi-periodic low amplitude variation of 96 days from 1984-87. • During the 2003-2004 observing season this variation had sped up to 71 days. • In 2007-2008 the period became 65 days. ...
... • Precise measurements out of eclipse revealed a quasi-periodic low amplitude variation of 96 days from 1984-87. • During the 2003-2004 observing season this variation had sped up to 71 days. • In 2007-2008 the period became 65 days. ...
answers
... distant objects ever found. All of the objects are galaxies of stars except for E, which is a single nearby star. Which object is more luminous? A) E B) F C) they are about the same B) The two objects look equally bright, but are very different. The star is much closer and much less luminous. The ga ...
... distant objects ever found. All of the objects are galaxies of stars except for E, which is a single nearby star. Which object is more luminous? A) E B) F C) they are about the same B) The two objects look equally bright, but are very different. The star is much closer and much less luminous. The ga ...
Jeopardy 2015
... You have been sitting out watching the star and you notice that the star you are watching has moved about 15 degrees, how long have you been watching? ...
... You have been sitting out watching the star and you notice that the star you are watching has moved about 15 degrees, how long have you been watching? ...
Set 1
... 2. The declination of a star is 42 57’ N and its proper motion components are: = -0.”0374, = 1”.21. Calculate its total proper motion. If the spectrum reveals a blueshift of 7.6 km s-1 and the parallax is 0.”376, calculate its space velocity relative to the Sun and its total proper motion at t ...
... 2. The declination of a star is 42 57’ N and its proper motion components are: = -0.”0374, = 1”.21. Calculate its total proper motion. If the spectrum reveals a blueshift of 7.6 km s-1 and the parallax is 0.”376, calculate its space velocity relative to the Sun and its total proper motion at t ...
Stars, Stellar classification, H
... Massive blue stars die first, followed by white, yellow, orange, and red stars Main-sequence turnoff ...
... Massive blue stars die first, followed by white, yellow, orange, and red stars Main-sequence turnoff ...
Skywatch Astro Ed Dec13
... of other stars, then hurled into space as the stars died, where they could be incorporated into new stars. Population II stars formed when there were almost no heavier elements around, so they have only tiny amounts of them. But Population I stars, like the Sun, are younger, so they have higher prop ...
... of other stars, then hurled into space as the stars died, where they could be incorporated into new stars. Population II stars formed when there were almost no heavier elements around, so they have only tiny amounts of them. But Population I stars, like the Sun, are younger, so they have higher prop ...
File
... 2. Which star would most likely be the brightest? Explain your answer. 3. Which star is most similar to our Sun? Explain your answer. ...
... 2. Which star would most likely be the brightest? Explain your answer. 3. Which star is most similar to our Sun? Explain your answer. ...
luminosity1
... of a star. (Along with color and Wien’s Law) • Spectral typing can also be used to find out how much of a given element is in a star. • HD 161817 has much less of all the elements, other than Hydrogen and Helium, than the Sun. • In fact, it has about 0.03 the value of the Sun for all 90 elements. Th ...
... of a star. (Along with color and Wien’s Law) • Spectral typing can also be used to find out how much of a given element is in a star. • HD 161817 has much less of all the elements, other than Hydrogen and Helium, than the Sun. • In fact, it has about 0.03 the value of the Sun for all 90 elements. Th ...
The Night Sky This Month - Usk Astronomical Society
... Some say that the constellation of the Bull was depicted in caves by humans tens of thousands of years ago to the extent that even the Pleiades were shown. What is certain is that Taurus the Bull, with the Scorpion and the Lion, was portrayed over 6000 years ago in the Euphrates Valley, in ancient M ...
... Some say that the constellation of the Bull was depicted in caves by humans tens of thousands of years ago to the extent that even the Pleiades were shown. What is certain is that Taurus the Bull, with the Scorpion and the Lion, was portrayed over 6000 years ago in the Euphrates Valley, in ancient M ...
A little bit more to do. Stefan
... of a star. (Along with color and Wien’s Law) • Spectral typing can also be used to find out how much of a given element is in a star. • HD 161817 has much less of all the elements, other than Hydrogen and Helium, than the Sun. • In fact, it has about 0.03 the value of the Sun for all 90 elements. Th ...
... of a star. (Along with color and Wien’s Law) • Spectral typing can also be used to find out how much of a given element is in a star. • HD 161817 has much less of all the elements, other than Hydrogen and Helium, than the Sun. • In fact, it has about 0.03 the value of the Sun for all 90 elements. Th ...
Lecture 17: General Relativity and Black Holes
... 38. In the center of our galaxy there is probably: a. globular cluster b. black hole c. open cluster d. another small galaxy e. none of these 33. The approximate number of stars in our galaxy? _______ 24. The approximate diameter of our own galaxy? _______ 25. The galactic north pole is in what cons ...
... 38. In the center of our galaxy there is probably: a. globular cluster b. black hole c. open cluster d. another small galaxy e. none of these 33. The approximate number of stars in our galaxy? _______ 24. The approximate diameter of our own galaxy? _______ 25. The galactic north pole is in what cons ...
Astro 18 – Section Week 2
... The deeper absorption line at 760nm is caused by our atmosphere's oxygen molecule. The two absorption lines at 720 and 890nm (from methane) appear on Saturn and Titan, but the rings do not have them ...
... The deeper absorption line at 760nm is caused by our atmosphere's oxygen molecule. The two absorption lines at 720 and 890nm (from methane) appear on Saturn and Titan, but the rings do not have them ...
Astro 18 – Section Week 2
... The deeper absorption line at 760nm is caused by our atmosphere's oxygen molecule. The two absorption lines at 720 and 890nm (from methane) appear on Saturn and Titan, but the rings do not have them ...
... The deeper absorption line at 760nm is caused by our atmosphere's oxygen molecule. The two absorption lines at 720 and 890nm (from methane) appear on Saturn and Titan, but the rings do not have them ...
Distances farther out
... UV Mg II lines at λ2796 & 2802 (h & k lines, visible only from satellite borne telescopes) - also exhibit self absorption. Wilson Bappu effect: 1956, Wilson & Bappu at Mt Wilson: Width of K2 line correlates very well with visual magnitude of classes G, K, M from dwarfs through supergiants over a mag ...
... UV Mg II lines at λ2796 & 2802 (h & k lines, visible only from satellite borne telescopes) - also exhibit self absorption. Wilson Bappu effect: 1956, Wilson & Bappu at Mt Wilson: Width of K2 line correlates very well with visual magnitude of classes G, K, M from dwarfs through supergiants over a mag ...
U7 Review WS KEY
... and brightness. Sirius B: low M, mid-range T; Capella: mid-range M, low T; Spica: high M, high T; Deneb: high M, mid-range T **On what part of the H-R diagram would you find the majority of the main-sequence stars? mid-range M and T **Define luminosity and absolute magnitude. luminosity: how much en ...
... and brightness. Sirius B: low M, mid-range T; Capella: mid-range M, low T; Spica: high M, high T; Deneb: high M, mid-range T **On what part of the H-R diagram would you find the majority of the main-sequence stars? mid-range M and T **Define luminosity and absolute magnitude. luminosity: how much en ...
Evolution of Stars and Galaxies
... when gravity holds together a large collection of stars, gas, and dust ...
... when gravity holds together a large collection of stars, gas, and dust ...
NASC 1100
... A Star’s Infancy A star is born when its core temperature exceeds 10 million K hydrogen fusion begins. The star’s interior stabilizes: thermal energy generated by fusion maintains the balance between gravity and pressure. The star becomes a main-sequence star. ...
... A Star’s Infancy A star is born when its core temperature exceeds 10 million K hydrogen fusion begins. The star’s interior stabilizes: thermal energy generated by fusion maintains the balance between gravity and pressure. The star becomes a main-sequence star. ...
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.