WHAT IS A STAR? - cloudfront.net
... If you remember feeling hot or pressured, this is similar to what happens to hydrogen atoms in the core of a star, where the temperature and pressure are very high. ...
... If you remember feeling hot or pressured, this is similar to what happens to hydrogen atoms in the core of a star, where the temperature and pressure are very high. ...
Stars - TeacherWeb
... • any object 15 to 75 times the mass of Jupiter • the object would not have been able to sustain fusion like a regular star - called "failed stars" • all are parts of a binary system. (two stars orbit around one another) • possible that brown dwarfs represent a lot of the mass in the universe ...
... • any object 15 to 75 times the mass of Jupiter • the object would not have been able to sustain fusion like a regular star - called "failed stars" • all are parts of a binary system. (two stars orbit around one another) • possible that brown dwarfs represent a lot of the mass in the universe ...
Name: Period : ______ The Universe – Life and Death of a Star How
... 22. What does all that extra heat cause the Sun-like star to do? 23. When a Sun-like star begins to eject its outer layers of gas in “cosmic burps” it will send shells of gas illuminated by the hot central star and that will cause the __________________ nebula phenomenon. 24. When a star cools, it c ...
... 22. What does all that extra heat cause the Sun-like star to do? 23. When a Sun-like star begins to eject its outer layers of gas in “cosmic burps” it will send shells of gas illuminated by the hot central star and that will cause the __________________ nebula phenomenon. 24. When a star cools, it c ...
SHORT ANSWER. Answer the questions, showingh your work for
... a. If there were no air resistance, so that the mass falls with the acceleration of gravity ge=10 m/s2, about how fast (in m/s) would it be going when it hit the ground? ...
... a. If there were no air resistance, so that the mass falls with the acceleration of gravity ge=10 m/s2, about how fast (in m/s) would it be going when it hit the ground? ...
Ch. 28 Test Topics
... -Define binary star system. -Know that this is the order of objects in the universe from smallest to largest: planet, solar system, star, star cluster, galaxy, galaxy cluster, super cluster -Know a local group of galaxies are galaxies that are in the close by each other and in our galaxy cluster. Th ...
... -Define binary star system. -Know that this is the order of objects in the universe from smallest to largest: planet, solar system, star, star cluster, galaxy, galaxy cluster, super cluster -Know a local group of galaxies are galaxies that are in the close by each other and in our galaxy cluster. Th ...
What do we see in the night sky - Laureate International College
... AUs are not sufficient. A light-year is ____________________________________________. Light travels at a speed of ____________________ – the fastest! One light year covers _________________ km. Most stars and galaxies are hundreds, thousands and even millions of light-years away! ...
... AUs are not sufficient. A light-year is ____________________________________________. Light travels at a speed of ____________________ – the fastest! One light year covers _________________ km. Most stars and galaxies are hundreds, thousands and even millions of light-years away! ...
Homework 5 (stellar properties)
... 7. (5 pts.) List the information we can get from an eclipsing binary star. (5 things, note: 5 things for each star – so don’t list “x” for star “a,” “x” for star “b,” etc.) ...
... 7. (5 pts.) List the information we can get from an eclipsing binary star. (5 things, note: 5 things for each star – so don’t list “x” for star “a,” “x” for star “b,” etc.) ...
W > 1 - The Open University
... IC = Index Catalogue. (Extension of the NGC). ds = double star. ms = multiple star. gc = globular cluster. oc = open cluster. pn = planetary nebula. en = emission nebula. rn = reflection nebula. sg = spiral galaxy. eg = elliptical galaxy. lg = lenticular galaxy. ir = irregular galaxy. pg = peculiar ...
... IC = Index Catalogue. (Extension of the NGC). ds = double star. ms = multiple star. gc = globular cluster. oc = open cluster. pn = planetary nebula. en = emission nebula. rn = reflection nebula. sg = spiral galaxy. eg = elliptical galaxy. lg = lenticular galaxy. ir = irregular galaxy. pg = peculiar ...
Name: ____________ Period: ______ STAR BIOGRAPHY Name of
... *May include diagram *Talk about the birth of your star, include its age if known, what life cycle it is in, and predict what will happen in the future with your star. (Include each Life Cycle Stage) ...
... *May include diagram *Talk about the birth of your star, include its age if known, what life cycle it is in, and predict what will happen in the future with your star. (Include each Life Cycle Stage) ...
It is evident from our observations of impact craters on planets and
... The presence of spectral features and dominance of certain lines is closely linked to surface temperature and conditions in the stellar atmosphere. Astronomers have based a classification system for stars based on the spectrum. Spectroscopic parallax using the distance modulus can be used to determi ...
... The presence of spectral features and dominance of certain lines is closely linked to surface temperature and conditions in the stellar atmosphere. Astronomers have based a classification system for stars based on the spectrum. Spectroscopic parallax using the distance modulus can be used to determi ...
Astronomy 2
... uses data from lots of stars, so there are lots of dots. The position of each dot on the diagram corresponds to the star's luminosity and its temperature The vertical position represents the star's luminosity (absolute magnitude). The horizontal position represents the star's surface temperature ...
... uses data from lots of stars, so there are lots of dots. The position of each dot on the diagram corresponds to the star's luminosity and its temperature The vertical position represents the star's luminosity (absolute magnitude). The horizontal position represents the star's surface temperature ...
- ALMA Observatory
... Have you ever pulled a loose thread on your sweater, only to find that it has no end? Astronomers have observed a similar phenomenon in space! Two stars orbit around each other, in what is called a binary ...
... Have you ever pulled a loose thread on your sweater, only to find that it has no end? Astronomers have observed a similar phenomenon in space! Two stars orbit around each other, in what is called a binary ...
Stellar Evolution Slideshow
... only neutrons are left (Guess where the name “Neutron Stars” came from?) Also called Pulsars because they emit radio waves with incredible regularity. Appear to be rapidly rotating neutron star ...
... only neutrons are left (Guess where the name “Neutron Stars” came from?) Also called Pulsars because they emit radio waves with incredible regularity. Appear to be rapidly rotating neutron star ...
Read
... Spectral type – Indicates the color of the star, which is related to its surface temperature. From the hottest to coolest, also from blue to red color, the types are: O, B, A, F, G, K, M. A second number is added for finer classification, like G0, G1, G2, …, G9. A blue star is hotter than a yellow s ...
... Spectral type – Indicates the color of the star, which is related to its surface temperature. From the hottest to coolest, also from blue to red color, the types are: O, B, A, F, G, K, M. A second number is added for finer classification, like G0, G1, G2, …, G9. A blue star is hotter than a yellow s ...
WK10revisedoneweek
... •A comparison of the evolution and fate of high and low mass stars. •A description of Einstein’s Principle of Equivalence, its effects, and predictions regarding Black Holes. •Give a brief summary of each of the popular possibilities for the fate of our universe, and suggest the evidence that may su ...
... •A comparison of the evolution and fate of high and low mass stars. •A description of Einstein’s Principle of Equivalence, its effects, and predictions regarding Black Holes. •Give a brief summary of each of the popular possibilities for the fate of our universe, and suggest the evidence that may su ...
An Assessment: Think Pair Share
... becomes much brighter because it is 1. moving closer to us. 2. losing its outer envelope. 3. fusing iron in its core. 4. increasing in size. ...
... becomes much brighter because it is 1. moving closer to us. 2. losing its outer envelope. 3. fusing iron in its core. 4. increasing in size. ...
Mountain Skies - Pisgah Astronomical Research Institute
... compiled a little over 200 years ago by the French comet hunter Charles Messier. His catalog, ironically, was a list of objects not to look at if you were looking for comets. Generally, when comets are first discovered optically, they ...
... compiled a little over 200 years ago by the French comet hunter Charles Messier. His catalog, ironically, was a list of objects not to look at if you were looking for comets. Generally, when comets are first discovered optically, they ...
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.