The Inverse Square Law and Surface Area
... The power received from a star per metre squared at the Earth is called the intensity (I) of the star’s radiation This is related to the power output per metre squared L of the star’s surface in this way ...
... The power received from a star per metre squared at the Earth is called the intensity (I) of the star’s radiation This is related to the power output per metre squared L of the star’s surface in this way ...
The Assembly of M31`s Halo from Dwarf Galaxy Building Blocks
... B. The typical photon emitted by star X has a lower energy than the typical photon emitted by the Sun C. Star X is reddish in color whereas the Sun is yellowish white D. If both stars were at the same distance from us, the Sun would ...
... B. The typical photon emitted by star X has a lower energy than the typical photon emitted by the Sun C. Star X is reddish in color whereas the Sun is yellowish white D. If both stars were at the same distance from us, the Sun would ...
The Sun and Other Stars - Tuslaw Local School District
... * 5 x’s the mass of the sun, 30 km in diameter * the gravity is so strong nothing can escape including light! ...
... * 5 x’s the mass of the sun, 30 km in diameter * the gravity is so strong nothing can escape including light! ...
Slide 1
... they run out of nuclear fuel.. Typically 1,000 times the size of our solar system These Ten have names like Owl, the Cat's Eye, the Ghost of Jupiter, Ring. This glorious final phase in the life of a star lasts only about 10,000 yrs. ...
... they run out of nuclear fuel.. Typically 1,000 times the size of our solar system These Ten have names like Owl, the Cat's Eye, the Ghost of Jupiter, Ring. This glorious final phase in the life of a star lasts only about 10,000 yrs. ...
Universe 8e Lecture Chapter 17 Nature of Stars
... above the main sequence, while white dwarfs are below the main sequence. By carefully examining a star’s spectral lines, astronomers can determine whether that star is a mainsequence star, giant, supergiant, or white dwarf. Using the H-R diagram and the inverse square law, the star’s luminosity and ...
... above the main sequence, while white dwarfs are below the main sequence. By carefully examining a star’s spectral lines, astronomers can determine whether that star is a mainsequence star, giant, supergiant, or white dwarf. Using the H-R diagram and the inverse square law, the star’s luminosity and ...
Our Community`s Place Among the Stars
... four hydrogen atoms fuse together to make one helium atom in a star’s core Some mass is “lost” in the reaction, because one helium atom has less mass than four hydrogen ...
... four hydrogen atoms fuse together to make one helium atom in a star’s core Some mass is “lost” in the reaction, because one helium atom has less mass than four hydrogen ...
8hrdiagram1s
... If you know the luminosity and you measure the flux you can find the distance (F = L/4pd2) Called spectroscopic parallax ...
... If you know the luminosity and you measure the flux you can find the distance (F = L/4pd2) Called spectroscopic parallax ...
Astrophysics
... system which ranks them in order of surface temperature (the letters were re-ordered from an older system): ...
... system which ranks them in order of surface temperature (the letters were re-ordered from an older system): ...
Star Life Guided Notes
... star _________ yet…. Expanded surface is actually “_______” so appears _____ ...
... star _________ yet…. Expanded surface is actually “_______” so appears _____ ...
Constellations
... • The constellations that lie along the ecliptic are called the zodiac. – 12 constellations ...
... • The constellations that lie along the ecliptic are called the zodiac. – 12 constellations ...
Classifying Stars - Concord Academy Boyne
... What is Stellar Classification? The classification of stars is based on the elements they absorb and their temperature, and are listed from hottest to coldest ...
... What is Stellar Classification? The classification of stars is based on the elements they absorb and their temperature, and are listed from hottest to coldest ...
doc
... Final Jeopardy: The Origin of the Elements -----------------------------------------An element, and the process or object which ultimately created it. ...
... Final Jeopardy: The Origin of the Elements -----------------------------------------An element, and the process or object which ultimately created it. ...
Hertzsprung-Russell Diagram
... The Main Sequence At one end, the stars are big, hot and bright. Due to their color and size they are called blue giants, and the very largest are blue supergiants. At the other end they are small, cool and dim and are known as red dwarfs. The sun is right in the middle. ...
... The Main Sequence At one end, the stars are big, hot and bright. Due to their color and size they are called blue giants, and the very largest are blue supergiants. At the other end they are small, cool and dim and are known as red dwarfs. The sun is right in the middle. ...
Loving The Universe
... “… then God formed the earthling from the dust of the ground, breathed into it the breath of life, and the earthling became a living being …” ...
... “… then God formed the earthling from the dust of the ground, breathed into it the breath of life, and the earthling became a living being …” ...
No Slide Title
... The neutron star may continue to gain mass from nearby stars. At a critical moment, it becomes so dense it collapses in on itself, becoming a single point of zero size! Its gravity is so strong that even light cannot escape from inside a certain boundary - the EVENT HORIZON. The star is now a BLACK ...
... The neutron star may continue to gain mass from nearby stars. At a critical moment, it becomes so dense it collapses in on itself, becoming a single point of zero size! Its gravity is so strong that even light cannot escape from inside a certain boundary - the EVENT HORIZON. The star is now a BLACK ...
Stellar evolution, II
... mass of Sun = 2 X 1030 kg 0.007 of mass of hydrogen is converted into energy 0.1 of mass of Sun (the core) is converted in He Total energy liberated by Sun during main sequence phase is (2 X 1030) X 0.007 X 0.1 X c2 = 1.26 X 1044 J. Luminosity of Sun = 3.8 X 1026 Joules/sec ...
... mass of Sun = 2 X 1030 kg 0.007 of mass of hydrogen is converted into energy 0.1 of mass of Sun (the core) is converted in He Total energy liberated by Sun during main sequence phase is (2 X 1030) X 0.007 X 0.1 X c2 = 1.26 X 1044 J. Luminosity of Sun = 3.8 X 1026 Joules/sec ...
HR DIAGRAM ACTIVITY
... Analysis- use pages 627-628 to help you You can check your HR diagram at: http://deskarati.com/wp-content/uploads/2012/03/HertzsprungRussell-Diagram.jpg 1. Draw a circle around all the red giants on your graph and label this enclosed area Red Giants. 2. Draw a circle around all the white dwarfs and ...
... Analysis- use pages 627-628 to help you You can check your HR diagram at: http://deskarati.com/wp-content/uploads/2012/03/HertzsprungRussell-Diagram.jpg 1. Draw a circle around all the red giants on your graph and label this enclosed area Red Giants. 2. Draw a circle around all the white dwarfs and ...
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.