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Chapter 28 Stars and Galaxies Reading Guide
Chapter 28 Stars and Galaxies Reading Guide

... 15. The Sun has an apparent magnitude of –26.7. A friend tells you about a star that also has a magnitude of –26.7. How could this be true? The friend can be referring to absolute magnitude and not apparent magnitude ...
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... What do scientists use to calculate distance to stars? • Because stars are so far away, astronomers use light years to measure the distance from Earth to the stars. • A light year is the distance that light travels in one year, or 186,282 miles per second, or 5.88 trillion miles**** This quasar is ...
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PHYS299B_Final_HudsonJustin

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FSA school wide Science Olympiad 12/8/2007
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... B. They are all objects for which the first detailed study was carried out by the Mauna Kea Observatory in Hawaii C. Objects which lie within 5 degrees on either side of the ecliptic, and are hence occulted by the moon at some time or the other. D. All of them lie in the Milky Way band of the sky (t ...
Characteristics of Stars
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... This is 9.5 trillion km in 1 year Proxima Centauri is 4.2 ly away or 39,900,000,000,000 km or 24.8 trillion miles  The circumference of the Earth is ~25,000 miles ...
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... between the stars. • Distance that light travels in one year. Its about 9.5 million million kilometers. That is not a typo!  ...
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... · spectrographs - device that separates light into different wavelengths (colors) · each star produces a unique spectrum (series of colors and lines) · a star's spectrum tells us elements present (composition) surface temperature how fast the star is moving toward or away from Earth ...
Lecture 6: Properties of Stars The Constellations The Constellations
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... o  Distant stars used as reference points. Closer star appears to move relative to distant stars during Earth’s orbit about Sun. o  Parallax angle: p ~ 1 AU / d => d = ~ 1 AU / p ...
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...  type of death for Massive and Giant Blue Stars. They are a ...
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ASTRONOMY 313

... 8. Astronomers investigate a region of nebulosity in the Milky Way by obtaining a spectrum of the cloud and find that the spectrum exhibits bright emission lines, most of which coincide in wavelength with those expected for lines of the Balmer series of hydrogen. What type of nebula is the cloud and ...
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... the luminosity vs. temperature of each. Temperature (spectral type) is on the horizontal axis (increasing to left) and luminosity is on the vertical axis. Accordingly, a star in the upper left is hotter and brighter than a star in the lower right. Note: When stars are plotted in this way, they fall ...
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... stars is that astronomers have a good idea about the masses of stars. The masses are usually expressed in terms of the mass of the Sun; this is called the solar mass. Obviously, the mass of the Sun is one solar mass (actually 2 x 10^30 kg ), and the masses of the other stars lie in the range of one ...
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The Brightness of Stars

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... between temperature and brightness. Identifies four characteristics of stars Temperature Brightness Color Category ...
Astronomy 162 Lab 4: Stars
Astronomy 162 Lab 4: Stars

... Magnitude is measured so that the smaller numbers correspond to the brightest objects. The Sun is by far the brightest object in the sky and has an Apparent Magnitude of about -30. The Apparent Magnitude of any object is determined by two things: the object's intrinsic brightness, and the object's d ...
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... E0102-72 is a supernova remnant in the Small Magellanic Cloud, a satellite galaxy of the Milky Way. This galaxy is 190,000 light years from Earth. E0102 -72, which is approximately a thousand years old, is believed to have resulted from the explosion of a massive star. Stretching across forty light ...
Lecture4
Lecture4

... mass star is about a million times brighter than the Sun. It has 100 times more fuel but uses it up a million times faster. It therefore lives only about 10-4 times as long as the Sun. Since the Sun lives 10 billion years, a 100 solar mass star lives only about one million years. ...
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Auriga (constellation)



Auriga is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy and remains one of the 88 modern constellations. Located north of the celestial equator, its name is the Latin word for ""charioteer"", associating it with various mythological charioteers, including Erichthonius and Myrtilus. Auriga is most prominent during winter evenings in the Northern Hemisphere, along with the five other constellations that have stars in the Winter Hexagon asterism. Because of its northern declination, Auriga is only visible in its entirety as far as 34° south; for observers farther south it lies partially or fully below the horizon. A large constellation, with an area of 657 square degrees, it is half the size of the largest constellation, Hydra.Its brightest star, Capella, is an unusual multiple star system among the brightest stars in the night sky. Beta Aurigae is an interesting variable star in the constellation; Epsilon Aurigae, a nearby eclipsing binary with an unusually long period, has been studied intensively. Because of its position near the winter Milky Way, Auriga has many bright open clusters in its borders, including M36, M37, and M38, popular targets for amateur astronomers. In addition, it has one prominent nebula, the Flaming Star Nebula, associated with the variable star AE Aurigae.In Chinese mythology, Auriga's stars were incorporated into several constellations, including the celestial emperors' chariots, made up of the modern constellation's brightest stars. Auriga is home to the radiant for the Aurigids, Zeta Aurigids, Delta Aurigids, and the hypothesized Iota Aurigids.
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