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... conservation of angular momentum. This is faster than any known (or possible) neutron star. Mass and angular momentum are lost during the collapse. ...
S1_LectureOutlines
S1_LectureOutlines

... • It is also known as Greenwich Mean Time (GMT) because 0° longitude is defined to pass through Greenwich, England • It is the standard time used for astronomy and navigation around the world ...
ABC`s of the Sky - Northern Stars Planetarium
ABC`s of the Sky - Northern Stars Planetarium

Sermon Notes
Sermon Notes

a new isotopic abundance anomaly in chemically peculiar stars
a new isotopic abundance anomaly in chemically peculiar stars

Ch 11c and 12 ( clusters 3-31-11)
Ch 11c and 12 ( clusters 3-31-11)

... becomes a protostar surrounded by a spinning disk of gas. • When core gets hot enough (10 million K), fusion of hydrogen begins and stops the shrinking • New star achieves long-lasting state of balance (main sequence ...
Excerpt from Aristotle`s “On the Heavens”
Excerpt from Aristotle`s “On the Heavens”

Measuring colour in astronomy
Measuring colour in astronomy

... body emits more radiation at any given temperature than any other object. (In reality there is no such thing as a perfectly black body, but there are objects which come very close to this theoretical ideal.) Other stars have spectra which are also close to being black body spectra. On a dark night i ...
End of the line for a star like ours
End of the line for a star like ours

Circular ac
Circular ac

BROCK UNIVERSITY Return both the exam script
BROCK UNIVERSITY Return both the exam script

... (b) to stake claims on various parts of the heavens in the names of certain mythological gods and goddesses. (c) to honour important writers, artists, and politicians. (d) as aids in navigation and for keeping track of seasons. 19. The main reason that the Earth has a significant atmosphere and the ...
Dynamite Diameters
Dynamite Diameters

...  e.g.: if you use spectroscopic log g and interferometric radius to derive a mass, then the star appears too massive  Radius is under-estimated  Age is under-estimated ...
Astrophysics
Astrophysics

EF Eri: Its White Dwarf Primary and L Dwarf Secondary
EF Eri: Its White Dwarf Primary and L Dwarf Secondary

... --> Polar or AM Herculis type. These contain no accretion disk. ...
From Simulation to Visualization: Astrophysics Goes
From Simulation to Visualization: Astrophysics Goes

... Data - N-body simulation, 6144 stars (Zwart)  3D position, absolute brightness, mass, & type  color derived from mass, type, and spectra* Stars as point objects  size depends on apparent brightness  size calculated in pixels, not 3D space Star shader in renderman  calculate app. brightness - ea ...
The Formation of Stars and Solar Systems
The Formation of Stars and Solar Systems

... Giant Molecular Clouds • Some parts of space, however, are not wide open frontiers containing a few atoms. These cosmic spaces comprise dense clouds of dust and gas left over from galaxy formation. • Since these clouds are cooler than most places, they are perfect breeding grounds for star birth. W ...
Space ppt
Space ppt

... What is a Galaxy? • Galaxy: A giant structure that contains hundreds of billions of stars bound together by gravity. • Spiral Galaxy: A galaxy whose arms curve outward in a pinwheel pattern. Contains solar systems and nebulae (gas, new stars, and dust). • Irregular Galaxy: A galaxy that does not ha ...
Stars, Galaxies, and the Universe Section 1 Section 1
Stars, Galaxies, and the Universe Section 1 Section 1

... from Earth, is caused by the movement of Earth. • The stars seem as though they are moving counterclockwise around a central star called Polaris, the North Star. Polaris is almost directly above the North Pole, and thus the star does not appear to move much. • Earth’s revolution around the sun cause ...
Neutron Stars
Neutron Stars

... • It reaches a peak luminosity of about 105 Lsun • A nova is different from supernova (luminosity of 109 Lsun) • Material from an ordinary star in a close binary can fall onto the surface of the companion white dwarf • Because of strong gravity, the transferred hydrogen mass is compressed into a den ...
AST 341 - Homework IV - Solutions
AST 341 - Homework IV - Solutions

Testing - Montgomery College
Testing - Montgomery College

... • It is also known as Greenwich Mean Time (GMT) because 0° longitude is defined to pass through Greenwich, England • It is the standard time used for astronomy and navigation around the world ...
Can we detect asteroid impacts with rocky extrasolar planets?
Can we detect asteroid impacts with rocky extrasolar planets?

... solar system, so we can expect one to be hit every 25 million years. However, half of these impacts will be on the side facing away from the Earth so a visible impact occurs, on average, once every 50 million years. During the first billion years of our solar system, though, the impact rate was at l ...
V = 3 d3 = 4188.8 pc N = ρV = 0.1 pc χ 4188.8 pc = 419
V = 3 d3 = 4188.8 pc N = ρV = 0.1 pc χ 4188.8 pc = 419

... M = M Sun   = M Sun   = (0.15) M Sun ≈ 1.9M Sun .  10Gyr   LifetimeSun  Since more massive stars have shorter lifetimes, we conclude that stars more massive than about 1.9 times the mass of the Sun will have lifetimes that are too short to allow intelligent life to evolve. Answer c) Stars wi ...
Iron does not burn.
Iron does not burn.

Fixed Stars - Mark Dodich
Fixed Stars - Mark Dodich

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Ursa Minor



Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.
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