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Life Cycles of Stars
Life Cycles of Stars

... This star core is typically composed of carbon and oxygen. Neon, magnesium, and helium are possible. ...
Review 2
Review 2

... Main features of Uranus and Neptune and of the Galilean moons of Jupiter. Structure of a comet. The asteroid belt and the Oort cloud. Why do we have meteor showers during specific days of a year? Chapter 16: How do we use the atomic emission and absorption spectra to find the composition of a star? ...
Lund Observatory Department of Astronomy and Theoretical Physics
Lund Observatory Department of Astronomy and Theoretical Physics

Life Cycle of Stars: Chapter 21
Life Cycle of Stars: Chapter 21

... Fusion • Star is born! ...
Pathways to Habitability: from disks to active stars, planets and life
Pathways to Habitability: from disks to active stars, planets and life

... During the initial disk phase, the first stages of planet formation take place ...
When Stars Blow Up
When Stars Blow Up

... •At the base of the accreted layer, electrons become degenerate •When the temperature reaches a few MK, fusion begins •Degenerate fusion is a runaway. •All the H fuses to He and heavier elements in a soundcrossing time (a few minutes) •The star increases in brightness ~ 10,000 times •Most of the mat ...
No Slide Title - steadyserverpages.com
No Slide Title - steadyserverpages.com

... Why does fusion stop at Iron? Elements lighter than iron undergo fission. There is an energy density limit of the fundamental forces Elements heavier than iron do undergo fusion. ...
Physical Science 1 Quiz 10 1 ID # or name:
Physical Science 1 Quiz 10 1 ID # or name:

... Please  circle  the  letter  or  write  the  letter  next  to  or  under  the  question  number.    This  quiz  is   due  by  7:30  pm,  Wed.,  May  28th.    Please  submit  your  quiz  to  me  via  email  to  one  of  the ...
1. Compute the deflection angle of a star whose light... limb of the Sun. Also compute the deflection angle of...
1. Compute the deflection angle of a star whose light... limb of the Sun. Also compute the deflection angle of...

... 1. Compute the deflection angle of a star whose light just grazes the limb of the Sun. Also compute the deflection angle of a star whose light just grazes the limb of a 1.4M neutron star, if the neutron star was at the same distance from the Earth as the Sun. State assumptions. 2. Use the Plummer p ...
the free PDF resource
the free PDF resource

... usually yellow, white or blue depending on temperature (hotter = more blue) mass varies hugely usually orbited by planets sometimes exists in a pair (called binary system) almost entirely hydrogen. ...
22.2 Stars Change Over Their Life Cycles
22.2 Stars Change Over Their Life Cycles

... determined my its temperature ...
tire
tire

... 5. Large black holes found at the center of most galaxies. 6. The oscillations of space caused the rapid movement of matter, such as a supernova or orbiting black holes. 7. An object whose gravity is so strong that the escape speed exceeds the speed of light. 8. A type of yellow supergiant pulsating ...
Chapter 4 Vocabulary
Chapter 4 Vocabulary

... during which stars produce energy by fusing hydrogen and helium ...
投影片 1
投影片 1

... GD 362 White Dwarf star  R.A. 17h 31m 34.33s  Dec. +37° 05' 20.6"  Distance: 22~26 pc ...
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Cygnus X-1



Cygnus X-1 (abbreviated Cyg X-1) is a well-known galactic X-ray source, thought to be a black hole, in the constellation Cygnus. It was discovered in 1964 during a rocket flight and is one of the strongest X-ray sources seen from Earth, producing a peak X-ray flux density of 6977229999999999999♠2.3×10−23 Wm−2 Hz−1 (7003230000000000000♠2.3×103 Jansky). Cygnus X-1 was the first X-ray source widely accepted to be a black hole and it remains among the most studied astronomical objects in its class. The compact object is now estimated to have a mass about 14.8 times the mass of the Sun and has been shown to be too small to be any known kind of normal star, or other likely object besides a black hole. If so, the radius of its event horizon is about 7004440000000000000♠44 km.Cygnus X-1 belongs to a high-mass X-ray binary system about 7019574266339685654♠6070 ly from the Sun that includes a blue supergiant variable star designated HDE 226868 which it orbits at about 0.2 AU, or 20% of the distance from the Earth to the Sun. A stellar wind from the star provides material for an accretion disk around the X-ray source. Matter in the inner disk is heated to millions of degrees, generating the observed X-rays. A pair of jets, arranged perpendicular to the disk, are carrying part of the energy of the infalling material away into interstellar space.This system may belong to a stellar association called Cygnus OB3, which would mean that Cygnus X-1 is about five million years old and formed from a progenitor star that had more than 7001400000000000000♠40 solar masses. The majority of the star's mass was shed, most likely as a stellar wind. If this star had then exploded as a supernova, the resulting force would most likely have ejected the remnant from the system. Hence the star may have instead collapsed directly into a black hole.Cygnus X-1 was the subject of a friendly scientific wager between physicists Stephen Hawking and Kip Thorne in 1975, with Hawking betting that it was not a black hole. He conceded the bet in 1990 after observational data had strengthened the case that there was indeed a black hole in the system. This hypothesis has not been confirmed due to a lack of direct observation but has generally been accepted from indirect evidence.
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