Star
Template:TOC-right A star is usually made of gas and a substance known as plasma. The Sun (Sol) is a star. A portion of the stars, however, those called white dwarfs and neutron stars, are composed of tightly packed atoms or subatomic particles and are much more dense than anything on Earth.
Stars range widely in size. Our Sun’s radius is about 432,000 miles (695,500 kilometres). Because there are other stars that are much larger, our sun is classified as a dwarf star. Stars classified as supergiants have a radius about 1,000 times that of the sun. Neutron stars are the smallest stars and have a radius of only about 6 miles (10 kilometres).
Our sun is a single star. However, about 75 % of all stars are binary stars, two stars that orbit each other. The star nearest our sun, Proxima Centauri, is part of a multiple-star system which includes Alpha Centauri A and Alpha Centauri B.[1]
Categories
Characteristics of stars
Stars are categorised by their five main attributes;
- (1) brightness, (magnitude or luminosity);
- (2) colour;
- (3) surface temperature;
- (4) size (diameter);
- (5) mass (amount of matter).
Colour is dependent of surface temperature, brightness depends on surface temperature and the size. Mass affects how fast a stars produces energy and effects surface temperature.
Astronomers use a diagramme to show how these are all related, the Hertzsprung-Russell (H-R) diagramme
Magnitude
Based on a numbering system used by Hipparchus (125 B.C. Greece) stars are numbered according to their brightness as they are seen from Earth. The brightest is of the first magnitude, the next brightest of the second magnitude and so on to the sixth magnitude, which are very faint stars. Today this is called apparent magnitude. There is now a measure of absolute magnitude, what the apparent magnitude would be if the star was 32.6 light-years from Earth
There are also stars that are brighter than the first magnitude and they are classed by numbers less than 1. Rigel’s apparent magnitude is 0.12. Extremely bright stars have numbers that are less than zero or negative numbers. The brightest stars in the night sky is Sirius with a apparent magnitude of -1.46 and the absolute magnitude of Rigel is -8.1. At the present time there are no stars classified with a absolute magnitude brighter than -8.0 Some very dim stars have an apparent magnitude of 28, but absolute magnitude can be no fainter than about 16.[2]
Luminosity
How bright a star looks is controlled by its actual brilliance and its distance from Earth. A star’s brilliance is the amount of visible light it produces. So a nearby star can be quite dim if it is not generating a great deal of light while a star much further away can be brighter because it actually is much brighter. The star Alpha Centauri appears brighter than another star called Rigel. It would seem that Alpha Centauri produces more energy. However, Rigel is actually much brighter but it is much further away fro Earth. Alpha Centauri is about 4.4 light years away while Rigel is 1,400 light years from Earth.
Stars radiate visible light but they also radiate energy the human eye can not see. A stars luminosity is the measure of energy it radiates[3] Our sun has a luminosity of 400 trillion trillion watts (1024). Commonly in astronomy however, the luminosity is measured another way, by comparing it with our Sun. In this way Alpha Centauri is about 1.3 times as luminous as our Sun and Rigel is 150,000 times as luminous.
There is a luminosity absolute magnitude comparison: 5 on the absolute magnitude scale equals 100 on the luminosity scale. So, if a star has absolute magnitude of 2, it is 100 times as luminous as a star with an absolute magnitude of 7. A star with an absolute magnitude of -3 is 100 times as luminous as a star with an absolute magnitude is 2 and 10,000 times more luminous than a star with an absolute magnitude of 7.
Colour
Surface temperature
Size
Mass
Fusion
Life Cycle
Stars have a beginning and an end. Our sun became a star about 4.6 billion years ago and may last another 5 billion years. After that it will become a red giant, later it will lose its outer layers and the remaining core of the star will become a white dwarf, eventually fading to a black dwarf, dense and without light.
Not all stars end this way. Some will cool off and without expanding to a red giant stage will become white dwarfs, then black dwarfs..
Another possibility for a small percentage of stars is a spectacular explosion called a supernovae. The star explodes and loses most of its material. An even smaller percentage, undergo a very rare occurrence, they completely explode and nothing is left.
Intermediate-mass stars
T-Tauri phase
Main-sequence stars
Red giant phase
Horizontal branch phase
Asymptotic giant phase
White dwarf phase
Black dwarf phase
Supernovae
Neutron stars
Black holes
Galaxies
Stars are grouped in galaxies with rare exceptions.[5] Astronomical observations to date have recorded galaxies at distances of 12 to 16 billion light years from our sun. Our sun is in the galaxy called the Milky Way which contains an estimated 100 billion stars. It is estimated that there are more than 100 billion galaxies in the universe and average about 100 billion stars per galaxy. This means that there is an estimated 10 billion, trillion stars in the universe (1021). From Earth however, without using binoculars or a telescope, it is only possible to see about 3,000 of them.
Notes
- ↑ The distance to Proxima Centauri is over 25 trillion miles (40 trillion kilometres) and light from Proxima Centauri must travel 4.2 years to travel to us before we can see it. One light-year, the distance that light travels in a vacuum in a year, equals about 5.88 trillion miles (9.46 trillion kilometres).
- ↑ Paul J. Green, (2005) "Star." World Book Online Reference Center.. World Book, Inc. [1] Reprinted by NASA at [2] Paul J. Green, PhD. is an Astrophysicist with Smithsonian Astrophysical Observatory.
- ↑ [3] Northern Arizona University, College of Engineering and Natural Sciences. Luminosity is defined as the total energy radiated by a star each second, at all wavelengths (measured as ergs per second). Star luminosity is commonly compared to our Sun (Lsun = 4 x 1033 ergs/s). Luminosity is measured in the same way as power which is energy per second.
- ↑ Paul J. Green, (Astrophysicist, Smithsonian Astrophysical Observatory) (2005) "Star." World Book Online Reference Center.. World Book, Inc. [4] Reprinted by NASA at [5] Paul J. Green, PhD. is an Astrophysicist with Smithsonian Astrophysical Observatory.
- ↑ 'Shot in the Dark' Star Explosion Stuns Astronomers NASA