astronomical object consisting of a luminous spheroid of plasma held together by its own gravity
(Redirected from Celestial)

A star is a very large ball of bright, glowing, hot matter in space. That matter is called plasma. Stars are held together by gravity. They emit light because they are very hot. The Sun is an example of a star. It is at the center of the solar system.

Reconstructed view of the surface of the star Antares in the constellation of Scorpius
A star-forming region in the Large Magellanic Cloud. NASA/ESA image
The open star cluster Pismis 24 is in the nebula NGC 6357. It has some of the largest stars known. Pismis 24-1 has nearly 300 times the mass of the Sun. It is a multiple system of at least three stars.
The strange shapes taken by the clouds are a result of the vast radiation emitted by these huge, hot stars.
This image combines image data with three different filters in visible light from the 1.5-metre Danish telescope at the ESO La Silla Observatory in Chile.
The Crab Nebula, remains of a supernova that was first seen around 1050 AD

The amount of material in a star (its mass) is so huge that a nuclear reaction called nuclear fusion goes on inside it. This reaction changes hydrogen to helium and gives off heat. The light and heat created by nuclear fusion makes stars very hot. It also makes bigger chemical elements. In the Sun (but not all stars) the change which takes place is the production of helium, with small amounts of heavier elements.

Stars have a lot of hydrogen. Fusion makes a lot of energy. The energy produced by stars moves (radiates) away from them. Much of the energy leaves as light, and the rest leaves as other kinds of electromagnetic radiation.

When a star like the Sun gets old, it will expand in size and become a red giant star. That will happen in about 5 billion years.

Earth's Sun


The star nearest to Earth is the Sun. The energy from the Sun supports almost all life on Earth by providing light for plants. Plants turn the light into energy in a process called photosynthesis.[1] The energy from the Sun also causes weather and humidity on Earth.

We can see other stars in the night sky when the Sun goes down. Like the Sun, they are made mostly of hydrogen and a little bit of helium plus other elements. Astronomers compare those other stars to the Sun. Their mass is measured in solar masses (). A solar mass is the mass of the Sun. A small star may be about 0.2 Mʘ, a medium one may be about the Sun's mass (1 Mʘ), and a large star may be about 10 Mʘ.



The Earth and other planets move around (orbit) the Sun. The Sun and all things that orbit it are called the Solar System. Many other stars have planets orbiting them, and those planets are called exoplanets. Our Sun would look like a star in the sky to someone on an exoplanet, but you would not see the Earth from one because it would be too far away.

Numbers, distances


Proxima Centauri is the closest star to the Sun. It is 39.9 trillion kilometres, equal to 4.2 light years, away. This means that light from Proxima Centauri takes 4.2 years to reach Earth.

Astronomers think there is a very large number of stars in the Universe. The observable Universe contains more than 2 trillion (1012) galaxies[2] and, overall, as many as an estimated 1×1024 stars[3][4] (more stars than all the grains of sand on planet Earth).[5] That is, 1,000,000,000,000,000,000,000,000 stars, which is many times more than the few hundred billion stars in our galaxy, the Milky Way.

Most stars are very old. They are usually thought to be between 1 billion and 10 billion years old. The oldest stars are 13.7 billion years old. That is as old as the Universe. Some young stars are only a few million years old.

Stars are different sizes. The smallest stars are neutron stars, which are actually dead stars. They are no bigger than a human city. A neutron star has a large amount of mass in a very small space. A neutron star has a mass of at least 1.4 Mʘ.

Hypergiant stars are the largest stars in the Universe. They have a diameter up to 1,600 times bigger than the Sun's. If the Sun was a hypergiant star, it would reach out to as far as Jupiter.

The star Betelgeuse is a red supergiant star about 640[6] times the Sun's diameter. Although these stars are very large, they also have low density.

Stars have many sizes. The star that the planet PSR B1257+12 B orbits is only 20 kilometers large, but VY Canis Majoris is 2 billion km large.

Some stars look brighter than other stars. This difference is measured in terms of apparent magnitude. There are two reasons why stars have different apparent magnitude. If a star is very close to us, it will appear much brighter. This is just like a candle. A candle that is close to us appears brighter. The other reason a star can appear brighter is that it is hotter than another cooler star.

Stars give off light but also give off a solar wind and neutrinos. These are very small particles of matter.

Stars are made of mass and mass makes gravity. Gravity makes planets orbit stars. This is why the Earth orbits the Sun. The gravity of two stars can make them go around each other. Stars that orbit each other are called binary stars. Scientists think there are many binary stars. There are even groups of three or more stars that orbit each other. Proxima Centauri is a small star that orbits other stars.

Stars are not spread evenly across all of space. Instead, they are grouped into galaxies. A galaxy contains hundreds of billions of stars.

History of seeing stars

People have seen patterns in the stars since long ago.[7] This, from 1690, is the constellation of Leo the lion, as imagined by Johannes Hevelius.[8]

Stars have been important to people all over the world for all of history. Stars have also been part of religious practices. Long ago, people believed that stars could never die.

Astronomers organized stars into groups called constellations. They used the constellations to help them see the motion of the planets and to guess the position of the Sun.[7] The motion of the Sun and other stars was used to make calendars. The calendars were used by farmers to decide when to plant crops and when to harvest them.[9]

The life of stars


Stars are made in nebulae. These are areas that have more gas than normal space. The gas in a nebula is pulled together by gravity. The Orion nebula is an example of a place where gas is coming together to form stars.

Stars spend most of their lives combining (fusing) hydrogen with hydrogen to make energy. When hydrogen is fused it makes helium and it makes a lot of energy. To fuse hydrogen into helium it must be very hot and the pressure must be very high. Fusion happens at the center of stars, called "the core".

The smallest stars are called red dwarfs. Red dwarfs fuse their hydrogen slowly and live for more than 100 billion years, so they live longer than any other star. At the end of their lives, they become dimmer and dimmer. Red dwarfs do not explode.

When very heavy stars die, they explode. This explosion is called a supernova. When a supernova happens in a nebula, the explosion pushes the gas in the nebula together. This makes the gas in the nebula very dense (thick). Gravity and exploding stars both help to bring the gas together to make new stars in nebulas.

Most stars use up the hydrogen at their core. When they do, their core becomes smaller and hotter. It becomes so hot that it pushes away the outer part of the star. The outer part expands and it makes a red giant star. Astrophysicists think that in about 5 billion years, the Sun will be a red giant. Our Sun will be so large it will "eat" the Earth. After our Sun stops using hydrogen to make energy, it will use helium in its very hot core. It will be hotter than when it was fusing hydrogen. Heavy stars will also make elements heavier than helium. As a star makes heavier and heavier elements, it makes less and less energy. Iron is a heavy element made in heavy stars.

Our star is an average star. Average stars will push away their outer gases. The gas it pushes away makes a cloud called a planetary nebula. The core part of the star will remain. It will be a ball as big as the Earth and called a white dwarf. It will fade into a black dwarf over a very long time.

Later in large stars (~ 10 Mʘ), heavier elements are made by fusion. Finally the star makes a supernova explosion. Most things happen in the universe so slowly we do not notice. But supernova explosions happen in only 100 seconds. When a supernova explodes its flash is as bright as a 100 billion stars. The dying star is so bright it can be seen during the day. Supernova means "new star" because people used to think it was the beginning of a new star. Today we know that a supernova is the death of an old star. The gas of the star is pushed away by the explosion. It forms a giant cloud of gas called a planetary nebula. The crab nebula is a good example. All that remains is a neutron star. If the star was very heavy (~ 25 Mʘ), the star will make a black hole. Gravity in a black hole is extremely strong. It is so strong that even light cannot escape from a black hole.

The heaviest elements are made in the explosion of a supernova. After billions of years of floating in space, the gas and dust come together to make new stars and new planets. Much of the gas and dust in space comes from supernovae. Our Sun, the Earth, and all living things are made from star dust.



Astronomers have known for centuries that stars have different colors. When looking at an electromagnetic spectrum, ultraviolet waves are the shortest, and infrared are the longest.[10] The visible spectrum has wavelengths between these two extremes.

Modern instruments can measure very precisely the color of a star. This allows astronomers to determine that star's temperature, because a hotter star's black-body radiation has shorter wavelengths. The hottest stars are blue and azure, then white, then yellow, and the coolest are red.[11] Below is a list of the coolest stars.

List of coolest stars
Name Temperature (K) Radius (Solar radii)
V688 Monocerotis 1670 1347
CWISE J124909.08+362116.0 1715 0.08
S Cassiopeiae 1800 930
RW Leonis Minoris 1800 1028.27
LL Pegasi 1800 1074
V384 Persei 1820 937
2MASS J07464256+2000321 A 1822 0.089
T Draconis 1850 1200
HIP 113330 1859 649.091
V346 Puppis 1875 1025
HD 110813 1916 843.811
2MASS J0523-1403 1939 0.086
S Aurigae 1940 957
V1426 Cygni 1975 216.1

Knowing the color and absolute magnitude, astronomers can place the star on the Hertzsprung-Russell diagram, and estimate its habitable zone and other facts about it.

For example, our Sun is yellow-white, and the Earth is the perfect distance away for life. If our Sun was a hotter, blue star, however, Earth would have to be much farther away or else it would be too hot to have water and sustain life.


  1. Simon A. 2001 (9 October 2001). The real science behind the X-Files: microbes, meteorites, and mutants. Simon & Schuster. pp. 25–27. ISBN 0684856182.{{cite book}}: CS1 maint: numeric names: authors list (link)
  2. Fountain, Henry (17 October 2016). "Two Trillion Galaxies, at the Very Least". The New York Times. Retrieved 17 October 2016.
  3. Staff (2019). "How Many Stars Are There In The Universe?". European Space Agency. Retrieved 21 September 2019.
  4. Marov, Mikhail Ya. (2015). "The Structure of the Universe". The Fundamentals of Modern Astrophysics. pp. 279–294. doi:10.1007/978-1-4614-8730-2_10. ISBN 978-1-4614-8729-6.
  5. Mackie, Glen (1 February 2002). "To see the Universe in a Grain of Taranaki Sand". Centre for Astrophysics and Supercomputing. Retrieved 28 January 2017.
  6. Mittag, M.; Schröder, K.-P.; Perdelwitz, V.; Jack, D.; Schmitt, J. H. M. M. (2023-01-01). "Chromospheric activity and photospheric variation of α Ori during the great dimming event in 2020". Astronomy & Astrophysics. 669: A9. doi:10.1051/0004-6361/202244924. ISSN 0004-6361.
  7. 7.0 7.1 Forbes, George (1909). History of Astronomy (Free e-book from Project Gutenberg). London: Watts & Co. ISBN 1153627744.
  8. Hevelius, Johannis (1690). Firmamentum Sobiescianum, sive Uranographia. Gdansk.
  9. Tøndering, Claus. "Other ancient calendars". WebExhibits. Archived from the original on 2019-11-21. Retrieved 2006-12-10.
  10. "The Electromagnetic Spectrum". Andy Darvill's Science Site. Retrieved 2016-06-06.
  11. "Star Colors Explained". One Minute Astronomer. December 23, 2008. Archived from the original on 2016-03-27. Retrieved 2016-06-06.

Other websites