Smallest Star in the Universe
Birth of tiny stars
Stars form from the gravitational collapse of gas in a nebula. The parts of the nebula that are slightly denser than the rest begin to collapse first, and then they attract more and more matter, forming ever denser clumps. From these clumps protostars form.
A protostar is hot because gravitational collapse releases heat. For as long as the protostar is gaining mass, the temperature increases. Finally, to become a real star the protostar needs enough mass to reach the temperature required to start nuclear fusion – that's several millions of degrees.
Physicists calculate that the minimum mass needed to create the conditions for hydrogen fusion is somewhere from 7 - 8% of the Sun's mass. They don't yet have an exact value for the mass limit because in practice, there are many factors involved in star formation that aren't well understood.
Brown dwarfs and red dwarfs
If a protostar doesn't make it to the mass limit, it's left as a brown dwarf, a failed star. The mass range of brown dwarfs starts at about thirteen times that of Jupiter, with the heaviest ones maybe reaching 75-80 times Jupiter's mass. Since red dwarfs are the smallest stars, the very smallest star would be a red dwarf just over the mass limit. It would have a mass similar to that of the largest brown dwarfs, presenting the oddity of a star the size of a gas giant planet with a mass about eighty times as great.
Gravity is the force that pulls matter together. Although stars come into being by gravitational collapse of nebulae, heavenly bodies can't exist unless they resist the inward pull of gravity. In stars the radiation pressure from nuclear reactions in the core is the outward force that balances gravity. But brown dwarfs are subject to different forces.
Since the core of a brown dwarf never gets enough mass to start hydrogen fusion, the only heat is produced by gravitational contraction. Yet as the brown dwarf cools, a weird force keeps it from collapsing, because the matter in the core is degenerate. This isn't a moral judgment. It refers to a particular quantum mechanical state that doesn't depend on temperature. Although the degeneracy pressure stops the brown dwarf from collapsing, it also stops it from acquiring more mass. This is why it can't become a real star.
A star's mass is directly related to its temperature, which is convenient for astronomers, because temperature is much easier to determine than mass. Higher-mass stars are bigger and hotter than lower-mass stars. This isn't the case for brown dwarfs. Because of the strange behavior of degenerate matter, higher-mass brown dwarfs are smaller than lower-mass brown dwarfs.
Finding the smallest star
Finding really big stars is difficult if they're a long way away, but finding small stars is tricky at any distance. All red dwarf stars are invisible to the unaided eye. Although about 75% of the stars around us are red dwarfs, none were seen until two centuries after the first use of astronomical telescopes.
Brown dwarfs are even harder to find. They're smaller and cooler than red dwarfs, and give out almost no visible light, radiating mainly in infra-red. The first confirmed discovery of a brown dwarf was in 1994.
Tiny stars and dark dwarfs are hard to see and sometimes difficult to distinguish from each other. Therefore if you want to try to find the smallest red dwarf and test the mass limit, you'd have your work cut out for you. As it happens, astronomers are very determined, and a group at Georgia State University in the USA, led by Sergio Dieterich, took up the challenge. They studied 63 objects that seemed to be near the borderline between stars and brown dwarfs.
In the graph of their results they plotted radius (size) against temperature (mass). As expected, the radius decreased with temperature – these were the red dwarfs. But it happened only down to about 2100 K (1830 °C /3300 °F). They were quite excited to see a break there, and then the radii increasing as temperature decreased – just what you'd expect of a set of brown dwarfs.
The smallest star so far
At the bottom of the stellar part of the graph, there was red dwarf 2MASS J05233822-1403022. You can barely see it in visible light, but it shows up well in infrared. The red dwarf lies forty light years away in the constellation Lepus (the Hare). Its name shows that it was discovered in the 2-Micron All Sky Survey, and the numbers give its sky coordinates. The teensy star, about the size of Saturn, has a mass less than 8% of the mass of the Sun. Its temperature of 1800 °C is less than a third of the Sun's 5600°C.
Nonetheless the models predict that the mass limit is around 1400° C. So 2MASS J0523-1403 probably isn't the smallest star around. It's the smallest star found out of a limited sample of stars. Sergio Dieterich is already at work with a team that's studying a larger sample, and extending the investigation to examine the effects of chemical composition on the mass limit.
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