Which spectral type has the longest lifespan?

The stars with the longest lifetimes are red dwarfs; some may be nearly as old as the universe itself.

Which main sequence spectral type lives the longest on the main sequence?

Most stars fall on the Main Sequence. On the Main Sequence, the more massive stars are bigger, hotter, more luminous, and die faster. The life span of stars ranges from about 10 million years for the blue giants to about 100 billion years for the red dwarfs.

How long do O type stars live?

The least luminous O-type stars can remain on the main sequence for around 10 million years, but cool slowly during that time and become early B-type stars. No massive star remains with spectral class O for more than about 5–6 million years.

How long do B type stars live?

They have absolute luminosities as bright as any star in the Galaxy—on the order of one million times the luminosity of the Sun. Such stars have very short lifetimes, only lasting a few million years.

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Do big stars live longer?

1) The bigger a star is, the longer it will live. 2) The smaller a star is, the longer it will live. … A smaller star has less fuel, but its rate of fusion is not as fast. Therefore, smaller stars live longer than larger stars because their rate of fuel consumption is not as rapid.

What is the most common spectral class?

A red dwarf is a small, cool, very faint, main sequence star whose surface temperature is under about 4,000 K. Red dwarfs are the most common type of star.

Spectral Classes.

Star Type O
Color Blue
Approximate Surface Temperature over 25,000 K
Average Mass (The Sun = 1) 60
Examples 10 Lacertra

What is the lifetime of a star?

The lifetimes of main sequence stars therefore range from a million years for a 40 solar mass O-type star, to 560 billion years for a 0.2 solar mass M-type star.

What type of visible star is the coolest?

  • A red dwarf is the smallest and coolest kind of star on the main sequence. …
  • The coolest red dwarfs near the Sun have a surface temperature of ~2,000 K and the smallest have radii of ~9% that of the Sun, with masses about ~7.5% that of the Sun.

Why are 90 of stars on the main sequence?

Main sequence stars fuse hydrogen atoms to form helium atoms in their cores. About 90 percent of the stars in the universe, including the sun, are main sequence stars. … Stars start their lives as clouds of dust and gas. Gravity draws these clouds together.

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Do stars actually twinkle?

As light from a star races through our atmosphere, it bounces and bumps through the different layers, bending the light before you see it. Since the hot and cold layers of air keep moving, the bending of the light changes too, which causes the star’s appearance to wobble or twinkle.

Do stars die?

Stars die because they exhaust their nuclear fuel. … Once there is no fuel left, the star collapses and the outer layers explode as a ‘supernova’. What’s left over after a supernova explosion is a ‘neutron star’ – the collapsed core of the star – or, if there’s sufficient mass, a black hole.

What stars live the shortest?

So the total lifespan of a star with the mass of the Sun is about 10 billion years. The smallest stars are the red dwarfs, these start at 50% the mass of the Sun, and can be as small as 7.5% the mass of the Sun.

What is the oldest star?

There is no question that the Methuselah star is old – indeed it is the oldest star in the universe for which there is a fairly precise estimate of its age.

What is the longest a star can live?

The stars with the longest lifetimes are red dwarfs; some may be nearly as old as the universe itself.

  • Red Dwarf Stars. Astronomers define a red dwarf as a star having between about 0.08 and 0.5 times the mass of the sun and formed primarily of hydrogen gas. …
  • Luminosity and Lifetime. …
  • Nuclear Fusion. …
  • Life Cycle of Stars.
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Will our Sun become a black hole?

No. Stars like the Sun just aren’t massive enough to become black holes. Instead, in several billion years, the Sun will cast off its outer layers, and its core will form a white dwarf – a dense ball of carbon and oxygen that no longer produces nuclear energy, but that shines because it is very hot.

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