Class A — A-type (White)

A-type stars are white or blue-white stars with surface temperatures of 7,500 to 10,000 K. They comprise about 0.6% of main-sequence stars and are known for having the strongest hydrogen absorption lines in their spectra. Many of the best-known stars are A-type, including Sirius (A1V), the brightest star in the night sky, and Vega (A0V), which was historically the reference star for the magnitude system. A-type stars live for roughly 1-2 billion years.

A-type stars are white to blue-white stars with surface temperatures between 7,500 and 10,000 K. They represent about 0.6% of main-sequence stars and include many of the most culturally important stars in the sky. A-type stars are particularly significant in astronomical history: Vega, the prototypical A0V star, served as the original definition of apparent magnitude 0.0 and was the first star (other than the Sun) to be photographed (1850) and to have its spectrum recorded (1872).

Characteristics

A-type spectra are dominated by the hydrogen Balmer series, which reaches maximum strength at A0. These stars are massive enough (1.4-2.1 solar masses) to have radiative envelopes rather than convective ones, which allows chemical peculiarities to develop. The Am (metallic-line) and Ap (peculiar) stars show unusual abundances of certain elements concentrated by diffusion in their stable atmospheres. A-type main-sequence stars live for roughly 1-3 billion years. The debris disks detected around many A stars (notably Vega and Fomalhaut) hint at planetary systems in formation.

Notable Examples

Sirius (Alpha Canis Majoris, A1V) is the brightest star in the night sky at magnitude -1.46, largely due to its proximity at 8.6 light-years. Its white dwarf companion Sirius B was the first white dwarf discovered. Vega (Alpha Lyrae, A0V) and Altair (Alpha Aquilae, A7V) join Deneb to form the Summer Triangle. Fomalhaut (Alpha Piscis Austrini, A3V) hosts a dramatic debris ring and was the first star with a directly imaged exoplanet candidate. Castor (Alpha Geminorum) is a spectacular sextuple star system dominated by A-type components.

HIP 73450HIP 73451HIP 85031HIP 75729HIP 75736HIP 75737HIP 85034HIP 85038HIP 85044HIP 33430HIP 33436HIP 33438HIP 30240HIP 3025HIP 30251HIP 30252HIP 30255HIP 30257HIP 73483HIP 73507HIP 73516HIP 73520HIP 75759HIP 75764HIP 7577HIP 75770HIP 75772HIP 73535HIP 73552HIP 73559HIP 62214HIP 75788HIP 75789HIP 75795HIP 73571HIP 73584HIP 73587HIP 75825HIP 75830HIP 75842HIP 75848HIP 73601HIP 73608HIP 73612HIP 73613HIP 73616HIP 75875HIP 75876

Frequently Asked Questions

What is a class A star?
Class A (A-type (White)) stars are white stars. A-type stars are white or blue-white stars with surface temperatures of 7,500 to 10,000 K. They comprise about 0.6% of main-sequence stars and are known for having the strongest hydrogen absorption li
How hot are class A stars?
Class A stars have surface temperatures between 7,500 K and 10,000 K.
What color are class A stars?
Class A stars appear white.
How many class A stars are in the StarFYI database?
StarFYI currently catalogs 18,693 class A stars.
How luminous are class A stars?
Luminous, 5-25 solar luminosities