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 21213HIP 21219HIP 21241HIP 21258HIP 21265HIP 21266HIP 21274HIP 21282HIP 21290HIP 21291HIP 21292HIP 21295HIP 21311HIP 21315HIP 21325HIP 21330HIP 21342HIP 21346HIP 21350HIP 21356HIP 21370HIP 21375HIP 21376HIP 21377HIP 21382HIP 21390HIP 21374HIP 21419HIP 21434HIP 21446HIP 21452HIP 21465HIP 21467HIP 21469HIP 21484HIP 21486HIP 21535HIP 21544HIP 21555HIP 21634HIP 21641HIP 21644HIP 21645HIP 21650HIP 21653HIP 21664HIP 21667HIP 21690

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