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 78452HIP 73820HIP 56746HIP 37306HIP 28660HIP 53379HIP 74387HIP 53395HIP 55395HIP 34654HIP 34657HIP 34659HIP 34660HIP 35578HIP 35584HIP 36052HIP 37431HIP 37440HIP 37898HIP 37904HIP 38361HIP 38867HIP 39291HIP 39518HIP 40220HIP 40209HIP 40210HIP 40211HIP 40212HIP 40216HIP 40667HIP 40669HIP 40673HIP 41133HIP 51250HIP 48539HIP 48541HIP 49458HIP 49689HIP 50381HIP 50840HIP 51302HIP 51518HIP 51774HIP 52707HIP 54561HIP 55477HIP 55485

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