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 9955HIP 99561HIP 99564HIP 99569HIP 90298HIP 90302HIP 90304HIP 90315HIP 90318HIP 97733HIP 97734HIP 92253HIP 97736HIP 97741HIP 90328HIP 99604HIP 33669HIP 33677HIP 33679HIP 97745HIP 97760HIP 92385HIP 92461HIP 92463HIP 90367HIP 90392HIP 90429HIP 90517HIP 90520HIP 90526HIP 90528HIP 72895HIP 97762HIP 92485HIP 92486HIP 92493HIP 92494HIP 92496HIP 92514HIP 36807HIP 36810HIP 36811HIP 36815HIP 90531HIP 90534HIP 90537HIP 9054HIP 90541

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