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 1024HIP 1039HIP 1043HIP 1075HIP 1088HIP 1089HIP 1132HIP 1167HIP 1278HIP 1284HIP 1286HIP 1272HIP 1302HIP 1318HIP 1320HIP 1348HIP 1340HIP 1343HIP 1488HIP 1493HIP 1496HIP 1524HIP 1538HIP 1548HIP 1554HIP 1561HIP 1584HIP 1603HIP 1635HIP 1641HIP 1670HIP 1676HIP 1677HIP 1840HIP 1826HIP 1859HIP 1896HIP 1900HIP 1903HIP 1913HIP 2054HIP 2071HIP 2089HIP 2093HIP 2075HIP 2125HIP 2130HIP 2133

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