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Alpha Arietis
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Alpha Arietis

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Also known as Hamal, α Arietis, α Ari, 13 Ari, 13 Arietis, LTT 10711, GJ 84.3, GJ 9072

Hamal, , is a star in the northern zodiacal constellation of Aries. It has the Bayer designation Alpha Arietis, which is Latinized from α Arietis and abbreviated Alpha Ari or α Ari. This star is visible to the naked eye with an apparent visual magnitude of 2.0. Hamal is the brightest star in the constellation and, on average, the 50th-brightest star in the night sky. Based upon parallax measurements made with the Hipparcos astrometry satellite, Hamal is about from Earth. It is drifting closer to the Sun with a radial velocity of −14 km/s.

Wikidata facts

Instance of
orange giant
Constellation
Aries
Distance from Earth
20.2
Radius
13.9
Mass
1.5
Show 14 more facts
catalog code
[B10] 447
spectral class
K2 IIIab
metallicity
-0.19
radial velocity
-14.412
apparent magnitude
-0.63
stellar rotational velocity
0.50
effective temperature
4537
surface gravity
700
right ascension
31.793357100
declination
23.462417550
parallax
49.48
epoch
J2000.0
right ascension component of proper motion
192
declination component of proper motion
-146
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Encyclopedic overview

8 sections
Contents
  • Nomenclature
  • Properties
  • Planetary system
  • In culture
  • See also
  • Notes
  • References
  • External links

Hamal, , is a star in the northern zodiacal constellation of Aries. It has the Bayer designation Alpha Arietis, which is Latinized from α Arietis and abbreviated Alpha Ari or α Ari. This star is visible to the naked eye with an apparent visual magnitude of 2.0. Hamal is the brightest star in the constellation and, on average, the 50th-brightest star in the night sky. Based upon parallax measurements made with the Hipparcos astrometry satellite, Hamal is about from Earth. It is drifting closer to the Sun with a radial velocity of −14 km/s.

This is an aging giant star that is likely to host an orbiting planet with a mass greater than Jupiter.

Excerpted from Wikipedia’s “Alpha Arietis” article, available under the CC BY-SA 4.0 licence.

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