Stars Constellations Articles Sitemap ← Back
Stars in Cassiopeia

Eta Cassiopeia, a white main-sequence star in Cassiopeia

Eta Cassiopeia is a white main-sequence star in the constellation Cassiopeia. At 19.4 light years away, it is the 272nd brightest star in the Earth's sky, where it shines at an apparent visual magnitude of 3.46.

Ashland Astronomy Studio Star

Eta Cassiopeia (HIP 3821)

Eta Cassiopeia is a white main-sequence star in the constellation Cassiopeia. At 19.4 light years away, it is the 272nd brightest star in the Earth's sky, where it shines at an apparent visual magnitude of 3.46. Eta Cassiopeia is the primary component of a multiple-star system. The star's age is estimated to be 5.1 billion years but is certainly no less than 2 billion years and no greater than 8.4 billion years. The iron abundance of Eta Cassiopeia is -0.28 (52.5% of the Sun). It is moving through the Galaxy at a speed of 35.5 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,100 and 27,400 light years from the center of the Galaxy.

Sky position: RA 0h 49.1m, Dec +57° 49.2'

Common designations: Eta Cassiopeiae, Achird, 24 Cassiopeiae, HIP 3821, HD 4614, Gliese 34 A, Wolf 24

Learn how to find naked-eye stars with:

Stars of the Northern Hemisphere
Deluxe Astronomy Poster Brightest stars in Cassiopeia:
(list all)

RankMag.Star
12.15Gamma Cassiopeiae
22.24Schedar
32.28Caph
42.66Ruchbah
53.35Segin

6

| 3.46

) Eta Cassiopeia

RankMag.Star
73.69Zeta Cassiopeiae
83.9550 Cassiopeiae
94.17Kappa Cassiopeiae
104.34Marfak
114.46Iota Cassiopeiae
124.48Omicron Cassiopeiae
134.49A Cassiopeiae
144.51Rho Cassiopeiae
154.62Upsilon-2 Cassiopeiae
164.68Chi Cassiopeiae
174.72Psi Cassiopeiae
Location of Eta Cassiopeia circled Map detail from Stars of the Northern Hemisphere
Hover over other bright stars to identify or click to jump.

Galactic Orbit of Eta Cassiopeia

(compared to the Sun)

E

ccentricity: 8.6% vs. 16.0%

Angle φ : -62.8°vs. 26.0°

Semi-major axis : 7,751 pc vs. 8,686 pc

Semi-minor axis: 7,722 pc vs. 8,574 pc

Focus-to-center

: 665 pcvs. 1,388 pc

Semilatus rectum : 7,694 pc vs. 8,464 pc

Perigalacticon: 7,086 pc vs. 7,297 pc

Apogalacticon

: 8,416 pcvs. 10,074 pc
  Some Tabulated XHIP Data for Eta Cassiopeia
(see also: SIMBAD)

Astrometry
2007A&A...474..653V

Position Proper Motion
Right Ascension: 12.27125307° ±0.30 mas 1,086.59 ±0.40 mas/yr.
Declination: 57.81654753° ±0.27 mas -559.43 ±0.33 mas/yr.
Galactic Longitude: 122.61739279° 1,081.41 mas/yr.
Galactic Latitude: -5.05376554° -569.37 mas/yr.

Parallax: 167.98 ± 0.48 mas

Spectrography

Spectral Type: F9V 2008ApJS..176..216A.

Radial Velocity: 8.33 ±0.10 km/s [A rating] 2002ApJS..141..503N, 2005ApJS..159..141V.
This star is a spectroscopic binary with a solved orbit.

Iron Abundance [Fe/H]: -0.28 dex  2011A&A...525A..71W, 2009A&A...501..941H, 2007A&A...465..271R, 2006ApJ...652.1604B, 2006AJ....131.3069L, 2005PASJ...57...27T, 2005ApJS..161..444T, 2005ApJS..159..141V, 2005AJ....129.1063L, 2004A&A...420..183A, 2004A&A...418..551M, 2003AJ....126.2015H, 2000Priv.C........F, 1996A&A...314..191G, 1993A&A...275..101E.
 


Photometry
 
band magnitude Abs. Mag.
U
B 4.05 5.17
V 3.46 4.59
R 3.10 4.23
I 2.80 3.93
J 2.11 3.24
H 2.09 3.21
K 1.99 3.11

B-V: +0.59 V-I: +0.66

Derivations

Heliocentric distance: 5.95 pc (0.3% margin of error)

Galactocentric distance: 7,403 pc

Transverse velocity: 34.5 km/s

3D heliocentric position and motion:

toward:   

Galactic center Galactic rotation North Galactic Pole
Position ( X, Y, Z) -3.2 pc 5.0 pc -0.5 pc
Velocity (U, V, W) -29.4 km/s -10.7 km/s -16.7 km/s

← Back to all stars
// Fade in · only sidebar boxes, never the main content if('IntersectionObserver' in window){var io=new IntersectionObserver(function(es){es.forEach(function(en){if(en.isIntersecting){en.target.style.opacity='1';en.target.style.transform='none';io.unobserve(en.target);}});},{threshold:.05});document.querySelectorAll('.side__box').forEach(function(el){el.style.opacity='0';el.style.transform='translateY(10px)';el.style.transition='opacity .4s ease,transform .4s ease';io.observe(el);});}