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Star in the constellation Pisces
94 Piscium is a single
[9]
star in the
zodiac
constellation
Pisces ,
[8] located 305
light years away from the Sun.
[1] It is visible to the naked eye as a faint, orange-hued star with an
apparent visual magnitude of 5.495.
[2] The object is moving closer to the Earth with a heliocentric
radial velocity of −43 km/s.
[5] It is a possible member of the
Wolf 630 moving group .
[10]
This is an
evolved
K-type
giant star with a
stellar classification of K1 III.
[3] It is a
red clump giant, which indicates it is on the
horizontal branch and is generating energy through
helium fusion at its
core .
[11] The star is 4.1 billion years old with 1.34
[6] times the
mass of the Sun and 13 times the
Sun's radius . It is radiating 69
[1] times the
Sun's luminosity from its enlarged
photosphere at an
effective temperature of 4,665 K.
[7]
References
^
a
b
c
d
e
f
g
h
i
Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018).
"Gaia Data Release 2: Summary of the contents and survey properties" .
Astronomy & Astrophysics . 616 . A1.
arXiv :
1804.09365 .
Bibcode :
2018A&A...616A...1G .
doi :
10.1051/0004-6361/201833051 .
Gaia DR2 record for this source at
VizieR .
^
a
b Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics . 355 : L27–L30.
Bibcode :
2000A&A...355L..27H .
^
a
b McWilliam, Andrew (1990).
"High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances" . The Astrophysical Journal Supplement Series . 74 : 1075.
Bibcode :
1990ApJS...74.1075M .
doi :
10.1086/191527 .
^
a
b Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters , 38 (5): 331,
arXiv :
1108.4971 ,
Bibcode :
2012AstL...38..331A ,
doi :
10.1134/S1063773712050015 ,
S2CID
119257644 .
^
a
b Famaey, B.; Jorissen, A.; Luri, X; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters". Astronomy and Astrophysics . 430 : 165.
arXiv :
astro-ph/0409579 .
Bibcode :
2005A&A...430..165F .
doi :
10.1051/0004-6361:20041272 .
S2CID
17804304 .
^
a
b
c Martig, Marie; Fouesneau, Morgan; Rix, Hans-Walter; Ness, Melissa; Mészáros, Szabolcs; García-Hernández, D. A.; Pinsonneault, Marc; Serenelli, Aldo; Aguirre, Victor Silva; Zamora, Olga (2016). "Red giant masses and ages derived from carbon and nitrogen abundances". Monthly Notices of the Royal Astronomical Society . 456 (4): 3655.
arXiv :
1511.08203 .
Bibcode :
2016MNRAS.456.3655M .
doi :
10.1093/mnras/stv2830 .
S2CID
54647886 .
^
a
b
c
d Bubar, Eric J.; King, Jeremy R. (2010). "Spectroscopic Abundances and Membership in the Wolf 630 Moving Group". The Astronomical Journal . 140 (2): 293.
arXiv :
1005.1205 .
Bibcode :
2010AJ....140..293B .
doi :
10.1088/0004-6256/140/2/293 .
S2CID
118455341 .
^
a
b
"94 Psc" .
SIMBAD .
Centre de données astronomiques de Strasbourg . Retrieved 2019-03-25 .
^ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems",
Monthly Notices of the Royal Astronomical Society , 389 (2): 869–879,
arXiv :
0806.2878 ,
Bibcode :
2008MNRAS.389..869E ,
doi :
10.1111/j.1365-2966.2008.13596.x ,
S2CID
14878976 .
^ Bubar, Eric J.; King, Jeremy R. (August 2010), "Spectroscopic Abundances and Membership in the Wolf 630 Moving Group", The Astronomical Journal , 140 (2): 293–318,
arXiv :
1005.1205 ,
Bibcode :
2010AJ....140..293B ,
doi :
10.1088/0004-6256/140/2/293 ,
S2CID
118455341 .
^ Tautvaišienė, G.; et al. (December 2010), "C, N and O abundances in red clump stars of the Milky Way",
Monthly Notices of the Royal Astronomical Society , 409 (3): 1213–1219,
arXiv :
1007.4064 ,
Bibcode :
2010MNRAS.409.1213T ,
doi :
10.1111/j.1365-2966.2010.17381.x ,
S2CID
119182458