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Phi Persei information


φ Persei
Location of φ Persei (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 01h 43m 39.63792s[1]
Declination 50° 41′ 19.4328″[1]
Apparent magnitude (V) 4.06[2] (3.96 - 4.11[3])
Characteristics
Spectral type B2Vep[4] + sdO[5]
U−B color index −0.92[2]
B−V color index −0.04[2]
Variable type γ Cas[3]
Astrometry
Radial velocity (Rv)+0.80[6] km/s
Proper motion (μ) RA: +24.59[1] mas/yr
Dec.: −14.01[1] mas/yr
Parallax (π)4.54 ± 0.20 mas[1]
Distance720 ± 30 ly
(220 ± 10 pc)
Absolute magnitude (MV)−3.11[7]
Orbit[7][8]
Period (P)126.6731 days
Semi-major axis (a)5.89 mas
Inclination (i)77.6°
Longitude of the node (Ω)295.7°
Periastron epoch (T)2456110.03
Semi-amplitude (K1)
(primary)
9.97 km/s
Semi-amplitude (K2)
(secondary)
81.3 km/s
Details
A
Mass9.6[9] M
Radius5.5 - 8.0[7] R
Luminosity14,454[9] L
Surface gravity (log g)4.46[10] cgs
Temperature29,300[9] K
Rotational velocity (v sin i)440[10] km/s
B
Mass1.14[11] M
Radius1.3[11] R
Luminosity6,310[9] L
Surface gravity (log g)4.2[9] cgs
Temperature53,000[11] K
Age57±9[9] Myr
Other designations
φ Persei, φ Per, Phi Per, 54 Andromedae, BD+49°444, FK5 57, GC 2102, HD 10516, HIP 8068, HR 496, PPM 26670, SAO 22554
Database references
SIMBADdata

Phi Persei (Phi Per, φ Persei, φ Per) is a class B2Vep fourth-magnitude star in the constellation Perseus, location about 720 light-years from Earth.

  1. ^ a b c d e Cite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
  2. ^ a b c Cite error: The named reference Ducati2002 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference gcvs was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference Hoffleit1991 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Mourard2015 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference Wilson1953 was invoked but never defined (see the help page).
  7. ^ a b c Cite error: The named reference gies was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference navy was invoked but never defined (see the help page).
  9. ^ a b c d e f Cite error: The named reference schootemeijer2018 was invoked but never defined (see the help page).
  10. ^ a b Cite error: The named reference Zorec2016 was invoked but never defined (see the help page).
  11. ^ a b c Cite error: The named reference subluminous was invoked but never defined (see the help page).

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Phi Persei

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Phi Persei (Phi Per, φ Persei, φ Per) is a class B2Vep fourth-magnitude star in the constellation Perseus, location about 720 light-years from Earth....

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Gamma Cassiopeiae variable

Last Update:

Goraya, P. S. (April 1988). "Scanner observations of shell stars Phi Persei and Psi Persei". Astrophysics and Space Science. 143 (1): 99–105. Bibcode:1988Ap&SS...

Word Count : 781

51 Andromedae

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refers to an asterism consisting of 51 Andromedae, Gamma Andromedae, Phi Persei, 49 Andromedae, Chi Andromedae, Upsilon Andromedae, Tau Andromedae, 56...

Word Count : 747

Upsilon Andromedae

Last Update:

refers to an asterism consisting of Upsilon Andromedae, Gamma Andromedae, Phi Persei, 51 Andromedae, 49 Andromedae, Chi Andromedae, Tau Andromedae, 56 Andromedae...

Word Count : 3386

Gamma Persei

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consisting of γ Persei, η Persei, α Persei, ψ Persei, δ Persei, 48 Persei, μ Persei and HD 27084. Consequently, the Chinese name for γ Persei itself is 天船二...

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Beta Canis Minoris

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Be primary. If confirmed, this would make it a member of the very rare Phi Persei Be+sdO-type systems. van Leeuwen, F. (November 2007). "Validation of the...

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Superluminal motion

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The apparent superluminal motion in the faint nebula surrounding Nova Persei was first observed in 1901 by Charles Dillon Perrine. “Mr. Perrine’s photograph...

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Zeta Herculis Moving Group

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members were identified. Among the group members he included β Hydri, ρ Persei, η Reticuli, φ1 Lupi, ζ Herculis and ε Octantis. He estimated the group...

Word Count : 358

Omicron

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position. Such stars include Omicron Andromedae, Omicron Ceti, and Omicron Persei. In Claudius Ptolemy's (c. 100–170) Almagest, tables of sexagesimal numbers...

Word Count : 1614

List of brightest natural objects in the sky

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Gruis Star 1.77 1.75 Alioth Star 1.77 Alnitak Triple star system 1.79 Alpha Persei Star 1.79 Dubhe Binary star system 1.84 Delta Canis Majoris Star 1.85 Epsilon...

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Open cluster

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number of open clusters, such as the Pleiades, the Hyades and the Alpha Persei Cluster, are visible with the naked eye. Some others, such as the Double...

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Mithraism

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horns. The context is a prayer to the god Phoebus. The cave is described as persei, which in this context is usually translated Persian. According to the translator...

Word Count : 20830

List of Chinese star names

Last Update:

Corpses Pi Persei Perseus A single-star asterism in the Stomach mansion. 積水 Jī Shuǐ Stored Water Lambda Persei 天讒 Tiān Chán Celestial Slander 42 Persei 北落師門...

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