25 Orionis

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25 Orionis, Ψ1 Ori
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25 Orionis is located roughly between δ Ori and γ Ori.
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05h 24m 44.8265s[1]
Declination 01° 50′ 47.201″[1]
Apparent magnitude (V) 4.873
Characteristics
Spectral type B1Vpe[1]
U−B color index -0.92[2]
B−V color index -0.20[2]
Astrometry
Radial velocity (Rv) 19.3[1] km/s
Proper motion (μ) RA: 0.12[1] mas/yr
Dec.: -0.60[1] mas/yr
Parallax (π) 2.94 ± 0.87[3] mas
Distance approx. 1,100 ly
(approx. 300 pc)
Details
Mass 10.5[4] M
Radius 6.4[5] R
Luminosity 10,500[4] L
Surface gravity (log g) 4.0[5] cgs
Temperature 24,661 ± 339[5] K
Rotational velocity (v sin i) 316[6] km/s
Age ~100[4] Myr
Other designations
Ψ1 Ori, 25 Ori, HR 1789, BD +01° 1005, HD 35439, FK5 2406, HIP 25302, SAO 112734, GC 6660, CCDM J05247+0150A, AAVSO 0519+01
Database references
SIMBAD data

25 Orionis, less commonly known by its Bayer designation Psi1 Orionis (Ψ1 Orionis, Ψ1 Ori) is a fifth-magnitude star in the constellation Orion. Its kinematics place it among a dense cluster of almost 200 low-mass pre-main-sequence stars in the Orion OB1a subassociation known as the 25 Orionis group.[7]

Properties

Like the star Pleione in the Pleiades open cluster, 25 Ori is a Be star with a gaseous circumstellar disk. The SIMBAD astronomical database lists its spectral class as B1Vpe.[1] The suffix "pe" refers to "Emission lines with peculiarity", a classification typical of many Be stars whose peculiar emissions come from the gaseous equatorial disks formed of material ejected from the star.

25 Orionis is a fast rotator, clocking a rotational velocity of 316 km/s, significantly faster than Achernar's speed of 251 km/s in the constellation Eridanus.[6][8] Having a radius of 6 R, the star rotates on its axis roughly once every 23 hours. With a mass in excess of 10 M, the star is expected to explode as a supernova.[4]

See also

References

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External links

Coordinates: Sky map 05h 24m 44.80s, +01° 50′ 47.0″