Pi1 Orionis

Star in the constellation Orion From Wikipedia, the free encyclopedia

Pi1 Orionis1 Ori, π1 Orionis) is a star in the equatorial constellation of Orion. It is faintly visible to the naked eye with an apparent visual magnitude of 4.74.[2] Based upon an annual parallax shift of 28.04 mas,[1] it is located about 116 light-years from the Sun.

Right ascension04h 54m 53.72877s[1]
Declination+10° 09 02.9952[1]
Quick facts Constellation, Right ascension ...
π1 Orionis
Location of π1 Orionis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Orion
Right ascension 04h 54m 53.72877s[1]
Declination +10° 09 02.9952[1]
Apparent magnitude (V) 4.74[2]
Characteristics
Spectral type A3 Va[3]
U−B color index +0.09[2]
B−V color index +0.08[2]
Astrometry
Proper motion (μ) RA: +41.49[1] mas/yr
Dec.: −128.73[1] mas/yr
Parallax (π)28.04±0.25 mas[1]
Distance116 ± 1 ly
(35.7 ± 0.3 pc)
Absolute magnitude (MV)1.71±0.09[4]
Details[4]
Mass1.90+0.08
−0.09
 M
Radius1.73±0.13 R
Luminosity16.91+1.42
−1.29
 L
Surface gravity (log g)4.22+0.04
−0.05
 cgs
Temperature8,900±131 K
Metallicity [Fe/H]−0.12+0.14
−0.16
 dex
Rotational velocity (v sin i)120[5] km/s
Age100[6] Myr
Other designations
π1 Ori, 7 Orionis, BD+09°683, HD 31295, HIP 22845, HR 1570, SAO 94201[7]
Database references
SIMBADdata
Close

This is an A-type main-sequence star with a stellar classification of A3 Va.[3] It is a Lambda Boötis star,[8] which means the spectrum shows lower-than-expected abundances for heavier elements.[9] Pi1 Orionis is a relatively young star, just 100 million years old,[6] and is spinning fairly rapidly with a projected rotational velocity of 120 km/s.[5] It has nearly double the mass of the Sun and 173% of the Sun's radius. The star radiates 16.9 times the solar luminosity from its outer atmosphere at an effective temperature of 8,900 K.[4]

An infrared excess indicates there is a debris disk with a temperature of 80 K orbiting 49 AU from the star. The dust has a combined mass 2.2% that of the Earth.[6]

References

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