Pi1 Orionis

{{Short description|Star in the constellation Orion}}

{{for|other stars with this Bayer designation|Pi Orionis}}

{{DISPLAYTITLE:Pi1 Orionis}}

{{Starbox begin

| name = π1 Orionis}}

{{Starbox image

| image=

{{Location mark

|image=Orion constellation map.svg|alt=|float=center|width=280

|label=|position=right

|mark=Red circle.svg|mark_width=10|mark_link=π1 Orionis

|x=860|y=232

}}

|caption=Location of π1 Orionis (circled)

}}

{{Starbox observe

| epoch = J2000.0

| equinox = J2000.0 (ICRS)

| constell = Orion

| ra = {{RA|04|54|53.72877}}

| dec = {{DEC|+10|09|02.9952}}

| appmag_v = 4.74

}}

{{Starbox character

| class = A3 Va

| u-b = +0.09

| b-v = +0.08

| r-i =

}}

{{Starbox astrometry

| radial_v =

| prop_mo_ra = +41.49

| prop_mo_dec = −128.73

| parallax = 28.04

| p_error = 0.25

| parallax_footnote =

| absmag_v = {{val|1.71|0.09}}

}}

{{Starbox detail

| source =

| mass = {{val|1.90|0.08|0.09}}

| radius = {{val|1.73|0.13}}

| luminosity = {{val|16.91|1.42|1.29}}

| temperature = {{val|8900|131|fmt=commas}}

| gravity = {{val|4.22|0.04|0.05}}

| metal_fe = {{val|-0.12|0.14|0.16}}

| rotational_velocity = 120

| rotation =

| age_myr = 100

}}

{{Starbox catalog

| names = π1 Ori, 7 Orionis, BD+09°683, HD 31295, HIP 22845, HR 1570, SAO 94201

}}

{{Starbox reference

|Simbad=7+Ori

}}

{{Starbox end}}

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. Based upon an annual parallax shift of 28.04 mas, it is located about 116 light-years from the Sun.

This is an A-type main-sequence star with a stellar classification of A3 Va. It is a Lambda Boötis star, which means the spectrum shows lower-than-expected abundances for heavier elements. Pi1 Orionis is a relatively young star, just 100 million years old, and is spinning fairly rapidly with a projected rotational velocity of 120 km/s. 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 {{Val|8900|fmt=commas|ul=K}}.

An infrared excess indicates there is a debris disk with a temperature of 80 K orbiting {{Val|49|ul=AU}} from the star. The dust has a combined mass 2.2% that of the Earth.

References

{{reflist|refs=

{{citation

| title=Validation of the new Hipparcos reduction

| last1=van Leeuwen | first1=F.

| journal=Astronomy and Astrophysics

| volume=474 | issue=2 | pages=653–664 | date=2007

| arxiv=0708.1752 | bibcode=2007A&A...474..653V

| doi=10.1051/0004-6361:20078357 | s2cid=18759600 | postscript=. }}

{{Cite journal |last1=Murphy |first1=S. J. |last2=Paunzen |first2=E. |last3=Bedding |first3=T. R. |last4=Walczak |first4=P. |last5=Huber |first5=D. |date=2020-06-01 |title=The pulsation properties of λ bootis stars I. the southern TESS sample |journal=Monthly Notices of the Royal Astronomical Society |volume=495 |issue=2 |pages=1888–1912 |doi=10.1093/mnras/staa1271 |doi-access=free |bibcode=2020MNRAS.495.1888M |arxiv=2005.09187 |issn=0035-8711}}

{{citation

| title=λ Bootis stars: Current status and new insights from Spitzer

| display-authors=1

| last1=Kamp | first1=I. | last2=Martínez-Galarza | first2=J. R.

| last3=Paunzen | first3=E. | last4=Su | first4=K. Y. L.

| last5=Gáspár | first5=A. | last6=Rieke | first6=G. H.

| journal=Contributions of the Astronomical Observatory Skalnaté Pleso

| volume=38 | issue=2 | pages=147–156 | date=April 2008

| bibcode=2008CoSka..38..147K | postscript=. }}

{{citation

| last1=Mermilliod | first1=J.-C.

| title=Compilation of Eggen's UBV data, transformed to UBV (unpublished)

| journal=Catalogue of Eggen's UBV Data

| year=1986 | publisher=SIMBAD

| bibcode=1986EgUBV........0M | postscript=. }}

{{citation

| title=A search for Lambda Bootis stars in OB associations

| last1=Gray | first1=R. O. | last2=Corbally | first2=C. J.

| journal=Astronomical Journal

| volume=106 | issue=2 | pages=632–636 | date=August 1993

| doi=10.1086/116668 | bibcode=1993AJ....106..632G

| postscript=. }}

{{citation

| display-authors=1 | last1=Royer | first1=F.

| last2=Zorec | first2=J. | last3=Gómez | first3=A. E.

| title=Rotational velocities of A-type stars. III. Velocity distributions

| journal=Astronomy and Astrophysics

| volume=463 | issue=2 | pages=671–682 | date=February 2007

| doi=10.1051/0004-6361:20065224 | bibcode=2007A&A...463..671R

| arxiv=astro-ph/0610785 | s2cid=18475298 | postscript=. }}

{{citation

| display-authors=1

| last1=Rhee | first1=Joseph H. | last2=Song | first2=Inseok

| last3=Zuckerman | first3=B. | last4=McElwain | first4=Michael

| title=Characterization of Dusty Debris Disks: The IRAS and Hipparcos Catalogs

| journal=The Astrophysical Journal

| volume=660 | issue=2 | pages=1556–1571 | date=May 2007

| doi=10.1086/509912 | bibcode=2007ApJ...660.1556R

| arxiv=astro-ph/0609555 | s2cid=11879505 | postscript=. }}

{{citation

| display-authors=1

| last1=Gray | first1=R. O. | last2=Corbally | first2=C. J.

| last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T.

| last5=Bubar | first5=E. J. | last6=McGahee | first6=C. E.

| last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R.

| title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample

| journal=The Astronomical Journal

| volume=132 | issue=1 | pages=161–170 | date=July 2006

| doi=10.1086/504637 | bibcode=2006AJ....132..161G

| arxiv=astro-ph/0603770 | s2cid=119476992 | postscript=. }}

{{cite simbad

| title=* pi.01 Ori

| access-date=2016-11-15 | postscript=. }}

}}

{{Stars of Orion|state=collapsed}}

{{DEFAULTSORT:Pi1 Orionis}}

Category:A-type main-sequence stars

Category:Orion (constellation)

Orionis, Pi1

Orionis, 07

031295

022845

01570

Category:Durchmusterung objects