HD 141937

{{short description|Star in the constellation Libra}}

{{Starbox begin}}

{{Starbox observe

| epoch = J2000

| constell = Libra

| ra = {{RA|15|52|17.54814}}

| dec = {{DEC|−18|26|09.7939}}

| appmag_v = 7.25

}}

{{Starbox character

| type =

| class = G1V

| b-v = {{Val|+0.628|0.002}}

| u-b =

| variable =

}}

{{Starbox astrometry

| radial_v = {{Val|−2.20|0.68}}

| prop_mo_ra = {{val|+97.231|0.133}}

| prop_mo_dec = {{val|+19.113|0.116}}

| parallax = 29.9453

| p_error = 0.0640

| parallax_footnote =

| absmag_v = 4.71

}}

{{Starbox detail

| source =

| mass = 1.03

| radius = 1.05

| luminosity = {{Val|1.202|0.003}}

| gravity = 4.44

| temperature = {{Val|5890|15|30|fmt=commas}}

| metal_fe = {{Val|+0.10|0.01}}

| rotational_velocity = 6.0

| age_gyr = 3.82

}}

{{Starbox catalog

| names = {{odlist | BD=−17° 4442 | HD=141937 | HIP=77740 | SAO=159551 }}

}}

{{Starbox reference

| Simbad = HD+141937

| EPE = HD+141937

}}

{{End}}

HD 141937 is a star in the southern zodiac constellation of Libra, positioned a couple of degrees to the north of Lambda Librae. It is a yellow-hued star with an apparent visual magnitude of 7.25, which means it is too faint to be seen with the naked eye. This object is located at a distance of 108.9 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −2.2 km/s. It has an absolute magnitude of 4.71.

This is a G-type main-sequence star with a stellar classification of G1V. It is a solar-type star with slightly higher mass and radius compared to the Sun. The metallicity is higher than solar. It is an estimated 3.8 billion years old and is spinning with a projected rotational velocity of 6 km/s. The star is radiating 1.2 times the luminosity of the Sun from its photosphere at an effective temperature of 5,890 K.

The star has a substellar companion (HD 141937 b) announced in April 2001 by the European Southern Observatory. It has a minimum mass of 9.7 {{Jupiter mass|link=y}}. In 2020, the inclination of the orbit was measured, revealing its true mass to be 27.4 {{Jupiter mass|link=y}}, which makes it a brown dwarf. A 653-day orbit places the orbital distance 1.5 times farther away from the star as Earth is from the Sun, with a high eccentricity of 41%.

{{OrbitboxPlanet begin

| table_ref =

}}

{{OrbitboxPlanet

| exoplanet = b

| mass = {{val|27.42|6.78|9.86}}

| period = {{Val|653.22|1.21}}

| semimajor = {{Val|1.4877|0.0018}}

| eccentricity = {{Val|0.41|0.01}}

| inclination = {{val|20.52|12.47|4.16}}

}}

{{Orbitbox end}}

See also

References

{{Reflist|refs=

{{cite journal

| title=XHIP: An extended hipparcos compilation

| last1=Anderson | first1=E. | last2=Francis | first2=Ch.

| journal=Astronomy Letters | arxiv=1108.4971

| volume=38 | issue=5 | pages=331 | year=2012

| bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | s2cid=119257644 }}

{{cite journal

| title=Abundances in the Local Region II: F, G, and K Dwarfs and Subgiants

| last1=Luck | first1=R. Earle

| journal=The Astronomical Journal

| volume=153 | issue=1 | id=21 | pages=19 | date=January 2017

| bibcode=2017AJ....153...21L | arxiv=1611.02897

| doi=10.3847/1538-3881/153/1/21 | s2cid=119511744 | doi-access=free }}

{{cite press release

| title=Exoplanets: The Hunt Continues!

| publisher=European Southern Observatory

| date=April 4, 2001 | location=Garching, Germany

| url=http://www.eso.org/public/news/eso0114/ | access-date=December 29, 2012 }}

{{Cite Gaia DR2|6248534171318085376}}

{{cite journal

| display-authors=1 | last1=Gray | first1=R. O.

| first2=C. J. | last2=Corbally | first3=R. F. | last3=Garrison

| first4=M. T. | last4=McFadden | first5=P. E. | last5=Robinson

| title=Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Northern Sample I

| journal=The Astronomical Journal

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

| doi=10.1086/504637 | arxiv=astro-ph/0603770

| bibcode=2006AJ....132..161G | s2cid=119476992 }}

{{cite journal | title=Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets | last1=Kiefer | first1=F. | last2=Hébrard | first2=G. | last3=Lecavelier des Etangs | first3=A. | last4=Martioli | first4=E. | last5=Dalal | first5=S. | last6=Vidal-Madjar | first6=A. | display-authors=1 | journal=Astronomy & Astrophysics | volume=645 | page= | article-number=A7 | date=January 2021 | arxiv=2009.14164 | bibcode=2021A&A...645A...7K | bibcode-access=free | doi=10.1051/0004-6361/202039168 | doi-access=free | s2cid=221995447 }}

{{cite journal

| title=Precise determination of fundamental parameters of six exoplanet host stars and their planets

| last1=Liu | first1=Kang | last2=Bi | first2=Shao-Lan

| last3=Li | first3=Tan-Da | last4=Liu | first4=Zhi-E.

| last5=Tian | first5=Zhi-Jia | last6=Ge | first6=Zhi-Shuai

| display-authors=1 | journal=Research in Astronomy and Astrophysics

| volume=14 | issue=11 | id=1447-1457 | date=November 2014

| pages=1447–1457 | doi=10.1088/1674-4527/14/11/008 | arxiv=1406.2173

| bibcode=2014RAA....14.1447L | s2cid=118779573 }}

{{cite journal

| title=Li depletion in solar analogues with exoplanets. Extending the sample

| display-authors=1 | last1=Delgado Mena | first1=E.

| last2=Israelian | first2=G. | last3=González Hernández | first3=J. I.

| last4=Sousa | first4=S. G. | last5=Mortier | first5=A.

| last6=Santos | first6=N. C. | last7=Adibekyan | first7=V. Zh.

| last8=Fernandes | first8=J. | last9=Rebolo | first9=R.

| last10=Udry | first10=S. | last11=Mayor | first11=M.

| journal=Astronomy & Astrophysics

| volume=562 | id=A92 | pages=17 | date=February 2014

| doi=10.1051/0004-6361/201321493 | arxiv=1311.6414

| bibcode=2014A&A...562A..92D | s2cid=56104807 }}

{{cite simbad | title=HD 117207 | access-date=2018-07-23}}

{{cite journal

| url=http://www.aanda.org/articles/aa/full/2002/28/aa2416/aa2416.html

| display-authors=1 | last1=Udry | first1=S.

| last2=Mayor | first2=M. | last3=Naef | first3=D.

| last4=Pepe | first4=F. | last5=Queloz | first5=D.

| last6=Santos | first6=N. C. | last7=Burnet | first7=M.

| title=The CORALIE survey for southern extra-solar planets VIII. The very low-mass companions of HD141937, HD162020, HD168443, HD202206: brown dwarfs or superplanets?

| journal=Astronomy and Astrophysics

| year=2002 | volume=390 | issue=1 | pages=267–279

| bibcode=2002A&A...390..267U | arxiv=astro-ph/0202458

| doi=10.1051/0004-6361:20020685 | s2cid=9389274 }}

}}

{{Sky|15|52|17.5474|-|18|26|09.834|109}}

{{Stars of Libra}}

{{DEFAULTSORT:HD 141937}}

Category:G-type main-sequence stars

Category:Brown dwarfs

Category:Libra (constellation)

Category:Durchmusterung objects

141937

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