HD 25171#Planetary system

{{Starbox begin

| name = HD 25171

}}

{{Starbox observe

| epoch = J2000.0

| equinox = J2000.0 (ICRS)

| constell = Reticulum

| ra = {{RA|03|55|49.440}}

| dec = {{DEC|–65|11|12.03}}

| appmag_v = 7.79

}}

{{Starbox character

| class = F8 V

| u-b =

| b-v = 0.554

| r-i =

}}

{{Starbox astrometry

| radial_v = +42.8

| prop_mo_ra = +144.020

| prop_mo_dec = +81.550

| pm_footnote =

| parallax = 17.928

| p_error = 0.0163

| parallax_footnote =

| absmag_v = 4.09{{±|0.07}}

}}

{{Starbox detail

| rotational_velocity = 1.0

| rotation = 14.4{{±|0.6}} d

| radius = 1.069{{±|0.041}}

| luminosity = 1.89

| temperature = 6,063{{±|50}}

| gravity = 4.17{{±|0.1}}

| mass = 1.09{{±|0.03}}

| metal_fe = −0.11{{±|0.04}}

| age_gyr = 4.0{{±|1.6}}

}}

{{Starbox catalog

| names = {{odlist | CD=–65 199 | HD=25171 | HIP=9141 | SAO=248911 | TYC 8874-376-1 }}

}}

{{Starbox reference

| Simbad = HD+25171

}}

HD 25171 is a star with an orbiting exoplanet[https://web.archive.org/web/20101225195413/http://exoplanet.eu/star.php?st=HD+25171 HD 25171 System] in the southern constellation of Reticulum, the reticle. With an apparent visual magnitude of 7.79, this star is too faint to be viewed with the naked eye. However, it is readily visible through a small telescope from the southern hemisphere. Parallax measurements place it at a distance of roughly {{Convert|182|ly|pc|abbr=off|lk=on}} from Earth. It is drifting further away with a heliocentric radial velocity of +43 km/s.

Based upon its spectrum, this is an ordinary F-type main sequence star with a stellar classification of F8 V. It is slightly larger than the Sun, with 9% more mass and an 7% greater radius. As such, it is radiating 189% of the Sun's luminosity from its outer atmosphere at an effective temperature of 6,063 K. This gives it the yellow-white hued glow of an F-type star. It appears to be roughly the same age as the Sun; around four billion years.

A survey in 2015 ruled out the existence of any stellar companions at projected distances above 26 astronomical units.{{cite journal |last1=Mugrauer |first1=M. |last2=Ginski |first2=C. |title=High-contrast imaging search for stellar and substellar companions of exoplanet host stars |journal=Monthly Notices of the Royal Astronomical Society |date=12 May 2015 |volume=450 |issue=3 |pages=3127–3136 |doi=10.1093/mnras/stv771 |bibcode=2015MNRAS.450.3127M |url=https://academic.oup.com/mnras/article/450/3/3127/1063872 |accessdate=19 June 2020|doi-access=free |hdl=1887/49340 |hdl-access=free }}

Planetary system

The planetary companion was discovered in 2010 with the HARPS instrument, which measured the radial velocity displacement caused by the gravitational perturbation of the star by the planet. This data provided an orbital period of 1,845 days and set a lower bound of the planet's mass at 95% of the mass of Jupiter. The planetary system of HD 25171 is analogous to Solar System in the sense that a gas giant orbiting outside the frost line, far enough to do not destabilize orbits within a circumstellar habitable zone.{{cite journal|arxiv=1804.06547|title=Properties of the single Jovian planet population and the pursuit of Solar system analogues|year=2018|doi=10.1093/mnras/sty868|last1=Agnew|first1=Matthew T.|last2=Maddison|first2=Sarah T.|last3=Horner|first3=Jonathan|s2cid=119232995|journal=Monthly Notices of the Royal Astronomical Society|volume=477|issue=3|pages=3646–3658|doi-access=free |bibcode=2018MNRAS.477.3646A}}

{{OrbitboxPlanet begin

| table_ref =

}}

{{OrbitboxPlanet

| exoplanet = b

| mass = >0.956{{±|0.234}}

| period = {{val|1845|15}}

| semimajor = {{val|3.02|0.16}}

| eccentricity = {{val|0.08|0.06}}

}}

References

{{reflist|refs=

{{cite simbad

| title=HD 25171

| access-date = 2023-12-12 }}

{{cite journal|arxiv=1802.06794|year=2018|doi=10.3847/1538-4357/aaafca|last1=Buchhave|first1=Lars A.|last2=Bitsch|first2=Bertram|last3=Johansen|first3=Anders|last4=Latham|first4=David W.|last5=Bizzarro|first5=Martin|last6=Bieryla|first6=Allyson|last7=Kipping|first7=David M.|title=Jupiter Analogs Orbit Stars with an Average Metallicity Close to That of the Sun|s2cid=119332645|journal=The Astrophysical Journal|volume=856|issue=1|page=37|bibcode=2018ApJ...856...37B |doi-access=free }}

{{citation | first=F. | last=van Leeuwen | s2cid=18759600 |date=November 2007 | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | postscript=. |arxiv = 0708.1752 }}

{{citation |doi=10.1051/0004-6361/201015371 |arxiv=1012.3830 |title=The HARPS search for southern extra-solar planets: XXVI: Seven new planetary systems |last1=Moutou |first1=Claire |last2=Mayor |first2=Michel |last3=Lo Curto |first3=Gaspare |last4=Ségransan |first4=Damien |last5=Udry |first5=Stéphane |last6=Bouchy |first6=François |last7=Benz |first7=Willy |last8=Lovis |first8=Christophe |last9=Naef |first9=Dominique |last10=Pepe |first10=Francesco |last11=Queloz |first11=Didier |last12=Santos |first12=Nuno C. |last13=Sousa |first13=Sérgio Gonçalves |s2cid=118696125 |year=2010 }}

{{citation | last1=Holmberg | first1=J. | last2=Nordstrom | first2=B. | last3=Andersen | first3=J. | s2cid=118577511 | title=The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics | journal=Astronomy and Astrophysics | volume=501 | issue=3 |date=July 2009 | pages=941–947 | doi=10.1051/0004-6361/200811191 | bibcode=2009A&A...501..941H | postscript=. |arxiv = 0811.3982 }}

{{citation|title=Characterisation of the radial velocity signal induced by rotation in late-type dwarfs|year=2017|doi=10.1093/mnras/stx771|arxiv=1703.08884|last1=Suárez Mascareño|first1=A.|last2=Rebolo|first2=R.|last3=González Hernández|first3=J. I.|last4=Esposito|first4=M.|s2cid=119215361|journal=Monthly Notices of the Royal Astronomical Society|volume=468|issue=4|pages=4772–4781|doi-access=free |bibcode=2017MNRAS.468.4772S}}

}}

Category:F-type main-sequence stars

Category:Planetary systems with one confirmed planet

Category:Reticulum

Category:Durchmusterung objects

025171

009141