HD 131496 is an evolved subgiant star with an orbiting exoplanet in the constellation Boötes. With an apparent visual magnitude of 7.9 it is too faint to be visible to the naked eye. It is located at a distance of 432 light-years based on parallax measurements,^[2] and is drifting further away with a heliocentric radial velocity of 1.4 km/s.^[5] At an age of around three billion years, this star has 1.6 times the mass of the Sun and has expanded to 4.3 times the Sun's radius. It is radiating around ten times the luminosity of the Sun from its photosphere at an effective temperature of 4,927 K.^[3]

Stars like HD 131496 are sometimes referred to as "retired A-stars", since they would have been A-type stars while on the main sequence. This name is most commonly used in connection with the search for extrasolar planets, where they are useful because these evolved stars are cooler and have more spectral lines than their main sequence counterparts, making planet detection easier.^[7]

HD 131496 and its planet, HD 131496b, were chosen as part of the 2019 NameExoWorlds campaign organised by the International Astronomical Union, which assigned each country a star and planet to be named. HD 131496 was assigned to Andorra. The winning proposal for the name of the star was Arcalís, after a mountain peak in northern Andorra where the Sun shines through a gap twice a year at fixed dates, leading to its use as a primitive Solar calendar. The planet was named Madriu, after a glacial valley and river in southeastern Andorra that forms the major part of the Madriu-Perafita-Claror UNESCO World Heritage Site.^[8]

Planetary system[edit]

An exoplanet was discovered in 2011. It has a mass at least 2.2 times that of Jupiter and is orbiting at a distance of 2.09 astronomical units (AU) once every 883 days.^[3]

The HD 131496 planetary system^[9]

Companion
(in order from star)

Mass

Semimajor axis
(AU)

Orbital period
(days)

Eccentricity

Inclination

Radius

b / Madriu

≥2.2±0.2 $M$ _J

2.09±0.07

883±29

0.163±0.073

—

References[edit]

^ ^a ^b Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644.

^ ^a ^b ^c ^d ^e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this sourceatVizieR.

^ ^a ^b ^c ^d ^e ^f Johnson, John Asher; Clanton, Christian; Howard, Andrew W.; Bowler, Brendan P.; Henry, Gregory W.; Marcy, Geoffrey W.; Crepp, Justin R.; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Wright, Jason T. (2011). "Retired A Stars and Their Companions. VII. 18 New Jovian Planets". The Astrophysical Journal Supplement Series. 197 (2): 26. arXiv:1108.4205. Bibcode:2011ApJS..197...26J. doi:10.1088/0067-0049/197/2/26. hdl:2152/42985. ISSN 0067-0049. S2CID 15088371.

^ Cannon, A. J.; Pickering, E. C. (1993). "VizieR Online Data Catalog: Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989)". VizieR On-line Data Catalog. Bibcode:1993yCat.3135....0C.