On October 15, 2001, an extrasolar planet was found orbiting the star.[7]Pi Mensae b is one of the most massive planets ever discovered, and has a very eccentricorbit that takes approximately 2,151 days (5.89 years) to complete. Because of its eccentricity, and being a massive brown dwarf that passes through the habitable zone, it would have disrupted the orbits of any Earth-like planets, and possibly thrown them into the star, or out into the interstellar medium.
Incorporating more accurate Hipparcos data yields a mass range for the companion to be anywhere from 10.27 to 29.9 times that of Jupiter, confirming its substellar nature with the upper limit of mass putting it in the brown dwarf range.[8]
In 2020, the true mass of Pi Mensae b was measured to be 14.1MJ via astrometry.[9] Since this is greater than 13 Jupiter masses, the object could be considered a brown dwarf, although more recent astrometric results suggest a slightly lower mass. Pi Mensae was ranked 100th on the list of top 100 target stars for the planned (but now-canceled) Terrestrial Planet Finder mission to search for Earth-like planets.
On September 16, 2018, a preprint was posted to arXiv detailing the discovery of a super-Earth on a 6.27-day orbit around the star, the first exoplanet detection by the Transiting Exoplanet Survey Satellite (TESS) submitted for publication.[10] This was confirmed two days later, where the attention was called that the system is amenable for future planet atmospheric studies.[11]
In 2020, an analysis with Gaia DR2 and Hipparcosastrometry showed that planets b and c are located on orbits mutually inclined by 49°−131° (1 sigma), which causes planet c to not transit most of the time, and acquire large misalignments with its host star's spin axis.[12]
Planet c likely formed on a wide orbit, and then migrated inward under the gravitational influence of the planet or brown dwarfb.[13] It is likely to retain a portion of primordial, highly volatile atmosphere.[14]
In 2022, the discovery by the radial velocity method of a third planet, Pi Mensae d, on a 125-day orbit was announced.[15] Another 2022 study did not confirm this planet,[16] but a 2023 study did detect it.[17]: 24
^ abcJohnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4 (99): 99. Bibcode:1966CoLPL...4...99J.
^Reffert, S.; Quirrenbach, A. (2011). "Mass constraints on substellar companion candidates from the re-reduced Hipparcos intermediate astrometric data: nine confirmed planets and two confirmed brown dwarfs". Astronomy & Astrophysics. 527. id.A140. arXiv:1101.2227. Bibcode:2011A&A...527A.140R. doi:10.1051/0004-6361/201015861. S2CID54986291.
^Gandolfi, D.; Barragan, O.; Livingston, J.; Fridlund, M.; Justesen, A. B.; Redfield, S.; Fossati, L.; Mathur, S.; Grziwa, S.; Cabrera, J.; Garcia, R. A.; Persson, V.; van Eylen, V.; Hatzes, A. P.; Hidalgo, D.; Bugnet, L.; Cochran, W. D.; Csizmadia, Sz.; Deeg, H.; Eigmueller, Ph.; Endl, M.; Erikson, E.; Esposito, M.; Guenther, E.; Korth, J.; Luque, R.; Montanes-Rodriguez, P.; Nespral, D.; Nowak, G.; Paetzold, M.; Prieto-Arranz, J. (2019). "TESS's first planet: a super-Earth transiting the naked-eye star Pi Mensae". Astronomy & Astrophysics. 619 (1): L10. arXiv:1809.07573. Bibcode:2018A&A...619L..10G. doi:10.1051/0004-6361/201834289.
^Xuan, Jerry W.; Wyatt, Mark C. (2020), "Evidence for a high mutual inclination between the cold Jupiter and transiting super Earth orbiting π Men", Monthly Notices of the Royal Astronomical Society, 497 (2): 2096–2118, arXiv:2007.01871, doi:10.1093/mnras/staa2033
^Kunovac Hodžić, Vedad; Triaud, Amaury H M J.; Cegla, Heather M.; Chaplin, William J.; Davies, Guy R. (2021), "Orbital misalignment of the super-Earth π Men c with the spin of its star", Monthly Notices of the Royal Astronomical Society, 502 (2): 2893–2911, arXiv:2007.11564, doi:10.1093/mnras/stab237
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