Astronomy:TOI-2180 b
 illustration of TOI-2180 b | |
| Discovery | |
|---|---|
| Discovered by | The TESS-Keck Survey |
| Discovery date | February 2022 |
| Transit Method | |
| Designations | |
| HD 238894 b | |
| Orbital characteristics | |
| 0.828±0.012 au[1] | |
| Eccentricity | 0.3683 ± 0.0073[1] |
| Orbital period | 260.15764 ± 0.00045 days[2] |
| Inclination | 89.955+0.032 −0.044[1] |
| Star | HD 238894 |
| Physical characteristics | |
| Mean radius | 1.010+0.022 −0.019 |♃|J}}}}}} |
| Mass | 2.755+0.087 −0.081 |♃|J}}}}}}[1] |
| 3.827+0.012 −0.015 dex[1] | |
| Physics | 348.0+3.3 −3.6 K[1] |
TOI-2180 b is a giant exoplanet orbiting the G-type star TOI-2180, also known as HD 238894.[1] It was discovered with the help of the Transiting Exoplanet Survey Satellite and is currently the exoplanet with the longest orbital period TESS was able to uncover (as of September 2022).[3] TOI-2180 b orbits its host star every 260.16 days.[2]
Discovery
TOI-2180 b was first identified as an exoplanet candidate due to a single transit with TESS at 12./13. December 2019 by a group of citizen scientists called the Visual Survey Group, which includes Thomas Lee Jacobs, a former U.S. naval officer.[4] The group was using the light curve processing tool lcTools. In May 2020 the Planet Hunters: TESS collaboration announced this object as a Community TESS Object of Interest (CTOI) and it was soon promoted into a regular TOI.[1]
The TESS-Keck Survey collaboration performed radial velocity follow-up observations for nearly 2 years with the Automated Planet Finder and Keck I. The follow-up observations uncovered that the single transit was caused by a long-period planet.[1]
Orbital properties
TOI-2180 b has a long orbital period of 260.16 days,[2] which also leads to a long transit duration of 24 hours.[1] The distance to the host star is 82.8% the sun-earth distance.[1] The planet does not orbit inside the habitable zone, despite this close resemblance in semi-major axis.[5] TOI-2180 b has a high eccentricity of the orbit at 0.37.[1]
The second transit was not detected from the ground and the third transit was not observed.[1] The fourth transit was observed at 31. January/01. February 2022, refining the orbital period. The next transit will occur on 2022 October 18 at 21:28 UTC.[2]
Physical properties
The planet has the same size as Jupiter, but is 2.8 times heavier than Jupiter. TOI-2180 b stand out because of its cold estimated temperature of about 348 Kelvin (74.9 °C, 166.7 °F).[1] This is closer to Jupiters 165 K than most discovered giant exoplanets. TOI-2180 b belongs to a small sample of temperature Jupiters with a temperature <400 K that transit, such as Kepler-167 e, WD 1856+534 b, Kepler-1704 b, KOI-3680 b, Kepler-1514 b and Kepler-539 b. TOI-2180 b has by far the brightest host star with a visual magnitude of 9.16, which is about 3 magnitudes brighter than the next brightest system in this sample.[5]
The planet is likely enriched in metals compared to its host star. The discovery team inferred that TOI-2180 b is enriched in metals by a factor of about 5 compared to its host star. This means it has about 100 M⊕ of heavy elements in its envelope and interior.[1]
Future observations
The exoplanet is a poor target for transmission spectroscopy because of its high surface gravity and the large radius of the host star. The large radius of the star causes a relative shallow transit depth of about 0.5%. The system is still an excellent target to find rings and exomoons around TOI-2180 b. It is also a good target to study the migration of exoplanets.[1] It could be one of the best targets for exomoon searches.[6]
Host star
The host star is a 9.16 magnitude[7] bright and slightly evolved star with a spectral type of G5. It has a mass of 1.1 M☉ and a radius of 1.6 R☉. The radius is increased due to the evolved nature of the star. The star is 116 parsec (379 light-years) distant from earth and has an age of about 8.1 billion years.[1]
Habitable Zone
Currently the habitable zone around TOI-2180 is between 1.5 and 2.2 astronomical units.[1][note 1] Because TOI-2180 is slightly evolved, it had a habitable zone closer to the star in the past. At an age of about 3 billion years the habitable zone was located between 1.1 and 1.6 astronomical units.[1][8][note 2]
Outer planet candidate
The radial velocity monitoring also showed acceleration of TOI 2180 b due to an outer planet or low-mass star in the system.[1] A later analysis of RV data has shown that an outer companion has an orbital period of 1558+68
−19 days, an eccentricity of about 0.31 and a minimum mass of 3.94+0.27
−0.22 MJ, making it likely a giant planet. The acceleration (TTV) and the outer companion detected in the RV could be the same object.[6]
Notes
- ↑ Using a luminosity of 2.544 by Dalba et al. and using step 2 by Morris
- ↑ Using MIST evolutionary track with initial mass=1.115 Msun (best match from isochromes), initial metallicity [Fe/H]=0.269 (Delba et al for TOI-2180) and using synthetic photometry output UBV etc. Then the approach by Morris was used, assuming the star was an F-type back then.
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 1.13 1.14 1.15 1.16 1.17 1.18 1.19 Dalba, Paul A.; Kane, Stephen R.; Dragomir, Diana; Villanueva, Steven; Collins, Karen A.; Jacobs, Thomas Lee; LaCourse, Daryll M.; Gagliano, Robert et al. (2022-02-01). "The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope". The Astronomical Journal 163 (2): 61. doi:10.3847/1538-3881/ac415b. ISSN 0004-6256. Bibcode: 2022AJ....163...61D.
- ↑ 2.0 2.1 2.2 2.3 Dalba, Paul A.; Jacobs, Thomas Lee; Omohundro, Mark; Gagliano, Robert; Jursich, Jay; Kristiansen, Martti H.; LaCourse, Daryll M.; Schwengeler, Hans M. et al. (2022-04-01). "The Refined Transit Ephemeris of TOI-2180 b". Research Notes of the American Astronomical Society 6 (4): 76. doi:10.3847/2515-5172/ac64fd. ISSN 2515-5172. Bibcode: 2022RNAAS...6...76D.
- ↑ "Planetary Systems". https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=PS.
- ↑ Landau, Elizabeth (2022-01-11). "Citizen Scientists Spot Jupiter-like Planet". http://www.nasa.gov/feature/citizen-scientists-spot-jupiter-like-planet-in-nasa-tess-data.
- ↑ 5.0 5.1 "Exoplanet-catalog". https://exoplanets.nasa.gov/exoplanet-catalog/8374/toi-2180-b/.
- ↑ 6.0 6.1 Dalba, Paul A.; Kane, Stephen R.; Isaacson, Howard; Fulton, Benjamin; Howard, Andrew W.; Schwieterman, Edward W.; Thorngren, Daniel P.; Fortney, Jonathan et al. (2024-01-01), Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets, doi:10.48550/arXiv.2401.03021, https://ui.adsabs.harvard.edu/abs/2024arXiv240103021D, retrieved 2024-01-27
- ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (2000-03-01). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H. https://ui.adsabs.harvard.edu/abs/2000A&A...355L..27H.
- ↑ "MIST". http://waps.cfa.harvard.edu/MIST/interp_tracks.html.
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