HD 18438 b
| Discovery[1] | |
|---|---|
| Discovered by | Lee Byeong-Cheol et al. |
| Discovery date | 15 March 2023 (accepted) |
| Radial-velocity method | |
| Designations | |
| Orbital characteristics[1] | |
| 2.1±0.1 AU | |
| Eccentricity | 0.1±0.1 |
| 803±5 d | |
| Inclination | 88.49°+0.78° −0.49° |
| Semi-amplitude | 305±18 m/s |
| Star | HD 18438 |
| Physical characteristics[1] | |
| Mass | >21±1 MJ |
HD 18438 b is a substellar object, either a massive gas giant exoplanet or a brown dwarf, orbiting the star HD 18438, a red giant star located about 731 light-years (224 pc) away from Earth.[3]
Observational history
[edit]Radial velocity variations of HD 18438 were first analyzed and reported in 2018, which found regular fluctuations with a period of 719.0 days (1.969 years), longer than the stellar rotation period of 562 days (1.54 years).[4] This was then attributed to oscillations of the star itself, as they were similar to that of long secondary period (LSP) giant stars,[4] though a definite conclusion could not be established.[1]
In 2023, however, with four more years of observations, a follow-up study ruled out the association of LSP with the radial velocity variations, and instead determined that the signals, with a revised period of 803 days (2.20 years), were caused by an orbiting planetary (or brown dwarf) companion with a minimum mass of 21 MJ.[1] This also agrees with a previous study[5] that provided mass estimates for a companion to HD 18438. In this re-analysis process, the rotation period of the host star was also revised to 637 days (1.74 years) to better match the accumulated data.[1]
Physical characteristics
[edit]HD 18438 b is a massive planet with a mass of 21 MJ and an estimated radius of 1.08 RJ.[6] This is above the deuterium burning limit (~13 MJ), and thus according to some definitions, including the IAU standard, it may be classified as a brown dwarf.[7] However, other organizations deem the object a planet, such as the NASA Exoplanet Science Institute, which includes bodies as massive as 30 MJ in the NASA Exoplanet Catalog.[3][8]
Orbit
[edit]The planet orbits its host star at a distance of 2.1 AU (310,000,000 km; 200,000,000 mi), taking 803 days (2.20 years) to complete one orbit around the star. It has an orbital eccentricity of 0.1.[3]
Host star
[edit]HD 18438 is a red giant with a spectral type of M2.5 III, inflated to a diameter of 88 R☉. If HD 18438 b is to be considered a planet at all, this would make it the largest host to an exoplanet known to date as of September 2024. Its sheer size means that despite having an effective temperature significantly cooler than the Sun at 3,860 K (3,590 °C; 6,490 °F), it shines 929 times as bright. With a mass of 1.84 M☉ and an age of 5.5±2.4 Gyr, it is nearing the end of its lifespan, having long since left the main-sequence stage. The star has a low metallicity of −0.4±0.1 dex, meaning it only has an iron content between 32% and 50% that of the Sun.[1]
References
[edit]- ^ a b c d e f g Lee, Byeong-Cheol; et al. (30 December 2023). "A Search for Exoplanets around Northern Circumpolar Stars. VII. Detection of Planetary Companion Orbiting the Largest Host Star HD 18438". Journal of the Korean Astronomical Society. 56 (1): 35–40. arXiv:2303.08357. Bibcode:2023JKAS...56...35L. doi:10.5303/JKAS.2023.56.1.35.
This article incorporates text available under the CC BY-SA 4.0 license.
- ^ a b c d e f "HD 18438". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 September 2024.
- ^ a b c "HD 18438 Overview". NASA Exoplanet Archive. Retrieved 31 October 2023.
- ^ a b Bang, Tae-Yang; et al. (28 February 2018). "SEARCH FOR EXOPLANETS AROUND NORTHERN CIRCUMPOLAR STARS III. LONG-PERIOD RADIAL VELOCITY VARIATIONS IN HD 18438 AND HD 158996". Journal of the Korean Astronomical Society. 51 (1): 17–25. arXiv:1803.07213. Bibcode:2018JKAS...51...17B. doi:10.5303/JKAS.2018.51.1.17.
- ^ Stassun, Keivan G.; et al. (1 October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256.
- ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 4 June 2023. Retrieved 31 October 2023.
- ^ "Working Group on Extrasolar Planets: Definition of a "Planet"". IAU position statement. 28 February 2003. Archived from the original on 16 December 2014. Retrieved 28 April 2014.
- ^ "Exoplanet Criteria for Inclusion in the Archive". NASA Exoplanet Archive.
