 Artist's impression of the IRAS 04125+2902 system. | |
| Discovery | |
|---|---|
| Discovered by | Madyson Barber et al. |
| Discovery date | November 20, 2024 |
| Detection method | Transit |
| Designations | |
| Alternative names | TIDYE-1b |
| Orbital characteristics | |
| Semi-major axis | 0.077+0.0069 −0.0100 AU |
| Orbital period (sidereal) | 8.834978(28) days |
| Inclination | 88.3°+1.2° −1.6° |
| Star | IRAS 04125+2902 |
| Physical characteristics | |
| Mean radius | 0.958+0.077 −0.075 RJ |
| Mass | <90 M🜨 (<0.3 MJ) |
| Temperature | 854+59 −32 K |
IRAS 04125+2902 b (TIDYE-1 b) is an extrasolar planet orbiting a young protostar. It is the youngest transiting exoplanet so far discovered, with an age of just three million years.
Characteristics
The planet has a mass less than 0.3 Jupiter masses (90 Earth masses) and a radius nearly equal to that of Jupiter, just 4% smaller, or the same as 10.7 Earth radii. It is still enshrouded in an hydrogen envelope, and will shed its outer layers during its evolution, becoming either a sub-Neptune, super-Earth or a sub-Saturn. The radius would shrink to 1.5–4 R🜨 if the planet becomes a super-Neptune or to 4–7 R🜨 if it becomes a sub-Saturn. The planet likely has an extended atmoshpere due to its large radius and relatively low mass, making it a potential candidate for follow-up observations with the James Webb Space Telescope.
It has a compact orbit around its host star, completing an orbit every just 8.8 days, and semi-major axis (mean separation from the star) is just 8% of the Earth-Sun distance (astronomical unit). Its short orbit and high mass mean that it likely formed at a larger distance and then migrated to inner regions, as regions so close to the host star don't have sufficient mass to form large planets.
With an age of just three million years, IRAS 04125+2902 b is the youngest transiting exoplanet so far discovered, and also one of the youngest exoplanets, only a couple of younger <13 MJ objects are listed in the NASA Exoplanet Archive.
Discovery
IRAS 04125+2902 b was detected using the transit method, which consists of observing small, regular dips in the brightness of the host star. These dips are planetary transits and happen when the planet passes through its host star as viewed from an observer. Data from the Transiting Exoplanet Survey Satellite was analysed by the astronomer Madyson Barber and colleagues, allowing the planet detection. After rulling out alternative explanations for the observed transit, the team was able to confirm its existence. Its discovery and confirmation was published on November 20, 2024, in the journal Nature.
The planet has also the nickname TIDYE-1 b, derived from the TESS Investigation – Demographics of Young Exoplanets (TIDYE) project.
Host star
Main article: IRAS 04125+2902The host star of IRAS 04125+2902 b is IRAS 04125+2902, a T Tauri variable located at 520 light-years from Earth. It has cool effective temperature and a spectral type M1.25±0.25. Despite its cool temperature and late spectral type, this star is larger than the Sun, mostly because of its young age. IRAS 04125+2902 has a transitional disk located at 20–60 AU and makes a binary system with 2MASS J04154269+2909558, being separated by a projected distance of 635 astronomical units (9.50×10 km) from its companion.
The companions and the host star's equator are aligned, but the disk is not, and the reason for the misalignment of the disk is unclear. It could be due to planetary migration in the past which misaligned the orbit of IRAS 04125+2902 b's orbit, but such an hypothesis requires the existence of another planet in the system, which has not been detected. Another hypothesis suggest that infalling material from the surrounding Taurus Molecular Cloud could be the cause of this misalignment, as those places are densely packed.
See also
- V830 Tauri – Similar to IRAS 04125+2902 and has an unconfirmed planet
- K2-33b, previously the youngest transiting exoplanet
- DH Tauri b, youngest known exoplanet at 700,000 years
References
- ^ Barber, Madyson G.; Mann, Andrew W.; Vanderburg, Andrew; Krolikowski, Daniel; Kraus, Adam; Ansdell, Megan; Pearce, Logan; Mace, Gregory N.; Andrews, Sean M.; Boyle, Andrew W.; Collins, Karen A.; De Furio, Matthew; Dragomir, Diana; Espaillat, Catherine; Feinstein, Adina D. (November 2024). "A giant planet transiting a 3-Myr protostar with a misaligned disk". Nature. 635 (8039): 574–577. arXiv:2411.18683. Bibcode:2024Natur.635..574B. doi:10.1038/s41586-024-08123-3. ISSN 1476-4687. PMID 39567788.
- ^ Wenz, John (2024-11-20). "Young, shrouded super-Neptune could help teach us how such worlds form". Astronomy Magazine. Retrieved 2024-11-20.
- "NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 2024-11-20.
- ^ "Discovery Alert: A Rare Glimpse of a Newborn Planet - NASA Science". science.nasa.gov. Retrieved 2024-11-20.
- "IRAS 04125+2902". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Espaillat, C.; Andrews, S.; Powell, D.; Feldman, D.; Qi, C.; Wilner, D.; D’Alessio, P. (2015-07-09). "The Transitional Disk Around Iras 04125+2902". The Astrophysical Journal. 807 (2): 156. arXiv:1506.01007. Bibcode:2015ApJ...807..156E. doi:10.1088/0004-637x/807/2/156. ISSN 1538-4357.
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