NASA’s Transiting Exoplanet Survey Satellite (TESS) is conducting a survey of about 200,000 of the brightest stars near the sun with the aim of searching for transiting exoplanets. So far, it has identified nearly 2,700 candidate exoplanets (TESS Objects of Interest, or TOI), of which 125 have been confirmed so far. TOI-269 (also known as TIC 220479565) is an M dwarf located some 186 light years away from the Earth. It has a spectral type of M2V, radius of about 0.4 solar radii and mass of approximately 0.39 solar masses. The star’s effective temperature is estimated to be some 3,500 K, while its metallicity is at a level of around -0.29.
TOI-269 was observed by the TESS spacecraft between September 2018 and July 2019, which resulted in the identification of a transit signal in its light curve. Now, using various ground-based telescopes, including the Exoplanets in Transits and their Atmospheres (ExTrA) facility at La Silla Observatory in Chile, a group of astronomers led by Marion Cointepas has confirmed the planetary nature of this signal. “We surmise TOI-269 b may have acquired its high eccentricity as it migrated inward through planet-planet interactions,” the astronomers wrote in the study.
What is interesting is that TOI-269 b has an unusually high orbital eccentricity—approximately 0.425. This is one of the highest eccentricities among the known extrasolar planets with periods below 10 days and suggests that the object may have recently arrived in its position. Moreover, the density of TOI-269 b, calculated to be some 2.28 g/cm3, is significantly lower than the typical density of rock planets and indicates the presence of a volatile envelope. Such low density and its other properties make it an interesting target for atmospheric characterization in order to compare it with other sub-Neptunes. In particular, the authors of the paper propose to probe the atmosphere of TOI-269 b with transmission spectroscopy to shed more light on its composition.
The newly detected alien world has a radius of about 2.77 Earth radii, is 8.8 times more massive than our planet and orbits its host every 3.7 days. The observations show that TOI-269 b is separated by around 0.0345 AU from the parent star and its equilibrium temperature is most likely at a level of 530 K. “We present the confirmation of a new sub-Neptune close to the transition between super-Earths and sub-Neptunes transiting the M2 dwarf TOI-269,” the researchers wrote in the paper.
TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA, arXiv:2104.14782 arxiv.org/abs/2104.14782 THYME project discovers a sub-Neptune exoplanet orbiting young star
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.
© 2021 Science X Network
New sub-Neptune exoplanet discovered by astronomers (2021, May 10)
retrieved 11 May 2021
News Highlights Space
- Headline: New subneptune exoplanet discovered by astronomers
- Check all news and articles from the Space news information updates.