NGTS-10b: the shortest period hot Jupiter yet discovered

Smalley, Barry

Abstract

We report the discovery of a new ultrashort period (USP) transiting hot Jupiter from the Next Generation Transit Survey (NGTS). NGTS-10b has a mass and radius of 2.162+0.092-0.107?MJ and 1.205+0.117-0.083?RJ and orbits its host star with a period of 0.7668944 ± 0.0000003?d, making it the shortest period hot Jupiter yet discovered. The host is a 10.4 ± 2.5?Gyr old K5V star (Teff = 4400 ± 100?K) of Solar metallicity ([Fe/H] = -0.02 ± 0.12?dex) showing moderate signs of stellar activity. NGTS-10b joins a short list of USP Jupiters that are prime candidates for the study of star–planet tidal interactions. NGTS-10b orbits its host at just 1.46 ± 0.18 Roche radii, and we calculate a median remaining inspiral time of 38?Myr and a potentially measurable orbital period decay of 7 s over the coming decade, assuming a stellar tidal quality factor Q's =2 × 107.

Citation

Smalley, B., McCormac, J., Gillen, E., Jackman, J. A. G., Brown, D. J. A., Bayliss, D., Wheatley, P. J., Anderson, D. R., Armstrong, D. J., Bouchy, F., Briegal, J. T., Burleigh, M. R., Cabrera, J., Casewell, S. L., Chaushev, A., Chazelas, B., Chote, P., Cooke, B. F., Costes, J. C., Csizmadia, S., …West, R. G. (2020). NGTS-10b: the shortest period hot Jupiter yet discovered. Monthly Notices of the Royal Astronomical Society, 493(1), 126-140. https://doi.org/10.1093/mnras/staa115

• Journal Article Type: Article
• Acceptance Date: Jan 10, 2020
• Publication Date: Mar 1, 2020
• Publicly Available Date: May 26, 2023
• Journal: Monthly Notices of the Royal Astronomical Society
• Print ISSN: 0035-8711
• Electronic ISSN: 1365-2966
• Publisher: Oxford University Press
• Volume: 493
• Issue: 1
• Pages: 126-140
• DOI: https://doi.org/10.1093/mnras/staa115
• Keywords: techniques: photometric; stars: individual: NGTS-10; planetary systems
• Public URL: https://keele-repository.worktribe.com/output/414684
• Publisher URL: http://dx.doi.org/10.1093/mnras/staa115