ORTIS Design and development report

Authors:

PG Irwin, B Ellison, S Calcutt

Planet Hunters TESS III: two transiting planets around the bright G dwarf HD 152843

Authors:

Nora L Eisner, Belinda A Nicholson, Oscar Barragán, Suzanne Aigrain, Chris Lintott, Laurel Kaye, Baptiste Klein, Grant Miller, Jake Taylor, Norbert Zicher, Lars A Buchhave, Douglas A Caldwell, Jonti Horner, Joe Llama, Annelies Mortier, Vinesh M Rajpaul, Keivan Stassun, Avi Sporer, Andrew Tkachenko, Jon M Jenkins, David W Latham, George R Ricker, Sara Seager, Joshua N Winn, Safaa Alhassan, Elisabeth ML Baeten, Stewart J Bean, David M Bundy, Vitaly Efremov, Richard Ferstenou, Brian L Goodwin, Michelle Hof, Tony Hoffman, Alexander Hubert, Lily Lau, Sam Lee, David Maetschke, Klaus Peltsch, Cesar Rubio-Alfaro, Gary M Wilson

Abstract:

We report on the discovery and validation of a two-planet system around a bright (V = 8.85 mag) early G dwarf (1.43 $R_{\odot}$, 1.15 $M_{\odot}$, TOI 2319) using data from NASA's Transiting Exoplanet Survey Satellite (TESS). Three transit events from two planets were detected by citizen scientists in the month-long TESS light curve (sector 25), as part of the Planet Hunters TESS project. Modelling of the transits yields an orbital period of \Pb\ and radius of $3.41 _{ - 0.12 } ^ { + 0.14 }$ $R_{\oplus}$ for the inner planet, and a period in the range 19.26-35 days and a radius of $5.83 _{ - 0.14 } ^ { + 0.14 }$ $R_{\oplus}$ for the outer planet, which was only seen to transit once. Each signal was independently statistically validated, taking into consideration the TESS light curve as well as the ground-based spectroscopic follow-up observations. Radial velocities from HARPS-N and EXPRES yield a tentative detection of planet b, whose mass we estimate to be $11.56 _{ - 6.14 } ^ { + 6.58 }$ $M_{\oplus}$, and allow us to place an upper limit of $27.5$ $M_{\oplus}$ (99 per cent confidence) on the mass of planet c. Due to the brightness of the host star and the strong likelihood of an extended H/He atmosphere on both planets, this system offers excellent prospects for atmospheric characterisation and comparative planetology.

Preliminary report on sub-millimetre spectra of Jupiter and Saturn.

Seasonal changes in the vertical structure of ozone in the Martian lower atmosphere and its relationship to water vapour

Authors:

Kevin Olsen, Anna Fedorova, Alexander Trokhimovskiy, Franck Montmessin, Franck Lefèvre, Oleg Korablev, Lucio Baggio, Francois Forget, Ehouarn Millour, Antoine Bierjon, Juan Alday, Colin Wilson, Patrick Irwin, Denis Belyaev, Andrey Patrakeev, Alexey Shakun

Second report on sub-millimetre spectra of Jupiter, Saturn and Titan.