NGTS-12b: A sub-Saturn mass transiting exoplanet in a 7.53 day orbit

Author:

Bryant Edward M12,Bayliss Daniel12ORCID,Nielsen Louise D3ORCID,Veras Dimitri12ORCID,Acton Jack S4,Anderson David R12ORCID,Armstrong David J12ORCID,Bouchy François3,Briegal Joshua T5,Burleigh Matthew R4,Cabrera Juan6,Casewell Sarah L4,Chaushev Alexander7,Cooke Benjamin F12ORCID,Csizmadia Szilárd6ORCID,Eigmüller Philipp6,Erikson Anders6,Gill Samuel12,Gillen Edward85ORCID,Goad Michael R4,Grieves Nolan3,Günther Maximilian N9,Henderson Beth4,Hogan Aleisha4,Jenkins James S1011ORCID,Lendl Monika3ORCID,McCormac James12,Moyano Maximiliano12,Queloz Didier5,Rauer Heike67,Raynard Liam4,Smith Alexis M S6,Tilbrook Rosanna H4,Udry Stéphane3,Vines Jose I10ORCID,Watson Christopher A13,West Richard G12ORCID,Wheatley Peter J12ORCID

Affiliation:

1. Department of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK

2. Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK

3. Observatoire de Genève, Université de Genève, Chemin des Maillettes 51, CH-1290 Sauverny, Switzerland

4. School of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH, UK

5. Astrophysics Group, Cavendish Laboratory, J.J. Thomson Avenue, Cambridge CB3 0HE, UK

6. Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, D-12489 Berlin, Germany

7. Center for Astronomy and Astrophysics, TU Berlin, Hardenbergstr 36, D-10623 Berlin, Germany

8. Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK

9. Department of Physics, Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA

10. Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile

11. Centro de Astrofísica y Tecnologías Afines (CATA), Casilla 36-D, Santiago, Chile

12. Instituto de Astronomía, Universidad Católica del Norte, Casa Central, Angamos 0610, Antofagasta 1270709, Chile

13. Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, UK

Abstract

ABSTRACT We report the discovery of the transiting exoplanet NGTS-12b by the Next Generation Transit Survey (NGTS). The host star, NGTS-12, is a V = 12.38 mag star with an effective temperature of Teff = 5690 ± 130 K. NGTS-12b orbits with a period of P = 7.53 d, making it the longest period planet discovered to date by the main NGTS survey. We verify the NGTS transit signal with data extracted from the Transiting Exoplanet Survey Satellite (TESS) full-frame images, and combining the photometry with radial velocity measurements from HARPS and FEROS we determine NGTS-12b to have a mass of 0.208 ± 0.022 MJ and a radius of 1.048 ± 0.032 RJ. NGTS-12b sits on the edge of the Neptunian desert when we take the stellar properties into account, highlighting the importance of considering both the planet and star when studying the desert. The long period of NGTS-12b combined with its low density of just 0.223 ± 0.029 g cm−3 make it an attractive target for atmospheric characterization through transmission spectroscopy with a Transmission Spectroscopy Metric of 89.4.

Funder

European Southern Observatory

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data;The Astronomical Journal;2024-04-24

2. TESS duotransit candidates from the Southern Ecliptic Hemisphere;Monthly Notices of the Royal Astronomical Society;2024-01-23

3. TOI-3785 b: A Low-density Neptune Orbiting an M2-dwarf Star;The Astronomical Journal;2023-07-04

4. NGTS-21b: an inflated Super-Jupiter orbiting a metal-poor K dwarf;Monthly Notices of the Royal Astronomical Society;2022-10-07

5. High precision ground-based CCD photometry from the Next Generation Transit Survey;X-Ray, Optical, and Infrared Detectors for Astronomy X;2022-08-29

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3