• LOGIN
    Login with username and password
Repository logo

BORIS Portal

Bern Open Repository and Information System

  • Publications
  • Theses
  • Research Data
  • Projects
  • Organizations
  • Researchers
  • More
  • Collections
  • Statistics
  • LOGIN
    Login with username and password
Repository logo
Unibern.ch
  1. Home
  2. Publications
  3. Stellar Parameters for Trappist-1

Stellar Parameters for Trappist-1

Details
Files
DOI
10.7892/boris.126867
Publisher DOI
10.3847/1538-4357/aaa023
Abstract
TRAPPIST-1 is an ultracool dwarf star transited by seven Earth-sized planets, for which thorough characterization of atmospheric properties, surface conditions encompassing habitability, and internal compositions is possible with current and next-generation telescopes. Accurate modeling of the star is essential to achieve this goal. We aim to obtain updated stellar parameters for TRAPPIST-1 based on new measurements and evolutionary models, compared to those used in discovery studies. We present a new measurement for the parallax of TRAPPIST-1, 82.4 ± 0.8 mas, based on 188 epochs of observations with the TRAPPIST and Liverpool Telescopes from 2013 to 2016. This revised parallax yields an updated luminosity of L ͙=(5.22 ± 0.19) x 10⁻⁴ Lʘ, which is very close to the previous estimate but almost two times more precise. We next present an updated estimate for TRAPPIST-1 stellar mass, based on two approaches: mass from stellar evolution modeling, and empirical mass derived from dynamical masses of equivalently classified ultracool dwarfs in astrometric binaries. We combine them using a Monte-Carlo approach to derive a semi-empirical estimate for the mass of TRAPPIST-1. We also derive estimate for the radius by combining this mass with stellar density inferred from transits, as well as an estimate for the effective temperature from our revised luminosity and radius. Our final results are M ͙= 0.089 ± 0.006 Mʘ, R ͙ =0.121 ± 0.003 Rʘ , and Teff= 2516 ± 41 K. Considering the degree to which the TRAPPIST-1 system will be scrutinized in coming years, these revised and more precise stellar parameters should be considered when assessing the properties of TRAPPIST-1 planets.
Date Issued
2018-01
Publication Type
Article
Subject(s)
500 Science
500 Science > 520 Astronomy
500 Science > 530 Physics
Language(s)
en
Author(s)
Grootel, Valérie Van
Fernandes, Catarina S.
Gillon, Michael
Jehin, Emmanuel
Manfroid, Jean
Scuflaire, Richard
Burgasser, Adam J.
Barkaoui, Khalid
Benkhaldoun, Zouhair
Burdanov, Artem
Delrez, Laetitia
Demory, Brice-Olivier Denys  
Center for Space and Habitability (CSH)  
Wit, Julien de
Queloz, Didier
Triaud, Amaury H. M. J.
Additional Credits
Center for Space and Habitability (CSH)  
Journal
Astrophysical journal
Publisher
Institute of Physics Publishing IOP
ISSN
0004-637X
Access(Rights)
open.access
Show full item
BORIS Portal
Bern Open Repository and Information System
Build: 0eaa7c [ 7.08. 11:06]
Explore
  • Projects
  • Funding
  • Publications
  • Research Data
  • Organizations
  • Researchers
  • Audiovisual Material
  • Software & other digital items
  • Events
More
  • About BORIS Portal
  • BORIS Portal & Open Science
  • Send Feedback
  • Cookie settings
  • Service Policy
Follow us on
  • Mastodon
  • YouTube
  • LinkedIn
UniBe logo
Repository logo COAR Notify