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相关论文: Stellar parameters for TRAPPIST-1

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TRAPPIST-1 hosts seven Earth-sized planets transiting an M8 star. We observed mid-transit times of each of the inner two planets with the Astrophysical Research Consortium (ARC) 3.5 m Telescope at Apache Point Observatory (APO) to help…

地球与行星天体物理 · 物理学 2018-01-16 Brett M. Morris , Eric Agol , Suzanne L. Hawley

TRAPPIST-1 is an 0.09 $M_{\odot}$ star, which harbours a system of seven Earth-sized planets. Two main features stand out: (i) all planets have similar radii, masses, and compositions; and (ii) all planets are in resonance. Previous works…

地球与行星天体物理 · 物理学 2022-02-16 Shuo Huang , Chris W. Ormel

As the first and till date the only one multiple planet hosting dwarf star that is sufficiently cool to form condensate cloud in it atmosphere, Trappist-1 provides unique opportunity to test the efficiency of image polarimetry as a tool to…

地球与行星天体物理 · 物理学 2018-07-18 Sujan Sengupta

The nearby TRAPPIST-1 system, with its seven small rocky planets orbiting a late-type M8 star, offers an unprecedented opportunity to search for secondary atmospheres on temperate terrestrial worlds. In particular, the 0.8 Earth-radii…

The recent discovery of seven potentially habitable Earth-size planets around the ultra-cool star TRAPPIST-1 has further fueled the hunt for extraterrestrial life. Current methods focus on closely monitoring the host star to look for…

科普物理 · 物理学 2017-04-03 M. Turbo-King , B. R. Tang , Z. Habeertable , M. C. Chouffe , B. Exquisit , L. Keg-beer

The seven approximately Earth-sized transiting planets in the \object{TRAPPIST-1} system provide a unique opportunity to explore habitable zone and non-habitable zone small planets within the same system. Its habitable zone exoplanets --…

地球与行星天体物理 · 物理学 2018-10-17 Zhanbo Zhang , Yifan Zhou , Benjamin V. Rackham , Daniel Apai

As more exoplanets are being discovered around ultracool dwarfs, understanding their magnetic activity -- and the implications for habitability -- is of prime importance. To find stellar flares and photometric signatures related to…

太阳与恒星天体物理 · 物理学 2021-06-30 Bálint Seli , Krisztián Vida , Attila Moór , András Pál , Katalin Oláh

TRAPPIST-1 is an M8 dwarf hosting seven known exoplanets and is currently one of the most frequently observed targets of the James Webb Space Telescope (JWST). However, it is notoriously active, and its surface is believed to be covered by…

The first nearby very-low mass star planet-host discovered, TRAPPIST-1, presents not only a unique opportunity for studying a system of multiple terrestrial planets, but a means to probe magnetospheric interactions between a star at the end…

太阳与恒星天体物理 · 物理学 2018-10-31 J. Sebastian Pineda , Gregg Hallinan

The TRAPPIST-1 planetary system is an excellent candidate for study of the evolution and habitability of M-dwarf planets. Transmission spectroscopy observations performed with the Hubble Space Telescope (HST) suggest the innermost five…

地球与行星天体物理 · 物理学 2018-11-28 Sarah E. Moran , Sarah M. Hörst , Natasha E. Batalha , Nikole K. Lewis , Hannah R. Wakeford

TRAPPIST-1 (Gillon et al. 2017) is an extremely compact planetary system: seven earth-sized planets orbit at distances lower than 0.07 AU around one of the smallest M-dwarf known in the close neighborhood of the Sun (with a mass of less…

地球与行星天体物理 · 物理学 2018-10-29 Sylvain Breton , Emeline Bolmont , Gabriel Tobie , Stéphane Mathis

The TRAPPIST-1 system offers the opportunity to characterize terrestrial, potentially habitable planets orbiting a nearby ultracool dwarf star. We performed a four-orbit reconnaissance with the Space Telescope Imaging Spectrograph onboard…

地球与行星天体物理 · 物理学 2017-02-24 V. Bourrier , D. Ehrenreich , P. J. Wheatley , E. Bolmont , M. Gillon , J. de Wit , A. J. Burgasser , E. Jehin , D. Queloz , A. H. M. J. Triaud

TRAPPIST-1 is a late M-dwarf orbited by seven Earth-sized planets with orbital period ratios near a chain of mean motion resonances. Due to uncertain system parameters, most orbital configurations drawn from the inferred posterior…

地球与行星天体物理 · 物理学 2017-05-24 Daniel Tamayo , Hanno Rein , Cristobal Petrovich , Norman Murray

The Rossiter-McLaughlin effect is the principal method of determining the sky-projected spin--orbit angle ($\beta$) of transiting planets. Taking the example of the recently discovered TRAPPIST-1 system, we explore how ultracool dwarfs…

地球与行星天体物理 · 物理学 2016-08-17 Ryan Cloutier , Amaury H. M. J Triaud

The upcoming launch of the James Webb Space Telescope (JWST) combined with the unique features of the TRAPPIST-1 planetary system should enable the young field of exoplanetology to enter into the realm of temperate Earth-sized worlds.…

The TRAPPIST-1 system provides an exquisite laboratory for understanding exoplanetary atmospheres and interiors. Their mutual gravitational interactions leads to transit timing variations, from which Grimm et al. (2018) recently measured…

地球与行星天体物理 · 物理学 2018-05-01 Gabrielle Suissa , David Kipping

Small exoplanets of nearby M dwarf stars present the possibility to find and characterize habitable worlds within the next decade. TRAPPIST-1, an ultracool M dwarf star, was recently found to have seven Earth-sized planets of predominantly…

地球与行星天体物理 · 物理学 2020-01-29 Renyu Hu , Luke Peterson , Eric T. Wolf

The recent discovery of three Earth-sized, potentially habitable planets around a nearby cool star, TRAPPIST-1, has provided three key targets for the upcoming James Webb Space Telescope (JWST). Depending on their atmospheric…

地球与行星天体物理 · 物理学 2016-06-08 Joanna K. Barstow , Patrick G. J. Irwin

Nine transiting Earth-sized planets have recently been discovered around nearby late M dwarfs, including the TRAPPIST-1 planets and two planets discovered by the MEarth survey, GJ 1132b and LHS 1140b. These planets are the smallest known…

地球与行星天体物理 · 物理学 2017-12-06 Caroline V. Morley , Laura Kreidberg , Zafar Rustamkulov , Tyler Robinson , Jonathan J. Fortney

One of the most promising avenues for the detailed study of temperate Earth-sized exoplanets is the detection of such planets in transit in front of stars small and nearby enough to make possible their thorough atmospheric characterisation…