Abundant hydrocarbons in the disk around a very-low-mass star

M. Arabhavi, Aditya; Kamp, I.; Henning, Th.; F. van Dishoeck, E.; Christiaens, Valentin; Gasman, Danny; Perrin, A.; Güdel, M.; Tabone, Benoît; S. Kanwar, J.; B. F. M. Waters, L.; Pascucci, Ilaria; Samland, M.; Perotti, Giulia; Bettoni, Giulio; L. Grant, Sierra; Lagage, Pierre-Olivier; P. Ray, T.; Vandenbussche, B.; Absil, Olivier; Argyriou, Ioannis; Barrado, D.; Boccaletti, A.; Bouwman, J.; Caratti o Garatti, A.; M. Glauser, Adrian; Lahuis, F.; Mueller, Michael; Olofsson, G.; Pantin, E.; Scheithauer, Silvia; Morales‐Calderón, M.; Franceschi, Riccardo; Jang, Hyerin; Pawellek, Nicole; Rodgers-Lee, Donna; Schreiber, J.; R. Schwarz, Kamber; Temmink, Milou; Vlasblom, Marissa; Wright, Gillian; Colina, L.; Östlin, Göran

doi:10.1126/science.adi8147

Public

Abundant hydrocarbons in the disk around a very-low-mass star

Published in Science • Jun 6, 2024

Authors:

Aditya M. Arabhavi

I. Kamp

Th. Henning

Abstract

Very-low-mass stars (those less than 0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars. The compositions of those planets are largely unknown but are expected to relate to the protoplanetary disk in which they form. We used James Webb Space Telescope mid-i...

Subject

Planet

Protoplanetary disk

Debris disk

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