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Molecular Gas Clumps from the Destruction of Icy Bodies in the β Pictoris Debris Disk

2014/03/07 by W. R. F. Dent, M. C. Wyatt, Aki Roberge +21 · 6 citations
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Atomic and Molecular Physics #astro-ph.SR

paper · pdf · doi:10.1126/science.1248726

published as Science (2014) 343, 1490

openalex publication_date 2014/03/07 · arxiv created 2014/04/04 · arxiv updated 2015/06/19 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Many stars are surrounded by disks of dusty debris formed in the collisions of asteroids, comets and dwarf planets. But is gas also released in such events? Observations at submm wavelengths of the archetypal debris disk around β Pictoris show that 0.3% of a Moon mass of carbon monoxide orbits in its debris belt. The gas distribution is highly asymmetric, with 30% found in a single clump 85AU from the star, in a plane closely aligned with the orbit of the inner planet, β Pic b. This gas clump delineates a region of enhanced collisions, either from a mean motion resonance with an unseen giant planet, or from the remnants of a collision of Mars-mass planets.

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