A planetary collision afterglow and transit of the resultant debris cloud Article Swipe
Matthew A. Kenworthy
,
Simon J. Lock
,
Grant M. Kennedy
,
Richelle van Capelleveen
,
Eric E. Mamajek
,
L. Carone
,
Franz-Josef Hambsch
,
J. Masiero
,
Amy Mainzer
,
J. Davy Kirkpatrick
,
Edward Gomez
,
Z. M. Leinhardt
,
Jingyao Dou
,
Pavan Tanna
,
Arttu Sainio
,
Hamish Barker
,
S. Charbonnel
,
O. Garde
,
Pascal Le Dû
,
Lionel Mulato
,
Thomas Petit
,
Michael Rizzo Smith
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2310.08360
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2310.08360
Planets grow in rotating disks of dust and gas around forming stars, some of which can subsequently collide in giant impacts after the gas component is removed from the disk. Monitoring programs with the warm Spitzer mission have recorded significant and rapid changes in mid-infrared output for several stars, interpreted as variations in the surface area of warm dusty material ejected by planetary-scale collisions and heated by the central star: e.g., NGC 2354-ID8, HD 166191 and V844 Persei. Here we report combined observations of the young (about 300 Myr), solar-like star ASASSN-21qj: an infrared brightening consistent with a blackbody temperature of 1000 K and a luminosity of 4 percent of that of the star lasting for about 1000 days, partially overlapping in time with a complex and deep wavelength-dependent optical eclipse that lasted for about 500 days. The optical eclipse started 2.5 years after the infrared brightening, implying an orbital period of at least that duration. These observations are consistent with a collision between two exoplanets of several to tens of Earth masses at 2 to 16 au from the central star. Such an impact produces a hot, highly-extended post-impact remnant with sufficient luminosity to explain the infrared observations. Transit of the impact debris, sheared by orbital motion into a long cloud, causes the subsequent complex eclipse of the host star.
Related Topics
Concepts
Metadata
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2310.08360
- https://arxiv.org/pdf/2310.08360
- OA Status
- green
- Related Works
- 10
- OpenAlex ID
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All OpenAlex metadata
Raw OpenAlex JSON
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- DOI
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https://doi.org/10.48550/arxiv.2310.08360Digital Object Identifier
- Title
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A planetary collision afterglow and transit of the resultant debris cloudWork title
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2023Year of publication
- Publication date
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2023-10-12Full publication date if available
- Authors
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Matthew A. Kenworthy, Simon J. Lock, Grant M. Kennedy, Richelle van Capelleveen, Eric E. Mamajek, L. Carone, Franz-Josef Hambsch, J. Masiero, Amy Mainzer, J. Davy Kirkpatrick, Edward Gomez, Z. M. Leinhardt, Jingyao Dou, Pavan Tanna, Arttu Sainio, Hamish Barker, S. Charbonnel, O. Garde, Pascal Le Dû, Lionel Mulato, Thomas Petit, Michael Rizzo SmithList of authors in order
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https://arxiv.org/abs/2310.08360Publisher landing page
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https://arxiv.org/pdf/2310.08360Direct link to full text PDF
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YesWhether a free full text is available
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greenOpen access status per OpenAlex
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https://arxiv.org/pdf/2310.08360Direct OA link when available
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Physics, Astrophysics, Exoplanet, Astronomy, Luminosity, Eclipse, Transit (satellite), Stars, Planet, Planetary system, Debris disk, Infrared, Galaxy, Law, Public transport, Political scienceTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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10Other works algorithmically related by OpenAlex
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