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Necroplanetology : simulating the tidal disruption of differentiated planetary material orbiting WD 1145+017
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Duvvuri, Girish M., Redfield, Seth and Veras, Dimitri (2020) Necroplanetology : simulating the tidal disruption of differentiated planetary material orbiting WD 1145+017. The Astrophysical Journal, 893 (2). 166. doi:10.3847/1538-4357/ab7fa0
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WRAP-necroplanetology-simulating-tidal-disruption-differentiated-planetary-material-orbiting-WD-1145+017-Veras-2020.pdf - Accepted Version - Requires a PDF viewer. Download (1060Kb) | Preview |
Official URL: http://dx.doi.org/10.3847/1538-4357/ab7fa0
Abstract
The WD 1145+017 system shows irregular transit features that are consistent with the tidal disruption of differentiated asteroids with bulk densities $\lt 4\,{\rm{g}}\,{\mathrm{cm}}^{-3}$ and bulk masses $\lesssim {10}^{21}\,\mathrm{kg}$. We use the open-source N-body code REBOUND to simulate this disruption with different internal structures: varying the core volume fraction, mantle/core density ratio, and the presence/absence of a thin low-density crust. We allow the rubble pile to partially disrupt and capture lightcurves at a specific point during the disruption at cadences comparable to those from ground-based photometry. As a proof-of-concept we show that varying these structural parameters have observationally distinguishable effects on the transit lightcurve as the asteroid is disrupted and compare the simulation-generated lightcurves to data from Gary et al. With the caveat that our simulations do not model the sublimation in detail or account for its effects on orbital evolution, we find that a low core fraction and low mantle/core density ratio asteroid is most consistent with the stable transit feature present for multiple weeks circa 2016 April (referred to as G6121 in Gary et al. and A1 in Hallakoun et al.). Connecting tidal disruption simulations to photometry suggests characteristics for the interior structure and composition of an exoplanetary body, information that is only possible because we are observing the death of the planetary system in action. All-sky survey missions such as TESS and LSST will be able to detect other systems like WD 1145+017, creating a sample of subjects for a new subfield of planetary science: necroplanetology.
| Item Type: | Journal Article | ||||||||||||
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| Subjects: | Q Science > QB Astronomy | ||||||||||||
| Divisions: | Faculty of Science, Engineering and Medicine > Science > Physics | ||||||||||||
| Library of Congress Subject Headings (LCSH): | Extrasolar planets, White dwarf stars, Solar system, Astrophysics, Planetary science | ||||||||||||
| Journal or Publication Title: | The Astrophysical Journal | ||||||||||||
| Publisher: | Institute of Physics Publishing, Inc. | ||||||||||||
| ISSN: | 0004-637X | ||||||||||||
| Official Date: | 28 April 2020 | ||||||||||||
| Dates: |
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| Volume: | 893 | ||||||||||||
| Number: | 2 | ||||||||||||
| Article Number: | 166 | ||||||||||||
| DOI: | 10.3847/1538-4357/ab7fa0 | ||||||||||||
| Status: | Peer Reviewed | ||||||||||||
| Publication Status: | Published | ||||||||||||
| Reuse Statement (publisher, data, author rights): | © 2020. The American Astronomical Society. | ||||||||||||
| Access rights to Published version: | Restricted or Subscription Access | ||||||||||||
| RIOXX Funder/Project Grant: |
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