Extreme Debris Disk Variability: Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation
AuthorSu, Kate Y. L.
Jackson, Alan P.
Rieke, George H.
Kennedy, G. M.
Leinhardt, Zoë M.
Meng, Huan Y. A.
Rodriguez, Joseph E.
Reichart, D. E.
Stassun, Keivan G.
AffiliationUniv Arizona, Steward Observ
Univ Arizona, Lunar & Planetary Lab
infrared: planetary systems
planets and satellites: dynamical evolution and stability
stars: individual (2MASS J08090250-4858172, 2MASS J07354269-1450422)
MetadataShow full item record
PublisherIOP PUBLISHING LTD
CitationKate Y. L. Su et al 2019 AJ 157 202
RightsCopyright © 2019. The American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Collection InformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at email@example.com.
AbstractThe most dramatic phases of terrestrial planet formation are thought to be oligarchic and chaotic growth, on timescales of up to 100-200 Myr, when violent impacts occur between large planetesimals of sizes up to protoplanets. Such events are marked by the production of large amounts of debris, as has been observed in some exceptionally bright and young debris disks (termed extreme debris disks). Here we report five years of Spitzer measurements of such systems around two young solar-type stars: ID8 and P1121. The short-term (weekly to monthly) and long-term (yearly) disk variability is consistent with the aftermaths of large impacts involving large asteroid-sized bodies. We demonstrate that an impact-produced clump of optically thick dust, under the influence of the dynamical and viewing geometry effects, can produce short-term modulation in the disk light curves. The long-term disk flux variation is related to the collisional evolution within the impact-produced fragments once released into a circumstellar orbit. The time-variable behavior observed in the P1121 system is consistent with a hypervelocity impact prior to 2012 that produced vapor condensates as the dominant impact product. Two distinct short-term modulations in the ID8 system suggest two violent impacts at different times and locations. Its long-term variation is consistent with the collisional evolution of two different populations of impact-produced debris dominated by either vapor condensates or escaping boulders. The bright, variable emission from the dust produced in large impacts from extreme debris disks provides a unique opportunity to study violent events during the era of terrestrial planet formation.
NoteOpen Access Journal
VersionFinal published version
SponsorsNASA's ADAP program [NNX17AF03G]; Royal Society; NASA Exoplanets Research Program [80NSSC18K0397]; National Aeronautics and Space Administration