Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563

We present the discovery of deep but sporadic transits in the flux of SBSS 1232+563, a metal-rich white dwarf polluted by disrupted exoplanetary debris. Nearly 25 yr of photometry from multiple sky surveys reveal evidence of occasional dimming of the white dwarf, most notably evident in an 8 month l...

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Main Authors: J. J. Hermes, Joseph A. Guidry, Zachary P. Vanderbosch, Mariona Badenas-Agusti, Siyi Xu, Malia L. Kao, Antonio C. Rodriguez, Keith Hawkins
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ada5fd
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author J. J. Hermes
Joseph A. Guidry
Zachary P. Vanderbosch
Mariona Badenas-Agusti
Siyi Xu
Malia L. Kao
Antonio C. Rodriguez
Keith Hawkins
author_facet J. J. Hermes
Joseph A. Guidry
Zachary P. Vanderbosch
Mariona Badenas-Agusti
Siyi Xu
Malia L. Kao
Antonio C. Rodriguez
Keith Hawkins
author_sort J. J. Hermes
collection DOAJ
description We present the discovery of deep but sporadic transits in the flux of SBSS 1232+563, a metal-rich white dwarf polluted by disrupted exoplanetary debris. Nearly 25 yr of photometry from multiple sky surveys reveal evidence of occasional dimming of the white dwarf, most notably evident in an 8 month long event in 2023 that caused a >40% drop in flux from the star. In-transit follow-up shows additional short-timescale (minutes- to hours-long) dimming events. Transiting Exoplanet Survey Satellite photometry suggests a coherent 14.842 hr signal that could represent the dominant orbital period of debris. Six low-resolution spectra collected at various transit depths over two decades show no evidence of significant changes in the observed elemental abundances. SBSS 1232+563 demonstrates that debris transits around white dwarfs can be sporadic, with many years of inactivity before large-amplitude dimming events.
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spelling doaj-art-04355660eb3d49028c1704491f0efd3c2025-02-04T06:24:12ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-0198015610.3847/1538-4357/ada5fdSporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563J. J. Hermes0https://orcid.org/0000-0001-5941-2286Joseph A. Guidry1https://orcid.org/0000-0001-9632-7347Zachary P. Vanderbosch2https://orcid.org/0000-0002-0853-3464Mariona Badenas-Agusti3https://orcid.org/0000-0003-4903-567XSiyi Xu4https://orcid.org/0000-0002-8808-4282Malia L. Kao5https://orcid.org/0000-0001-5745-3535Antonio C. Rodriguez6https://orcid.org/0000-0003-4189-9668Keith Hawkins7https://orcid.org/0000-0002-1423-2174Department of Astronomy, Boston University , 725 Commonwealth Avenue, Boston, MA 02215, USA ; jjhermes@bu.eduDepartment of Astronomy, Boston University , 725 Commonwealth Avenue, Boston, MA 02215, USA ; jjhermes@bu.eduDivision of Physics, Mathematics, and Astronomy, California Institute of Technology , Pasadena, CA 91125, USAInstitute of Astronomy, University of Cambridge , Madingley Road, Cambridge CB3 0HA, UKGemini Observatory/NSF’s NOIRLab , 670 N. A’ohoku Place, Hilo, HI 96720, USADepartment of Astronomy, University of Texas at Austin , 2515 Speedway, Austin, TX 78712, USADivision of Physics, Mathematics, and Astronomy, California Institute of Technology , Pasadena, CA 91125, USADepartment of Astronomy, University of Texas at Austin , 2515 Speedway, Austin, TX 78712, USAWe present the discovery of deep but sporadic transits in the flux of SBSS 1232+563, a metal-rich white dwarf polluted by disrupted exoplanetary debris. Nearly 25 yr of photometry from multiple sky surveys reveal evidence of occasional dimming of the white dwarf, most notably evident in an 8 month long event in 2023 that caused a >40% drop in flux from the star. In-transit follow-up shows additional short-timescale (minutes- to hours-long) dimming events. Transiting Exoplanet Survey Satellite photometry suggests a coherent 14.842 hr signal that could represent the dominant orbital period of debris. Six low-resolution spectra collected at various transit depths over two decades show no evidence of significant changes in the observed elemental abundances. SBSS 1232+563 demonstrates that debris transits around white dwarfs can be sporadic, with many years of inactivity before large-amplitude dimming events.https://doi.org/10.3847/1538-4357/ada5fdWhite dwarf starsTransitsDebris disksVariable stars
spellingShingle J. J. Hermes
Joseph A. Guidry
Zachary P. Vanderbosch
Mariona Badenas-Agusti
Siyi Xu
Malia L. Kao
Antonio C. Rodriguez
Keith Hawkins
Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563
The Astrophysical Journal
White dwarf stars
Transits
Debris disks
Variable stars
title Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563
title_full Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563
title_fullStr Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563
title_full_unstemmed Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563
title_short Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563
title_sort sporadic dips from extended debris transiting the metal rich white dwarf sbss 1232 563
topic White dwarf stars
Transits
Debris disks
Variable stars
url https://doi.org/10.3847/1538-4357/ada5fd
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