Real-time Early Solar System Evolution in RW Auriga A: A New Major Dimming Event has Started in 2025 February

Abstract In this Note1 we introduce the problem of the highly dynamic T Tauri system RWAurA, and, using new analyses of lightcurves and imaged jet structures, its potential for understanding early solar system formation processes. In the following Note2 we describe how new physical modeling strengthens our arguments for the dynamic behavior of RWAurA arising from a migrating, differentiated, tidally disrupted Vesta-sized planetesimal. In the past two decades, the system’s lightcurve has undergone extreme excursions, dropping by up to 3 mag versus the normal median level. Of most importance here is the lightcurve event of 2014–2020, and the new major lightcurve downturn event that started in 2025 February (C. M. Lisse et al. 2025 CBAT). As we are finding that RWAurA is a solar system-sized laboratory allowing real-time study of early solar system formation processes, the new system-wide event needs to be observed on daily timescales for the next few years.

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Publication Details

Journal
Research Notes of the AAS
Published
2025-10-16
DOI
https://doi.org/10.3847/2515-5172/ae12e4
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.00
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article

Real-time Early Solar System Evolution in RW Auriga A: A New Major Dimming Event has Started in 2025 February

Joel D. Green, Alan P. Jackson, Brandon Johnson, S. J. Wolk et al.
Research Notes of the AAS
Astro and Planetary Science
article

Real-time Early Solar System Evolution in RW Auriga A: A New Major Dimming Event has Started in 2025 February

Joel D. Green, Alan P. Jackson, Brandon Johnson, S. J. Wolk, Tracy L. Beck, Hans Moritz Günther, Steven M. Silverberg, M. Koutoulaki, Jordan K. Steckloff, Tushar Mittal, C. M. Lisse, B. A. Sargent, S. Brittain, Catherine Espaillat, Michael L. Sitko, Christine Chen
article en

Abstract

Abstract In this Note1 we introduce the problem of the highly dynamic T Tauri system RWAurA, and, using new analyses of lightcurves and imaged jet structures, its potential for understanding early solar system formation processes. In the following Note2 we describe how new physical modeling strengthens our arguments for the dynamic behavior of RWAurA arising from a migrating, differentiated, tidally disrupted Vesta-sized planetesimal. In the past two decades, the system’s lightcurve has undergone extreme excursions, dropping by up to 3 mag versus the normal median level. Of most importance here is the lightcurve event of 2014–2020, and the new major lightcurve downturn event that started in 2025 February (C. M. Lisse et al. 2025 CBAT). As we are finding that RWAurA is a solar system-sized laboratory allowing real-time study of early solar system formation processes, the new system-wide event needs to be observed on daily timescales for the next few years.

Research Notes of the AASVol. 9(10)
Openalex Percentile: Top 80%
Astro and Planetary Science
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