Outburst and Splitting of Interstellar Comet 2I/Borisov
- 1University of California at Los Angeles (jewitt@ucla.edu)
- 2Max Planck, Gottingen
- 3Space Telescope Science Institute
- 4Johns Hopkins University, Applied Physics Laboratory
- 5Technical University at Braunschweig
- 6University of Hawaii
We present Hubble Space Telescope observations of a photometric outburst and splitting event in interstellar comet 2I/Borisov. The outburst, first reported with the comet outbound at 2.8 AU (Drahus et al.~2020), was caused by the expulsion of solid particles having a combined cross-section about 100 sq. km and a mass in 0.1 mm sized particles 2e7 kg. The latter corresponds to 1e-4 of the mass of the nucleus, taken as a sphere of radius 500 m. A transient double nucleus was observed on UT 2020 March 30 (about three weeks after the outburst), having a cross-section 0.6 sq. km and corresponding dust mass 1e5 kg. The secondary was absent in images taken on and before March 28, and in images taken on and after April 03. The unexpectedly delayed appearance and rapid disappearance of the secondary are consistent with an origin through rotational bursting of one or more large (meter-sized) boulders under the action of outgassing torques, following their ejection from the main nucleus. Overall, our observations reveal that the outburst and splitting of the nucleus are minor events involving a negligible fraction of the total mass: 2I/Borisov will survive its passage through the planetary region largely unscathed.
Journal: The Astrophysical Journal Letters, Volume 896, Issue 2, id.L39
How to cite: Jewitt, D., Kim, Y., Mutchler, M., Weaver, H., Agarwal, J., and Hui, M.-T.: Outburst and Splitting of Interstellar Comet 2I/Borisov, Europlanet Science Congress 2020, online, 21 Sep–9 Oct 2020, EPSC2020-964, https://doi.org/10.5194/epsc2020-964, 2020.