Coma composition and profiles of comet 12P/Pons-Brooks using long-slit spectroscopy DOI Creative Commons
Léa Ferellec, Cyrielle Opitom, Abbie Donaldson

et al.

Monthly Notices of the Royal Astronomical Society, Journal Year: 2024, Volume and Issue: 534(3), P. 1816 - 1826

Published: Sept. 19, 2024

ABSTRACT Comet 12P/Pons–Brook exhibited multiple large and minor outbursts in 2023 on its way to 2024 perihelion, as it has done during previous apparitions. We obtained long-slit optical spectra of the comet August November with INT-IDS, December NOT-ALFOSC. Using a standard Haser model 10 000-km-radius aperture commonly used empirical parent daughter scale lengths, our calculated abundance ratios show constant ‘typical’ composition throughout period C$_2$/CN ratio about 90 per cent. Molecular density profiles different species along slit asymmetries between opposite sides coma that C$_2$ seems behave differently than CN C$_3$. Comparing shows this cannot accurately reproduce shape coma, therefore production rates be deemed accurate. an outburst is slightly better match C$_3$ profile shapes, but still does not explain requires equal lengths. Our results suggest morphology could explained by extended sources, nature 12P’s activity introduces bias determination composition.

Language: Английский

Mass of particles released by comet 12P/Pons–Brooks during 2023–2024 outbursts DOI Creative Commons
Maria Gritsevich, Marcin Wesołowski, A. J. Castro‐Tirado

et al.

Monthly Notices of the Royal Astronomical Society, Journal Year: 2025, Volume and Issue: 538(1), P. 470 - 479

Published: Feb. 5, 2025

ABSTRACT During its most recent return, comet 12P/Pons–Brooks experienced 14 well-documented outbursts, observed between 2023 June 13 and 2024 April, at heliocentric distances ranging from $4.26\,$ to $0.85\,$ au. After perihelion, two additional outbursts were in summer 2024, of $1.20\,$ $2.26\,$ Using observational data, we developed a numerical model estimate the mass ejected during these events, focusing on sublimation ice through porous cometary nucleus. The key factors affecting estimates are outburst amplitude active surface area both quiet phases. Pogson’s law was used express magnitude, incorporating scattering cross-sections agglomerates. iteratively determined considering various types (H$_{2}$O CO$_{2}$) controlling activity. Our results indicate that ranged 10$^{10}$ 10$^{13}$ kg. findings highlight significant role morphology thermodynamic conditions providing insights into mechanisms driving phenomena their implications for evolution dust trail formation. Based analysis propose six-level classification scheme outbursts.

Language: Английский

Citations

1

Boulder Migration in the Khonsu Region of Comet 67P/Churyumov–Gerasimenko DOI Creative Commons
X.D. Tang, Xian Shi, M. R. El‐Maarry

et al.

The Astrophysical Journal, Journal Year: 2025, Volume and Issue: 979(1), P. 91 - 91

Published: Jan. 20, 2025

Abstract The European Space Agency's Rosetta mission is the only space that has performed long-term monitoring of a comet at close distances. For over two years, rendezvoused with 67P/Churyumov–Gerasimenko, which revealed diverse evolutionary processes cometary nucleus. One most striking events migration ∼30 m boulder in southern hemisphere region Khonsu. Previous works found boulder's ∼140 displacement occurred during three months from 2015 August to October, and several triggering mechanisms were proposed, including outburst site, seismic vibrations nearby activities, or surface erosion slope beneath boulder. In this work, we further analyze impressive event by analyzing imaging data Rosetta's OSIRIS camera. We constrained time within 14 hr derived detailed timeline local dust activities. High-resolution thermophysical modeling shows significant dichotomy thermal history northern sides, could have triggered facilitated its via own volatile activity.

Language: Английский

Citations

0

Coma composition and profiles of comet 12P/Pons-Brooks using long-slit spectroscopy DOI Creative Commons
Léa Ferellec, Cyrielle Opitom, Abbie Donaldson

et al.

Monthly Notices of the Royal Astronomical Society, Journal Year: 2024, Volume and Issue: 534(3), P. 1816 - 1826

Published: Sept. 19, 2024

ABSTRACT Comet 12P/Pons–Brook exhibited multiple large and minor outbursts in 2023 on its way to 2024 perihelion, as it has done during previous apparitions. We obtained long-slit optical spectra of the comet August November with INT-IDS, December NOT-ALFOSC. Using a standard Haser model 10 000-km-radius aperture commonly used empirical parent daughter scale lengths, our calculated abundance ratios show constant ‘typical’ composition throughout period C$_2$/CN ratio about 90 per cent. Molecular density profiles different species along slit asymmetries between opposite sides coma that C$_2$ seems behave differently than CN C$_3$. Comparing shows this cannot accurately reproduce shape coma, therefore production rates be deemed accurate. an outburst is slightly better match C$_3$ profile shapes, but still does not explain requires equal lengths. Our results suggest morphology could explained by extended sources, nature 12P’s activity introduces bias determination composition.

Language: Английский

Citations

0