Analysing the Onset of Cometary Activity by the Jupiter-Family Comet 2023 RN3

Fuente: arXiv
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Autori principali: Dobson, Matthew M., Schwamb, Megan E., Fitzsimmons, Alan, Kelley, Michael S. P., Holt, Carrie E., Murtagh, Joseph, Hsieh, Henry H., Denneau, Larry, Erasmus, Nicolas, Heinze, A. N., Shingles, Luke J., Siverd, Robert J., Smith, Ken W., Tonry, John L., Weiland, Henry, Young, David. R., Lister, Tim, Gomez, Edward, Chatelain, Joey, Greenstreet, Sarah
Natura: Preprint
Pubblicazione: 2024
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author Dobson, Matthew M.
Schwamb, Megan E.
Fitzsimmons, Alan
Kelley, Michael S. P.
Holt, Carrie E.
Murtagh, Joseph
Hsieh, Henry H.
Denneau, Larry
Erasmus, Nicolas
Heinze, A. N.
Shingles, Luke J.
Siverd, Robert J.
Smith, Ken W.
Tonry, John L.
Weiland, Henry
Young, David. R.
Lister, Tim
Gomez, Edward
Chatelain, Joey
Greenstreet, Sarah
author_facet Dobson, Matthew M.
Schwamb, Megan E.
Fitzsimmons, Alan
Kelley, Michael S. P.
Holt, Carrie E.
Murtagh, Joseph
Hsieh, Henry H.
Denneau, Larry
Erasmus, Nicolas
Heinze, A. N.
Shingles, Luke J.
Siverd, Robert J.
Smith, Ken W.
Tonry, John L.
Weiland, Henry
Young, David. R.
Lister, Tim
Gomez, Edward
Chatelain, Joey
Greenstreet, Sarah
contents We utilize serendipitous observations from the Asteroid Terrestrial-impact Last Alert System (ATLAS) and the Zwicky Transient Facility (ZTF) in addition to targeted follow-up observations from the Las Cumbres Observatory (LCO) and Liverpool Telescope to analyze the first observed instance of cometary activity by the newly-discovered Jupiter-family comet C/2023 RN3 (ATLAS), whose orbital dynamics place it close to residing on a Centaur-like orbit. Across our 7-month baseline, we observe an epoch of cometary activity commencing in August 2023 with an increase in brightness of >5.4 mag. The lightcurve of 2023 RN3 indicates the presence of continuous cometary activity across our observations, suggesting the onset of a new period of sustained activity. We find no evidence of any outbursts on top of the observed brightening, nor do we find any significant color evolution across our observations. 2023 RN3 is visibly extended in LCO and Liverpool Telescope observations, indicating the presence of a spatially-extended coma. Numerical integration of 2023 RN3's orbit reveals the comet to have recently undergone a slight increase in semimajor axis due to a planetary encounter with Jupiter, however whether this orbital change could trigger 2023 RN3's cometary activity is unclear. Our estimate for the maximum dust production metric of Afrho ~400 cm is consistent with previous measurements for the Jupiter-family comet and Centaur populations.
format Preprint
id arxiv_https___arxiv_org_abs_2410_13644
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Analysing the Onset of Cometary Activity by the Jupiter-Family Comet 2023 RN3
Dobson, Matthew M.
Schwamb, Megan E.
Fitzsimmons, Alan
Kelley, Michael S. P.
Holt, Carrie E.
Murtagh, Joseph
Hsieh, Henry H.
Denneau, Larry
Erasmus, Nicolas
Heinze, A. N.
Shingles, Luke J.
Siverd, Robert J.
Smith, Ken W.
Tonry, John L.
Weiland, Henry
Young, David. R.
Lister, Tim
Gomez, Edward
Chatelain, Joey
Greenstreet, Sarah
Earth and Planetary Astrophysics
We utilize serendipitous observations from the Asteroid Terrestrial-impact Last Alert System (ATLAS) and the Zwicky Transient Facility (ZTF) in addition to targeted follow-up observations from the Las Cumbres Observatory (LCO) and Liverpool Telescope to analyze the first observed instance of cometary activity by the newly-discovered Jupiter-family comet C/2023 RN3 (ATLAS), whose orbital dynamics place it close to residing on a Centaur-like orbit. Across our 7-month baseline, we observe an epoch of cometary activity commencing in August 2023 with an increase in brightness of >5.4 mag. The lightcurve of 2023 RN3 indicates the presence of continuous cometary activity across our observations, suggesting the onset of a new period of sustained activity. We find no evidence of any outbursts on top of the observed brightening, nor do we find any significant color evolution across our observations. 2023 RN3 is visibly extended in LCO and Liverpool Telescope observations, indicating the presence of a spatially-extended coma. Numerical integration of 2023 RN3's orbit reveals the comet to have recently undergone a slight increase in semimajor axis due to a planetary encounter with Jupiter, however whether this orbital change could trigger 2023 RN3's cometary activity is unclear. Our estimate for the maximum dust production metric of Afrho ~400 cm is consistent with previous measurements for the Jupiter-family comet and Centaur populations.
title Analysing the Onset of Cometary Activity by the Jupiter-Family Comet 2023 RN3
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2410.13644