First <i>JWST</i> spectrum of distant activity in long-period comet C/2024 E1 (Wierzchos)

ABSTRACT We observed the new long-period comet C/2024 E1 (Wierzchos), inbound at 7 au from the Sun, using the Near-Infrared Spectrograph (NIRSpec) integral field unit on JWST. The spectrum shows absorption features due to water ice in the coma and evidence for CO$_2$ driven activity, with a production rate of $Q(\mathrm{ CO}_2) = 2.546 \pm 0.019 \times 10^{25}$ molecules s$^{-1}$, and no emission features of water or CO. The latter is surprising, given that CO is more volatile than CO$_2$, and suggests that this comet may have lost its near-surface CO during its early evolution, before implantation in the Oort cloud.

Authors

Institutions

Publication Details

Journal
Monthly Notices of the Royal Astronomical Society Letters
Published
2025-05-07
DOI
https://doi.org/10.1093/mnrasl/slaf046
Citations
5
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
5.77

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

First JWST spectrum of distant activity in long-period comet C/2024 E1 (Wierzchos)

Aurélie Guilbert-Lepoutre, C. Tubiana, Michael S. P. Kelley, Emmanuël Jehin et al.
5 citations
Monthly Notices of the Royal Astronomical Society Letters
Astro and Planetary Science
5.77
article

First JWST spectrum of distant activity in long-period comet C/2024 E1 (Wierzchos)

Aurélie Guilbert-Lepoutre, C. Tubiana, Michael S. P. Kelley, Emmanuël Jehin, C. Snodgrass, Rosita Kokotanekova, M. Micheli, Matthew M. Knight, Carrie E. Holt, Cyrielle Opitom, Davide Farnocchia, A. Migliorini
article en
5 citations

Abstract

ABSTRACT We observed the new long-period comet C/2024 E1 (Wierzchos), inbound at 7 au from the Sun, using the Near-Infrared Spectrograph (NIRSpec) integral field unit on JWST. The spectrum shows absorption features due to water ice in the coma and evidence for CO$_2$ driven activity, with a production rate of $Q(\mathrm{ CO}_2) = 2.546 \pm 0.019 \times 10^{25}$ molecules s$^{-1}$, and no emission features of water or CO. The latter is surprising, given that CO is more volatile than CO$_2$, and suggests that this comet may have lost its near-surface CO during its early evolution, before implantation in the Oort cloud.

Monthly Notices of the Royal Astronomical Society LettersVol. 541(1)
Université Claude Bernard Lyon 1 (FR), Las Cumbres Observatory Global Telescope Network (US), Centre National de la Recherche Scientifique (FR), Jet Propulsion Laboratory (US), University of Liège (BE), United States Naval Academy (US), Istituto Nazionale di Fisica Nucleare, Galileo Galilei Institute for Theoretical Physics (IT), Astronomical Observatory of Rome (IT), Institute for Space Astrophysics and Planetology (IT), Royal Observatory (GB), Institute of Astronomy and National Astronomical Observatory (BG), Laboratoire de Géologie de Lyon : Terre, Planètes et Environnement (FR), University of Maryland, College Park (US), International Space Science Institute (CH), University of Edinburgh (GB)
National Aeronautics and Space Administration, California Institute of Technology, UK Space Agency, Space Telescope Science Institute, Fonds De La Recherche Scientifique - FNRS, Centre National d’Etudes Spatiales, Bulgarian National Science Fund, Jet Propulsion Laboratory
Clean water and sanitation
Openalex Percentile: Top 4%
Astro and Planetary Science
5.77
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.