Search Publications

Measurement of D/H and 13C/12C ratios in methane ice on Eris and Makemake: Evidence for internal activity
DOI: 10.1016/j.icarus.2023.115923 Bibcode: 2024Icar..41115923G

Lunine, J. I.; Emery, J. P.; Hammel, H. B. +13 more

James Webb Space Telescope's NIRSpec infrared imaging spectrometer observed the outer solar system dwarf planets Eris and Makemake in reflected sunlight at wavelengths spanning 1 through 5 µm. Both objects have high albedo surfaces that are rich in methane ice, with a texture that permits long optical path lengths through the ice for solar p…

2024 Icarus
Rosetta JWST 18
Chemistry of Complex Organic Molecules in the V883 Ori Disk Revealed by ALMA Band 3 Observations
DOI: 10.3847/1538-3881/ad11d9 Bibcode: 2024AJ....167...66Y

Aikawa, Yuri; Nomura, Hideko; Yamato, Yoshihide +3 more

Complex organic molecules (COMs) in protoplanetary disks are key to understanding the origin of volatiles in comets in our solar system, yet the chemistry of COMs in protoplanetary disks remains poorly understood. Here, we present Atacama Large Millimeter/submillimeter Array Band 3 observations of the disk around the young outbursting star V883 Or…

2024 The Astronomical Journal
Rosetta 17
The Ice Chemistry in Comets and Planet-forming Disks: Statistical Comparison of CH3OH, H2CO, and NH3 Abundance Ratios
DOI: 10.3847/2041-8213/ad5a6d Bibcode: 2024ApJ...970L...5L

Ceccarelli, Cecilia; Codella, Claudio; Villanueva, Geronimo L. +5 more

Comets are frozen remnants of our solar system's formation, and comparing their chemical composition to that of planet-forming systems can reveal crucial insights about our origins, potentially answering one of the most challenging questions in planetary science, i.e., whether cometary material was mainly inherited from the protosolar nebula or re…

2024 The Astrophysical Journal
Rosetta JWST 8
The GUAPOS project - V: The chemical ingredients of a massive stellar protocluster in the making
DOI: 10.1093/mnras/stae676 Bibcode: 2024MNRAS.529.3244L

Testi, L.; Mininni, C.; Lorenzani, A. +9 more

Most stars, including the Sun, are born in rich stellar clusters containing massive stars. Therefore, the study of the chemical reservoir of massive star-forming regions is crucial to understand the basic chemical ingredients available at the dawn of planetary systems. We present a detailed study of the molecular inventory of the hot molecular cor…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 7
Properties of the gas escaping from a non-isothermal porous dust surface layer of a comet
DOI: 10.1093/mnras/stad3994 Bibcode: 2024MNRAS.52712268S

Mottola, S.; Küppers, M.; Thomas, N. +6 more

Estimation of the properties of the sublimation products leaving the cometary nucleus is one of the significant questions in the study of the dusty-gas flow following the Rosetta mission. It is widely assumed that the temperature of the water molecules emitted is the temperature of ice directly exposed to the surface. However, it is the simplest n…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 6
Diurnal Ejection of Boulder Clusters on Comet 67P Lasting beyond 3 au
DOI: 10.3847/2041-8213/ad18d9 Bibcode: 2024ApJ...961L..16S

Keller, Horst Uwe; Shi, Xian; Güttler, Carsten +6 more

Ejection of large boulder-like debris is a vigorous form of cometary activity that is unlikely induced by water ice out-gassing alone but rather associated with the sublimation of super-volatile ices. Though perceived on several comets, the actual pattern and mechanism of such activity are still unclear. Here we report on a specialized observation…

2024 The Astrophysical Journal
Rosetta 5
Cliff collapse on Comet 67P/Churyumov-Gerasimenko - I. Aswan
DOI: 10.1093/mnras/stad3055 Bibcode: 2024MNRAS.527..112D

Davidsson, Björn J. R.

The Aswan cliff on Comet 67P/Churyumov-Gerasimenko collapsed on 2015 July 10. Thereby, relatively pristine comet material from a depth of $\sim 12\, \mathrm{m}$ was exposed at the surface. Observations of the collapse site by the microwave instrument Rosetta/Microwave Instrument for Rosetta Orbiter (MIRO) have been retrieved from 8 months prior to…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 5
Deciphering cometary outbursts: linking gas composition changes to trigger mechanisms
DOI: 10.1093/mnras/stae622 Bibcode: 2024MNRAS.529.2763M

Mall, Urs; De Keyser, Johan; Berthelier, Jean-Jacques +9 more

Dust and gas outbursts are recurrent cometary phenomena, playing a crucial role in shaping the coma. Proposed outburst trigger mechanisms include cliff collapse, pressure pockets, and amorphous-to-crystalline phase transition of water ice; however, the underlying processes remain inadequately understood. In this study, we analyse Rosetta/ROSINA da…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 5
Evidence for Abiotic Dimethyl Sulfide in Cometary Matter
DOI: 10.3847/1538-4357/ad8565 Bibcode: 2024ApJ...976...74H

De Keyser, Johan; Altwegg, Kathrin; Hänni, Nora +5 more

Technological progress related to astronomical observatories such as the recently launched James Webb Space Telescope (JWST) allows searching for signs of life beyond our solar system, namely, in the form of unambiguous biosignature gases in exoplanetary atmospheres. The tentative assignment of a 1σ–2.4σ spectral feature observed with JWST in the …

2024 The Astrophysical Journal
Rosetta 5
Measuring Erosional and Depositional Patterns Across Comet 67P's Imhotep Region
DOI: 10.1029/2023JE008089 Bibcode: 2024JGRE..12908089J

Soderblom, J. M.; Hayes, A. G.; Kirk, R. L. +8 more

Comet 67P/Churyumov-Gerasimenko displays a pronounced hemispherical dichotomy in surface morphology, where the southern hemisphere exhibits more erosional features than the northern hemisphere due to receiving much greater solar radiation. Consequently, it is generally assumed that particles are ejected from the southern hemisphere through sublima…

2024 Journal of Geophysical Research (Planets)
Rosetta 4