Search Publications

CO-driven Activity in Comet C/2017 K2 (PANSTARRS)
DOI: 10.3847/2041-8213/aa921f Bibcode: 2017ApJ...849L...8M

Chambers, Kenneth C.; Magnier, Eugene; Bauer, James +12 more

Comet C/2017 K2 (PANSTARRS) was discovered by the Pan-STARRS1 (PS1) Survey on 2017 May 21 at a distance of 16.09 au from the Sun, the second most distant discovery of an active comet. Pre-discovery images in the PS1 archive back to 2014 and additional deep CFHT images between 2013 May 10-13 showed the comet to be active at 23.75 au. We derive an u…

2017 The Astrophysical Journal
Rosetta 44
Formation of Methylamine and Ethylamine in Extraterrestrial Ices and Their Role as Fundamental Building Blocks of Proteinogenic α-amino Acids
DOI: 10.3847/1538-4357/aa7edd Bibcode: 2017ApJ...845...83F

Kaiser, Ralf I.; Förstel, Marko; Bergantini, Alexandre +2 more

The -CH-NH2 moiety represents the fundamental building block of all proteinogenic amino acids, with the cyclic amino acid proline being a special case (-CH-NH- in proline). Exploiting a chemical retrosynthesis, we reveal that methylamine (CH3NH2) and/or ethylamine (CH3CH2NH2) are es…

2017 The Astrophysical Journal
Rosetta 38
The Role of Pebble Fragmentation in Planetesimal Formation. II. Numerical Simulations
DOI: 10.3847/1538-4357/835/1/109 Bibcode: 2017ApJ...835..109W

Blum, Jürgen; Johansen, Anders; Wahlberg Jansson, Karl +1 more

Some scenarios for planetesimal formation go through a phase of collapse of gravitationally bound clouds of millimeter- to centimeter-size pebbles. Such clouds can form, for example, through the streaming instability in protoplanetary disks. We model the collapse process with a statistical model to obtain the internal structure of planetesimals wi…

2017 The Astrophysical Journal
Rosetta 30
Impact of Radiogenic Heating on the Formation Conditions of Comet 67P/Churyumov-Gerasimenko
DOI: 10.3847/2041-8213/aa6839 Bibcode: 2017ApJ...839L...4M

Wurz, P.; Altwegg, K.; Balsiger, H. +19 more

Because of the high fraction of refractory material present in comets, the heat produced by the radiogenic decay of elements such as aluminum and iron can be high enough to induce the loss of ultravolatile species such as nitrogen, argon, or carbon monoxide during their accretion phase in the protosolar nebula (PSN). Here, we investigate how heat …

2017 The Astrophysical Journal
Rosetta 19
Production of Sulfur Allotropes in Electron Irradiated Jupiter Trojans Ice Analogs
DOI: 10.3847/1538-4357/aa85e0 Bibcode: 2017ApJ...846..148M

Ehlmann, Bethany L.; Brown, Michael E.; Choukroun, Mathieu +7 more

In this paper, we investigate sulfur chemistry in laboratory analogs of Jupiter Trojans and Kuiper Belt Objects (KBOs). Electron irradiation experiments of CH3OH-NH3-H2O and H2S-CH3OH-NH3-H2O ices were conducted to better understand the chemical differences between primor…

2017 The Astrophysical Journal
Rosetta 19
A New 3D Multi-fluid Dust Model: A Study of the Effects of Activity and Nucleus Rotation on Dust Grain Behavior at Comet 67P/Churyumov-Gerasimenko
DOI: 10.3847/1538-4357/aa91ca Bibcode: 2017ApJ...850...72S

Huang, Z.; Jia, X.; Fougere, N. +7 more

Improving our capability to interpret observations of cometary dust is necessary to deepen our understanding of the role of dust in the formation of comets and in altering the cometary environments. Models including dust grains are in demand to interpret observations and test hypotheses. Several existing models have taken into account the gas-dust…

2017 The Astrophysical Journal
Rosetta 8
Stability of Sulphur Dimers (S2) in Cometary Ices
DOI: 10.3847/1538-4357/aa5279 Bibcode: 2017ApJ...835..134M

Lunine, J. I.; Mousis, O.; Ronnet, T. +5 more

S2 has been observed for decades in comets, including comet 67P/Churyumov-Gerasimenko. Despite the fact that this molecule appears ubiquitous in these bodies, the nature of its source remains unknown. In this study, we assume that S2 is formed by irradiation (photolysis and/or radiolysis) of S-bearing molecules embedded in th…

2017 The Astrophysical Journal
Rosetta 7
Dynamic Deuterium Enrichment in Cometary Water via Eley-Rideal Reactions
DOI: 10.3847/1538-4357/835/1/67 Bibcode: 2017ApJ...835...67Y

Yao, Yunxi; Giapis, Konstantinos P.

The deuterium-to-hydrogen ratio (D/H) in water found in the coma of Jupiter family comet (JFC) 67P/Churyumov-Gerasimenko was reported to be (5.3 ± 0.7) × 10-4, the highest among comets and three times the value for other JFCs with an ocean-like ratio. This discrepancy suggests the diverse origins of JFCs and clouds the issue of the orig…

2017 The Astrophysical Journal
Rosetta 3