Search Publications

Evidence of ammonium salts in comet 67P as explanation for the nitrogen depletion in cometary comae
DOI: 10.1038/s41550-019-0991-9 Bibcode: 2020NatAs...4..533A

De Keyser, Johan; Gombosi, Tamas I.; Berthelier, Jean-Jacques +14 more

Cometary comae are generally depleted in nitrogen. The main carriers for volatile nitrogen in comets are NH3 and HCN. It is known that ammonia readily combines with many acids, such as HCN, HNCO and HCOOH, encountered in the interstellar medium as well as in cometary ice to form ammonium salts (NH4+X-) a…

2020 Nature Astronomy
Rosetta 109
Infrared detection of aliphatic organics on a cometary nucleus
DOI: 10.1038/s41550-019-0992-8 Bibcode: 2020NatAs...4..500R

Bellucci, G.; Carlson, R. W.; Fornasier, S. +28 more

The European Space Agency's Rosetta mission1 has acquired unprecedented measurements of the surface of the nucleus of comet 67P/Churyumov-Gerasimenko (hereafter, 67P), the composition of which, as determined by in situ and remote-sensing instruments, including the VIRTIS instrument2, seems to be an assemblage of ices, mineral…

2020 Nature Astronomy
Rosetta 60
Far-ultraviolet aurora identified at comet 67P/Churyumov-Gerasimenko
DOI: 10.1038/s41550-020-1171-7 Bibcode: 2020NatAs...4.1084G

Altwegg, K.; Feldman, P. D.; Carr, C. +14 more

Having a nucleus darker than charcoal, comets are usually detected from Earth through the emissions from their coma. The coma is an envelope of gas that forms through the sublimation of ices from the nucleus as the comet gets closer to the Sun. In the far-ultraviolet portion of the spectrum, observations of comae have revealed the presence of atom…

2020 Nature Astronomy
Rosetta 18