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Dust-to-Gas and Refractory-to-Ice Mass Ratios of Comet 67P/Churyumov-Gerasimenko from Rosetta Observations
DOI: 10.1007/s11214-020-00662-1 Bibcode: 2020SSRv..216...44C

Pätzold, Martin; Choukroun, Mathieu; Thomas, Nicolas +9 more

This chapter reviews the estimates of the dust-to-gas and refractory-to-ice mass ratios derived from Rosetta measurements in the lost materials and the nucleus of 67P/Churyumov-Gerasimenko, respectively. First, the measurements by Rosetta instruments are described, as well as relevant characteristics of 67P. The complex picture of the activity of …

2020 Space Science Reviews
Rosetta 79
On the Origin and Evolution of the Material in 67P/Churyumov-Gerasimenko
DOI: 10.1007/s11214-020-00718-2 Bibcode: 2020SSRv..216..102R

Morbidelli, Alessandro; Snodgrass, Colin; Altwegg, Kathrin +5 more

Primitive objects like comets hold important information on the material that formed our solar system. Several comets have been visited by spacecraft and many more have been observed through Earth- and space-based telescopes. Still our understanding remains limited. Molecular abundances in comets have been shown to be similar to interstellar ices …

2020 Space Science Reviews
Rosetta 48
Origin and Evolution of Cometary Nuclei
DOI: 10.1007/s11214-019-0625-7 Bibcode: 2020SSRv..216....6W

Blum, Jürgen; Morbidelli, Alessandro; Davidsson, Björn +1 more

One of the key goals of the Rosetta mission was to understand how, where and when comets formed in our solar system. There are two major hypotheses for the origin of comets, both pre-Rosetta: (1) hierarchical accretion of dust and ice grains in the Solar Nebula and (2) the growth of pebbles, which are then brought together by streaming instabiliti…

2020 Space Science Reviews
Rosetta 36
Cometary Nuclei—From Giotto to Rosetta
DOI: 10.1007/s11214-020-0634-6 Bibcode: 2020SSRv..216...14K

Keller, Horst Uwe; Kührt, Ekkehard

We will briefly recapitulate the beginning of modern cometary physic. Then we will assess the results of the cometary flyby missions previous to ESA's Rosetta rendezvous with comet 67P/Churyumov-Gerasimenko. Emphasis is given to the physical properties of cometary nuclei. We will relate the results of the Rosetta mission to those of the flybys. A …

2020 Space Science Reviews
Rosetta 34
Cometary Comae-Surface Links
DOI: 10.1007/s11214-020-00744-0 Bibcode: 2020SSRv..216..130M

Skorov, Yuri; Kappel, David; Vincent, Jean-Baptiste +9 more

A comet is a highly dynamic object, undergoing a permanent state of change. These changes have to be carefully classified and considered according to their intrinsic temporal and spatial scales. The Rosetta mission has, through its contiguous in-situ and remote sensing coverage of comet 67P/Churyumov-Gerasimenko (hereafter 67P) over the time span …

2020 Space Science Reviews
Rosetta 20
Nongravitational Effects of Cometary Activity
DOI: 10.1007/s11214-019-0627-5 Bibcode: 2020SSRv..216....2M

Keller, Horst Uwe; Skorov, Yuri; Mottola, Stefano +4 more

Nongravitational forces induced by sublimation of volatiles affect the rotational and orbital dynamics of comets. In addition to contributing to the improvement of ephemerides and of rotational models, nongravitational effects can help constrain the regional distribution and temporal evolution of cometary activity, which in turn provides input for…

2020 Space Science Reviews
Rosetta 14
Tracing the Origins of the Ice Giants Through Noble Gas Isotopic Composition
DOI: 10.1007/s11214-020-00723-5 Bibcode: 2020SSRv..216...99M

Mousis, O.; Marty, B.; Mandt, K. E. +4 more

The current composition of giant planet atmospheres provides information on how such planets formed, and on the origin of the solid building blocks that contributed to their formation. Noble gas abundances and their isotope ratios are among the most valuable pieces of evidence for tracing the origin of the materials from which the giant planets fo…

2020 Space Science Reviews
Rosetta 13