2019
DOI: 10.48550/arxiv.1907.11081
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

AMBITION -- Comet Nucleus Cryogenic Sample Return (White paper for ESA's Voyage 2050 programme)

Abstract: The Giotto mission was the first interplanetary probe ever flown by the European Space Agency (ESA). Selected in 1980 and flown in 1985, Giotto was the most daring of an international fleet of five spaceprobes, which triumphantly visited the comet of all comets, 1P/Halley, in March 1986. Earlier on, in 1984, ESA and NASA established a Comet Nucleus Sample Return Science Definition Team; their work led in 1993 to the selection of the Rosetta mission as the Planetary Cornerstone of ESA's long-term programme Ho… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2020
2020
2020
2020

Publication Types

Select...
1

Relationship

0
1

Authors

Journals

citations
Cited by 1 publication
(1 citation statement)
references
References 137 publications
(169 reference statements)
0
1
0
Order By: Relevance
“…Furthermore, the results of this paper emphasise the need for a cometary sample-return mission, since the exact knowledge of the chemical composition and the morphology of the cometary grains are mandatory to understand the physics of the cometary dust-ejection mechanisms and for the preparation of high-quality cometary analogue materials. It should be noted here that samples from the interior of a comet are required, due to the possible processing of the surface material (Bockelée-Morvan et al 2019). Bardyn et al (2017) argued, based on the O/C ratio of ∼ 0.2 of the cometary dust measured by the COSIMA instrument, that the organic compound can be best compared to insoluble organic matter found in carbonaceous chondrites.…”
Section: Discussion and Applications To Cometsmentioning
confidence: 99%
“…Furthermore, the results of this paper emphasise the need for a cometary sample-return mission, since the exact knowledge of the chemical composition and the morphology of the cometary grains are mandatory to understand the physics of the cometary dust-ejection mechanisms and for the preparation of high-quality cometary analogue materials. It should be noted here that samples from the interior of a comet are required, due to the possible processing of the surface material (Bockelée-Morvan et al 2019). Bardyn et al (2017) argued, based on the O/C ratio of ∼ 0.2 of the cometary dust measured by the COSIMA instrument, that the organic compound can be best compared to insoluble organic matter found in carbonaceous chondrites.…”
Section: Discussion and Applications To Cometsmentioning
confidence: 99%