MASCOT—The Mobile Asteroid Surface Scout Onboard the Hayabusa2 Mission

被引：4

作者：

Tra-Mi Ho

Volodymyr Baturkin

Christian Grimm

Jan Thimo Grundmann

Catherin Hobbie

Eugen Ksenik

Caroline Lange

Kaname Sasaki

Markus Schlotterer

Maria Talapina

Nawarat Termtanasombat

Elisabet Wejmo

Lars Witte

Michael Wrasmann

Guido Wübbels

Johannes Rößler

Christian Ziach

Ross Findlay

Jens Biele

Christian Krause

Stephan Ulamec

Michael Lange

Olaf Mierheim

Roy Lichtenheldt

Maximilian Maier

Josef Reill

Hans-Jürgen Sedlmayr

Pierre Bousquet

Anthony Bellion

Olivier Bompis

Celine Cenac-Morthe

Muriel Deleuze

Stephane Fredon

Eric Jurado

Elisabet Canalias

Ralf Jaumann

Jean-Pierre Bibring

Karl Heinz Glassmeier

David Hercik

Matthias Grott

Luca Celotti

Federico Cordero

Jeffrey Hendrikse

Tatsuaki Okada

机构：

[1] DLR (German Aerospace Center),Institute of Space Systems

[2] DLR,Space Operations and Astronaut Training, MUSC

[3] DLR,Institute of Composite Structures and Adaptive Systems

[4] DLR,Robotic and Mechatronics Center

[5] DLR,Institute of Planetary Research

[6] CNES,IAS

[7] DLR,undefined

[8] Université Paris Sud,undefined

[9] Technische Universität Braunschweig,undefined

[10] Active Space Technologies GmbH,undefined

[11] Telespazio-Vega,undefined

[12] Airbus DS,undefined

[13] ISAS/JAXA,undefined

来源：

Space Science Reviews | 2017年 / 208卷

关键词：

Hayabusa2; MASCOT; Surface science package; Asteroid;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

On December 3rd, 2014, the Japanese Space Agency (JAXA) launched successfully the Hayabusa2 (HY2) spacecraft to its journey to Near Earth asteroid (162173) Ryugu. Aboard this spacecraft is a compact landing package, MASCOT (Mobile Asteroid surface SCOuT), which was developed by the German Aerospace Centre (DLR) in collaboration with the Centre National d’Etudes Spatiales (CNES). Similar to the famous predecessor mission Hayabusa, Hayabusa2, will also study an asteroid and return samples to Earth. This time, however, the target is a C-type asteroid which is considered to be more primitive than (25143) Itokawa and provide insight into an even earlier stage of our Solar System.

引用

页码：339 / 374

页数：35

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