MOP:: A space debris and interplanetary dust sample return mission

被引：0

作者：

Scherer, K ^{[1
]}

Hilchenbach, M ^{[1
]}

Kirsch, E ^{[1
]}

Livi, S ^{[1
]}

Bendisch, J ^{[1
]}

Blum, J ^{[1
]}

Mutschke, H ^{[1
]}

Diedrich, T ^{[1
]}

Oelze, H ^{[1
]}

Flury, W ^{[1
]}

Geis, S ^{[1
]}

Fricke, J ^{[1
]}

Häusler, B ^{[1
]}

Huisken, F ^{[1
]}

Jessberger, EK ^{[1
]}

Klöck, W ^{[1
]}

Koppenwallner, G ^{[1
]}

Ott, U ^{[1
]}

Sdunnnus, H ^{[1
]}

Srama, R ^{[1
]}

机构：

[1] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany

来源：

14TH ESA SYMPOSIUM ON EUROPEAN ROCKET AND BALLOON PROGRAMMES AND RELATED RESEARCH | 1999年 / 437卷

关键词：

D O I：

暂无

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

Our knowledge of the dynamics and composition of interplanetary dust particles is mainly based on theoretical models. Only for a few dust grains that were captured in low Earth orbits (< 2000 km) the composition and mineralogy has been studied. The additional contribution of space debris at low altitudes is rather well understood, but the flux of small space debris in higher orbits could not yet be determined. The MOP spacecraft will have a geostationary transfer orbit (i.e. an apogee distance of approximate to 42000 km) and will collect on aerogel plates both species, the interplanetary as well as the artifical grains in high altitudes far away from atmospheric influence. After a reentry manoeuvre, these particles can be investigated in laboratories on Earth. Their traces in the aerogel can be used to determine velocities and impact directions. Moreover, the MOP satellite will carry a new instrument to detect in-situ nano-particles, i.e. particles with masses in the range between 10(-17)-10(-21) grams. Thus, for the first time, the MOP mission will provide direct information (a) on interplanetary dust particles and space debris in high altitudes up to geostationary orbits, (b) on their phase space vectors, and (c) on the fluxes of nano-particles.

引用

页码：541 / 546

页数：6

共 50 条

[1] A collector for interplanetary dust particles and space debris
Xu, YL
Zhang, HQ
Zhang, N
Yu, M
Xie, P
Fan, CY
PHYSICS, CHEMISTRY, AND DYNAMICS OF INTERPLANETARY DUST, 1996, 104 : 243 - 246
[2] STARDUST: Comet and interstellar dust sample return mission
Brownlee, DE
Burnett, D
Clark, B
Hanner, MS
Horz, F
Kissel, J
Newburn, R
Sandford, S
Sekanina, Z
Tsou, P
Zolensky, M
PHYSICS, CHEMISTRY, AND DYNAMICS OF INTERPLANETARY DUST, 1996, 104 : 223 - 226
[3] Mission design for the Deep Space 4/Champollion comet sample return mission
Tan-Wang, GH
Sims, JA
SPACEFLIGHT MECHANICS 1998, VOL 99, PTS 1 AND 2, 1998, 99 : 1205 - 1212
[4] STARDUST: Discovery's interstellar dust and cometary sample return mission
Atkins, KL
Brownlee, DE
Duxbury, T
Yen, CW
Tsou, P
Vellinga, JM
1997 IEEE AEROSPACE CONFERENCE PROCEEDINGS, VOL 4, 1997, : 229 - 245
[5] Trade Space Evaluation of Ascent and Return Architectures for a Mars Sample Return Mission
Alibay, Farah
Bailey, Zachary J.
2014 IEEE AEROSPACE CONFERENCE, 2014,
[6] Microanalyses of interplanetary dust particles and micrometeorites: implications for sample return missions to undifferentiated protoplanets
Rietmeijer, FJM
SCIENTIFIC EXPLORATION, PLANETARY PROTECTION, ACTIVE EXPERIMENTS AND DUSTY PLASMAS, 2004, 34 (11): : 2286 - 2291
[7] INTERPLANETARY DUST AND DEBRIS, AS OBSERVED FROM THE MOON
LEVASSEURREGOURD, AC
ASTRONOMY AND SPACE SCIENCE FROM THE MOON, 1994, 14 (06): : 77 - 85
[8] Interplanetary Waveriders for atmospheric sample return
Lyons, Daniel T.
Sklyanskiy, Evgeniy
ASTRODYNAMICS 2007, PTS I-III, 2008, 129 : 1169 - 1188
[9] DISTRIBUTION OF DUST IN INTERPLANETARY SPACE
BLACKWELL, DE
INGHAM, MF
PETFORD, AD
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1967, 136 (03) : 313 - +
[10] PHOBOS SAMPLE RETURN MISSION
GALEEV, AA
MOROZ, VI
LINKIN, VM
ZAKHAROV, AV
BASILEVSKY, AT
SURKOV, YA
AKIM, EL
DUXBURY, T
KREMNEV, RS
MARTYNOV, BN
PAPKOV, OV
IN-SITU IMPACT DETECTION TECHNIQUES, INTERPLANETARY DUST, AND FUTURE MARS EXPLORATION, 1995, 17 (12): : 31 - 47

← 1 2 3 4 5 →