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Anomalous Orbital-Energy Changes Observed during Spacecraft Flybys of Earth
DOI: 10.1103/PhysRevLett.100.091102 Bibcode: 2008PhRvL.100i1102A

Anderson, John D.; Campbell, James K.; Ekelund, John E. +2 more

We report and characterize anomalous orbital-energy changes observed during six Earth flybys by the Galileo, NEAR, Cassini, Rosetta, and MESSENGER spacecraft. These anomalous energy changes are consistent with an empirical prediction formula which is proportional to the total orbital energy per unit mass and which involves the incoming and outgoin…

2008 Physical Review Letters
Rosetta 130
A Global Kinetic Model for Cometary Comae: The Evolution of the Coma of the Rosetta Target Comet Churyumov-Gerasimenko throughout the Mission
DOI: 10.1086/590376 Bibcode: 2008ApJ...685..659T

Tenishev, Valeriy; Combi, Michael; Davidsson, Björn

The Rosetta spacecraft is en route to comet 67P/Churyumov-Gerasimenko for a rendezvous, landing, and extensive orbital phase beginning in 2014. Model studies of the coma will be required not only for planning of the mission and interpretation of spacecraft data, but also for an expectedly large amount of complementary remote observational data tha…

2008 The Astrophysical Journal
Rosetta 119
Asteroids 2867 Steins and 21 Lutetia: surface composition from far infrared observations with the Spitzer space telescope
DOI: 10.1051/0004-6361:20078085 Bibcode: 2008A&A...477..665B

Jorda, L.; Lamy, P. L.; Barucci, M. A. +8 more

Aims:The aim of this paper is to investigate the surface composition of the two asteroids 21 Lutetia and 2867 Steins, targets of the Rosetta space mission.
Methods: We observed the two asteroids through their full rotational periods with the Infrared Spectrograph of the Spitzer Space Telescope to investigate the surface properties. The analysi…

2008 Astronomy and Astrophysics
Rosetta 65
Cometary dust trail associated with Rosetta mission target: 67P/Churyumov Gerasimenko
DOI: 10.1016/j.icarus.2007.08.027 Bibcode: 2008Icar..193...96I

Ishiguro, Masateru

A thin, bright dust cloud, which is associated with the Rosetta mission target object (67P/Churyumov-Gerasimenko), was observed after the 2002 perihelion passage. The neckline structure or dust trail nature of this cloud is controversial. In this paper, we definitively identify the dust trail and the neckline structure using a wide-field CCD camer…

2008 Icarus
Rosetta 59
Visible and near infrared spectroscopic investigation of E-type asteroids, including 2867 Steins, a target of the Rosetta mission
DOI: 10.1016/j.icarus.2008.02.015 Bibcode: 2008Icar..196..119F

Barucci, M. A.; Fornasier, S.; Dotto, E. +1 more

We present the results of a visible spectroscopic survey of igneous asteroids belonging to the small and intriguing E-class, including 2867 Steins, a target of the Rosetta mission. The survey was carried out at the 3.5 m Telescopio Nazionale Galileo (TNG), and at the 3.5 m New Technology Telescope (NTT) of the European Southern Observatory. We obt…

2008 Icarus
Rosetta 42
The dust trail of Comet 67P/Churyumov Gerasimenko
DOI: 10.1016/j.icarus.2007.08.018 Bibcode: 2008Icar..193..572K

Reach, William T.; Kelley, Michael S.; Lien, David J.

We report the detection of Comet 67P/Churyumov-Gerasimenko's dust trail and nucleus in 24 µm Spitzer Space Telescope images taken February 2004. The dust trail is not found in optical Palomar images taken June 2003. Both the optical and infrared images show a distinct neck-line tail structure, offset from the projected orbit of the comet. We…

2008 Icarus
Rosetta 41
Structure and density of cometary nuclei
DOI: 10.1111/j.1945-5100.2008.tb00691.x Bibcode: 2008M&PS...43.1033W

Weissman, Paul R.; Lowry, Stephen C.

Understanding the nature of the cometary nucleus remains one of the major problems in solar system science. Whipple’s (1950) icy conglomerate model has been very successful at explaining a range of cometary phenomena, including the source of cometary activity and the nongravitational orbital motion of the nuclei. However, the internal structure of…

2008 Meteoritics and Planetary Science
Rosetta 40
Capabilities of Philae, the Rosetta Lander
DOI: 10.1007/s11214-007-9278-z Bibcode: 2008SSRv..138..275B

Biele, J.; Ulamec, S.

In situ (and sample return) space missions are the most promising tools to investigate the origin and evolution of comet nuclei. We present the instruments and investigations that will be performed with PHILAE (the ROSETTA Lander) on comet 67P Churyumov Gerasimenko, starting in November 2014, ten years after launch. The rationale and the performan…

2008 Space Science Reviews
Rosetta 38
Results from the ESA SREM monitors and comparison with existing radiation belt models
DOI: 10.1016/j.asr.2008.03.022 Bibcode: 2008AdSpR..42.1527E

Nieminen, P.; Hajdas, W.; Bühler, P. +3 more

The Standard Radiation Environment Monitor (SREM) is a simple particle detector developed for wide application on ESA satellites. It measures high-energy protons and electrons of the space environment with a 20° angular resolution and limited spectral information. Of the ten SREMs that have been manufactured, four have so far flown. The first mode…

2008 Advances in Space Research
INTEGRAL Rosetta 36
Heterogeneous solid/gas chemistry of organic compounds related to comets, meteorites, Titan, and Mars: Laboratory and in lower Earth orbit experiments
DOI: 10.1016/j.asr.2007.09.017 Bibcode: 2008AdSpR..42.2019C

Szopa, C.; Cottin, H.; Coll, P. +14 more

To understand the evolution of organic molecules involved in extraterrestrial environments and with exobiological implications, many experimental programs in the laboratory are devoted to photochemical studies in the gaseous phase as well as in the solid state. The validity of such studies and their applications to extraterrestrial environments ca…

2008 Advances in Space Research
Rosetta 35