Search Publications

A plausible link between the asteroid 21 Lutetia and CH carbonaceous chondrites
DOI: 10.1111/maps.12703 Bibcode: 2016M&PS...51.1795M

Fornasier, Sonia; Barucci, Maria A.; Trigo-Rodríguez, Josep M. +3 more

A crucial topic in planetology research is establishing links between primitive meteorites and their parent asteroids. In this study, we investigate the feasibility of a connection between asteroids similar to 21 Lutetia, encountered by the Rosetta mission in July 2010, and the CH3 carbonaceous chondrite Pecora Escarpment 91467 (PCA 91467). Severa…

2016 Meteoritics and Planetary Science
Rosetta 6
Exploring the Moon's surface for remnants of the lunar mantle 1. Dunite xenoliths in mare basalts. A crustal or mantle origin?
DOI: 10.1111/maps.12480 Bibcode: 2015M&PS...50.1449S

Shearer, Charles K.; Burger, Paul V.; Bell, Aaron S. +2 more

Remotely sensed observations from recent missions (e.g., GRAIL, Kaguya, Chandrayaan-1) have been interpreted as indicating that the deep crust and upper mantle are close to or at the lunar surface in many large impact basins (e.g., Crisium, Apollo, Moscoviense). If this is correct, the capability of either impact or volcanic processes to transport…

2015 Meteoritics and Planetary Science
Chandrayaan-1 15
SMART-1 end of life shallow regolith impact simulations
DOI: 10.1111/maps.12479 Bibcode: 2015M&PS...50.1436B

Foing, B.; Burchell, M. J.; Cole, M. J. +3 more

The SMART-1 end-of-life impact with the lunar surface was simulated with impacts in a two stage light-gas gun onto inclined basalt targets with a shallow surface layer of sand. This simulated the probable impact site, where a loose regolith will have overlaid a well consolidated basaltic layer of rock. The impact angles used were at 5° and 10° fro…

2015 Meteoritics and Planetary Science
SMART-1 10
Stardust Interstellar Preliminary Examination X: Impact speeds and directions of interstellar grains on the Stardust dust collector
DOI: 10.1111/maps.12219 Bibcode: 2014M&PS...49.1680S

Postberg, Frank; Altobelli, Nicolas; Trieloff, Mario +65 more

On the basis of an interstellar dust model compatible with Ulysses and Galileo observations, we calculate and predict the trajectories of interstellar dust (ISD) in the solar system and the distribution of the impact speeds, directions, and flux of ISD particles on the Stardust Interstellar Dust Collector during the two collection periods of the m…

2014 Meteoritics and Planetary Science
Ulysses 25
The evolution of co-orbiting material in the orbit of 2201 Oljato from 1980 to 2012 as deduced from Pioneer Venus Orbiter and Venus Express magnetic records
DOI: 10.1111/maps.12102 Bibcode: 2014M&PS...49...28L

Zhang, Tielong; Russell, Christopher T.; Lai, Hairong +1 more

Asteroid 2201 Oljato passed through perihelion inside the orbit of Venus near the time of its conjunction with Venus in 1980, 1983, and 1986. During those three years, many interplanetary field enhancements (IFEs) were observed by the Pioneer Venus Orbiter (PVO) in the longitude sector where the orbit of Oljato lies inside Venus' orbit. We attribu…

2014 Meteoritics and Planetary Science
VenusExpress 16
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
Rosetta target asteroid 2867 Steins: An unusual E-type asteroid
DOI: 10.1111/j.1945-5100.2008.tb01089.x Bibcode: 2008M&PS...43..905W

Weissman, Paul R.; Hicks, Michael D.; Choi, Young-Jun +2 more

ESA's Rosetta spacecraft will fly by main-belt asteroid 2867 Steins on September 5, 2008. We obtained new visible wavelength spectra of 2867 Steins on December 19, 2006 (UT), using the Palomar 5 m telescope and the facility Double Spectrograph. Two sets of spectra, taken ∼3 h apart, one half of the rotation period for 2867 Steins, show it to be an…

2008 Meteoritics and Planetary Science
Rosetta 11
Finite difference time domain simulation of radar wave propagation through comet nuclei dielectric models
DOI: 10.1111/j.1945-5100.2008.tb00695.x Bibcode: 2008M&PS...43.1085C

Heggy, Essam; Carley, Ruth A.

The 90 MHz radar-wave experiment, Comet Nucleus Sounding Experiment by Radiowave Transmission (CONSERT), on board the Rosetta mission (ESA, 2004) is expected to probe the nucleus of the comet 67P/Churyumov-Gerasimenko (67P/C-G) to reveal information on its physical properties, chemical composition, and internal structure. This investigation assess…

2008 Meteoritics and Planetary Science
Rosetta 9
A review of penetrometers for subsurface access on comets and asteroids
DOI: 10.1111/j.1945-5100.2008.tb00690.x Bibcode: 2008M&PS...43.1021G

Ball, Andrew J.; Glaser, David L.; Zacny, Kris A.

The characterization of comet and asteroid interiors will eventually require in situ exploration with drills, penetrators/penetrometers, hypervelocity impactors, excavators or other devices. Because they offer desirable scientific capabilities and relative mechanical simplicity, penetrators and penetrometers, which use only axial force to push ben…

2008 Meteoritics and Planetary Science
Rosetta 7
Gamma rays from cosmic radioactivities
DOI: 10.1111/j.1945-5100.2007.tb00566.x Bibcode: 2007M&PS...42.1145D

Diehl, Roland; Hartmann, Dieter H.; Prantzos, Nikos

Gamma rays from radioactive byproducts of cosmic nucleosynthesis are direct messengers from nuclear processes taking place in various cosmic sites, and can be measured with telescopes operated in space. Due to low detector sensitivity, up until now, only a handful of sources have been detected in that electromagnetic window. Cobalt lines from SN19…

2007 Meteoritics and Planetary Science
INTEGRAL 3