Search Publications

Reconstruction of the surface topography from single images with the photometric method
DOI: 10.1134/S0038094608060051 Bibcode: 2008SoSyR..42..522D

Bondarenko, N. V.; Dulova, I. A.; Skuratovsky, S. I. +1 more

The possibility of reconstructing the surface topography from single images with the photometric method in the linear approximation is analyzed. The photometric method or surface topography Reconstruction employs a statistical approach to the problem formulation and is the most mathematically correct. This method allows determination of the most p…

2008 Solar System Research
MEx 7
Reduction of photographic observations of asteroids to the reference frame of a single catalog
DOI: 10.1134/S0038094608020068 Bibcode: 2008SoSyR..42..144C

Chernetenko, Yu. A.

In 2000, the last international program of photographic observations of selected asteroids aimed at the determination of the mutual orientation of the dynamic and stellar coordinate systems came to an end. The Institute of Applied Astronomy of the Russian Academy of Sciences collected more than 25 000 observations for 15 asteroids spanning from 19…

2008 Solar System Research
Hipparcos 3
On the probability of cryogenic mud volcanism on Titan
DOI: 10.1134/S0038094608020056 Bibcode: 2008SoSyR..42..139A

Alekseev, V. A.

Juxtaposing images of the surface of Titan made by the Huygens probe and photos of the mud volcano region on Earth (the Taman peninsula, the Caucasus) reveals similar geomorphologic features. This has led us to suggest the existence of cryogenic mud-volcanic activity on Titan. The role of liquid methane in supporting this process on Titan can be t…

2008 Solar System Research
Huygens 2
Craters, smooth terrains, flows, and layering on the comet nuclei
DOI: 10.1134/S0038094607020037 Bibcode: 2007SoSyR..41..109B

Keller, H. U.; Basilevsky, A. T.

The paper considers morphology of craters, smooth surfaces, and flows as well as signatures of layering observed on nuclei of Borrelly, Wild 2, and Tempel 1. In our analysis, we emphasize the role of the so-called planation process, which involves avalanche-type flows and can be responsible for the formation of flow-like features, smooth terrains,…

2007 Solar System Research
Rosetta 26
The Olympus volcano on Mars: Geometry and characteristics of lava flows
DOI: 10.1134/S0038094606050029 Bibcode: 2006SoSyR..40..375B

Neukum, G.; HRSC Co-Investigator Team; Basilevskaya, E. A.

The HRSC (image 0037) and MOC imagery and MOLA altimetry were used to determine the following parameters of the lava flows typical of the southern slope of the Martian volcano Olympus: the length (13-35 km), the width (0.2-4.8 km), and the angles of ground slopes along which these flows advanced (3.4°-6.9°). To measure the thickness of the flows, …

2006 Solar System Research
MEx 10
Search for causes of the low epithermal neutron flux anomaly in the Arabia Terra region (Mars)
DOI: 10.1134/S0038094606050017 Bibcode: 2006SoSyR..40..355B

Head, J. W.; Neukum, G.; Werner, S. +8 more

A geologic analysis of 274 images acquired by the high-resolution MOC camera onboard the Mars Global Surveyor spacecraft within the Arabia Terra low neutron flux anomaly (which is indicative of an anomalously high abundance of hydrogen: up to 16 wt % of the equivalent amount of water) was performed. Correlation between the enhanced abundance of eq…

2006 Solar System Research
MEx 4
Models of the protosatellite disk of Saturn: Conditions for Titan's formation
DOI: 10.1134/S0038094606060013 Bibcode: 2006SoSyR..40..441M

Dorofeeva, V. A.; Makalkin, A. B.

Models of the protosatellite accretion disk of Saturn are developed that satisfy cosmochemical constraints on the volatile abundances in the atmospheres of Saturn and Titan with due regard for the data obtained with the Cassini orbiter and the Huygens probe, which landed on Titan in January 2005. All basic sources of heating of the disk and protos…

2006 Solar System Research
Huygens 4
Morphology and geological structure of the western part of the Olympus Mons volcano on Mars from the analysis of the Mars Express HRSC imagery
DOI: 10.1007/s11208-005-0025-2 Bibcode: 2005SoSyR..39...85B

Jaumann, R.; Head, J. W.; Neukum, G. +8 more

The images of the western part of Olympus Mons and adjacent plains acquired by the HRSC camera onboard the Mars Express spacecraft were studied. The morphology, topography, and color of the surface were investigated. The surface age was determined by the frequencies of impact craters. The examination of the HRSC images combined with an analysis of…

2005 Solar System Research
MEx 26
The Surface Structure of the M-Type Asteroid 21 Lutetia: Spectral and Frequency Analysis
DOI: 10.1007/s11208-005-0052-z Bibcode: 2005SoSyR..39..410P

Prokof'eva, V. V.; Bochkov, V. V.; Busarev, V. V.

A preliminary study of the surface of the asteroid 21 Lutetia with ground-based methods is of significant importance, because this object is included into the Rosetta space mission schedule. From August 31 to November 20, 2000, about 50 spectra of Lutetia and the same number of spectra of the solar analog HD10307 (G2V) and regional standards were …

2005 Solar System Research
Rosetta 10
Spacecraft exploration of asteroids
DOI: 10.1007/s11208-005-0006-5 Bibcode: 2005SoSyR..39...73S

Shevchenko, V. G.; Mohamed, R. A.

The past, current, and planned space missions for asteroid exploration are reviewed. The main results based on observations performed with satellites in near-Earth orbits (OAO-2, IUE, FIRSSE, IRAS, HST, Hipparcos, ISO, MSX) and space probes sent to particular objects (Galileo, NEAR, DS1, Stardust) are reported. Future space missions (MUSES-C, Rose…

2005 Solar System Research
Rosetta eHST 2