Mars/Moon Cratering Rate Ratio Estimates

By B. Ivanov. 2001

610 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/885e279899a431758daffbd17815707b5fc0a576

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Citations in the corpus

The timing of martian valley network activity : Constraints from buffered crater counting (2008, methodology): “When we derive absolute ages in this contribution, we have chosen to apply two commonly used production functions: the Neukum production function (Neukum and Ivanov, 2001; Ivanov, 2001; see also Werner, 2005), and the 2004 iteration of the Hartmann production function (Hartmann, 2005).”
Map-projection-independent crater size-frequency determination in GIS environments—New software tool for ArcGIS (2011, methodology): “Theoretical modelling and observational data of fluxes of crater-forming impactors for different parts of our solar system made it possible to calibrate this lunar chronology function for different terrestrial planets and satellites (e.g., Neukum et al., 2001a; Ivanov, 2001; Hartmann and Neukum, 200”
THE IMPORTANCE OF SECONDARY CRATERING TO AGE CONSTRAINTS ON PLANETARY SURFACES (2006, background): “Average impact speeds for planet-crossing asteroids are ∼16 km s−1 on the Moon and ∼10 km s−1 on Mars (Ivanov 2001), whereas on Europa the cometary impact velocity averages ∼20 km s−1 (Zahnle et al. 1998).”
The early martian evolution—Constraints from basin formation ages (2008, methodology): “binations of crater size–frequency descriptions and chronology models (Neukum, 1983; Ivanov, 2001; Neukum et al., 2001).”
The global martian volcanic evolutionary history (2009, methodology): “The determination of absolute ages on Mars is based on the crater production function (Ivanov, 2001, originally in Neukum, 1983) and the applied chronology model (Hartmann and Neukum, 2001).”
Nonuniform cratering of the terrestrial planets (2008, background): “Nevertheless, as was pointed out by Ivanov (2001) , a modulation of the orbital distribution of Mars crossing objects with the evolution of the martian orbit is possible.”
Large-scale spring deposits on Mars? (2008, methodology): “Available cratering models have been used in order to obtain isochrones [Hartmann and Neukum, 2001; Ivanov, 2001]; a discussion on the errors in the method is provided by Neukum et al.”
Loss of water from Mars: Implications for the oxidation of the soil (2003, methodology): “Fig.”
The rayed crater Zunil and interpretations of small impact craters on Mars (2005, methodology): “We expect∼1 crater 10 km per 106 yrs on all of Mars(Ivanov, 2001), so Zunil may be less than a few (∼5) Ma old.”
Cataclysmic bombardment throughout the inner solar system 3.9–4.0 Ga (2002, background): “[18] The relative impact flux between the Moon and Mars is unity when scaled for surface area [Ivanov, 2001], implying at least 6400 craters with diameters 20 km were produced on Mars.”
Cratering History and Lunar Chronology (2006, background): “The shock wave generated by an impact weakens with decreasing impact angle (Pierazzo and Melosh 2000a; Artemieva and Ivanov 2001; Stöffler et al. 2002; Fig.”
Planetary surface dating from crater size–frequency distribution measurements: Spatial randomness and clustering (2012, background): “From then on, it accumulates craters, and the present age is determined from the crater population (e.g. Hartmann et al., 1981; Neukum and Hiller, 1981; Neukum, 1983; Neukum and Ivanov, 1995; Hartmann and Neukum, 2001; Ivanov, 2001).”
Cratering Chronology and the Evolution of Mars (2001, result): “Keszthelyi et al. (2000) confirmed unusually fresh-appearing lava textures, similar to examples of flood basalts found in Iceland. Hartmann and Berman (2000) derived an age of a few Myr to 100 Myr from crater counts.”