Rapid decrease in Martian crustal magnetization in the Noachian era: Implications for the dynamo and climate of early Mars
By R. Lillis, Herbert Frey, M. Manga. 2008
144 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/c8af56cb66d02627a05f09041031fe5583ae0f81
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In Astronomy and Astrophysics
- Stuart J. Robbins
- B. Hynek
- R. Lillis
- James W. Head III
- William Bottke
- Caleb I. Fassett
- Nicolas Mangold
- V. Ansan
Citations in the corpus
- Ages of very large impact basins on Mars: Implications for the late heavy bombardment in the inner solar system (2008, background): “As discussed in a companion paper [Lillis et al., 2008] basins with N(300) > 4 have strong magnetic signatures, those with N(300) 2 have no magnetic signatures, and those in the middle age range show a sharply decreasing intensity of magnetic intensity with decreasing age.”
- A chronology of early Mars climatic evolution from impact crater degradation (2012, background): “The very different magnetic signatures of basins larger than 1000 km and similar in age led to the conclusion that the Martian dynamo stopped at 4.1 Ga [Lillis et al., 2008].”
- The MAVEN Magnetic Field Investigation (2015, result): “This 103 view has been supported by more complete analyses of the large impact basins [Lillis et al., 2008; Lillis 104 et al., 2013], leading to more precise estimates of the dynamo’s demise.”
- Large impact crater histories of Mars: The effect of different model crater age techniques (2013, background): “Ladon is unambiguou sly magnetized (|B|185km = 42 nT), as shown by Lillis et al. (2008b), where the t the ages for both the Hartmann (2005) and Neukum et al. (2001) isochron systems basin (see Section 5.1, and Lillis et al. (2008a)), indicating that the magnetic field of dashed line in both frames…”
- Sequence and timing of conditions on early Mars (2011, background): “More recently, Frey (2008) and Lillis et al. (2008a) suggested that the combined population of possible QCDs and CTAs may provide the best data for considering the age of the largest basins (using features of 300 km and more in diameter).”