Redefinition of the crater-density and absolute-age boundaries for the chronostratigraphic system of Mars

By S. Werner, K. Tanaka. 2011

144 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/20798339d2d4d4bee5755e62a3fe4a2b0ad48e40

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. S. Byrne
2. A. S. McEwen
3. Nicolas Mangold
4. Ingrid Daubar
5. C. Dundas
6. M. Kennedy
7. B. Ivanov
8. S. Conway

In Atmospheric Science

1. B. Ivanov
2. S. Byrne
3. Nicolas Mangold
4. C. Dundas
5. A. S. McEwen
6. M. Kennedy
7. Ingrid Daubar

Citations in the corpus

• A chronology of early Mars climatic evolution from impact crater degradation (2012, background): “06 Gy, an age corresponding to the middle of the Early Hesperian period in this model age system [Ivanov, 2001; Werner and Tanaka, 2011].”
• The current martian cratering rate (2010, methodology): “We use the chronology function from Hartmann (2005) as derived in Werner and Tanaka (2011): N(D P 1 km) = 4.4246 !”
• Sequence of infilling events in Gale Crater, Mars: Results from morphology, stratigraphy, and mineralogy (2013, unknown): “Taking into account that the Late Noachian is ranging from 3.85Ga to 3.57Ga [Hartmann, 2005; Werner and Tanaka, 2011] and the uncertainties of the measurement, we estimate the age of the Gale impact to range between ~3.55Ga and ~3.65Ga and hence to be Late Noachian/Early Hesperian.”