Figure 10 from Possible Chemical Composition And Interior Structure Models Of Venus Inferred From Numerical Modelling

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Possible Chemical Composition And Interior Structure Models Of Venus Inferred From Numerical Modelling

Authors: Oliver Shah, Ravit Helled, Yann Alibert, and Klaus Mezger

2022 The Astrophysical Journal 926 217.

Provider: AAS Journals

Caption: Figure 10.

Estimated ranges of Venus’ MoI from Zhang & Zhang (1995), Aitta (2012), and Dumoulin et al. (2017) and the three different bulk compositions we consider. Measured values for the MoI for Earth, Venus, Mercury, and Mars are shown for comparison. The shaded region denotes the current uncertainty of Venus’ MoI from observations (Margot et al. 2021).

Other Images in This Article

Copyright and Terms & Conditions