Multiple viable spin period solutions for Apophis all converge on the same pre-encounter orientation in 2029, supporting a high likelihood that its short-axis spin mode persists after the close approach.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.EP 2roles
background 1polarities
background 1representative citing papers
A white paper outlining approaches, software tools, and infrastructure needs for maximizing solar system science with the LSST survey.
citing papers explorer
-
The spin state of asteroid Apophis and a prediction of its change during the 2029 close encounter with Earth
Multiple viable spin period solutions for Apophis all converge on the same pre-encounter orientation in 2029, supporting a high likelihood that its short-axis spin mode persists after the close approach.
-
Maximizing LSST Solar System Science: Approaches, Software Tools, and Infrastructure Needs
A white paper outlining approaches, software tools, and infrastructure needs for maximizing solar system science with the LSST survey.