Construct · 1 fields · 1 citations

Tisserand parameter: a standalone construct

One name. One construct. A landmark on the map.

● anchor · a standalone construct Nearest construct by meaning·not indexed
Tisserandparameter1 CONSTRUCTTisserand parameterMURRAY · PLANETARY SCIENCE

A single standalone construct; nearby constructs are located against it in the Collider. Tap a field for its definition, unit, and measures.

Planetary science

a near-conserved combination of orbital elements in the restricted three-body problem, used to identify comets and classify small-body orbits.

In planetary science, Tisserand parameter refers to a near-conserved combination of orbital elements in the restricted three-body problem, used to identify comets and classify small-body orbits. This meaning comes from Murray (2000) in Solar System Dynamics.[1]

Unit
Recovery means
Measured by

Next

Run it through the Collider, or take the citations with you.

See how Tisserand parameter sits against neighbouring constructs in the Collider, or export every reference on this page in one click.

Open in ColliderExport BibTeXReport this entry

Nearby constructs

circular restricted three-body problem1 fields · 1 citationsanchor · a standalone constructcombination1 fields · 2 citationsanchor · a standalone constructdynamics3 fields · 3 citationsjingle · one word, three constructs

References

  1. Murray, C. D., & Dermott, S. F. (2000). Solar System Dynamics. Cambridge University Press. https://doi.org/10.1017/cbo9781139174817

Cited on this page?

Confirm your construct, or correct us.

If your work is cited behind one of these entries, you know better than we do whether we captured the meaning right. Confirm it, suggest an edit, or dispute it, and your name goes on the entry as an author who has checked it, linked to your ORCID.

Claim your construct