`quantitykind:EccentricityOfOrbit`

http://qudt.org/vocab/quantitykind/EccentricityOfOrbit

Predicate	Object
`rdf:type`	`qudt:QuantityKind`
`dcterms:description`	“The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle. In a two-body problem with inverse-square-law force, every orbit is a Kepler orbit. The eccentricity of this Kepler orbit is a positive number that defines its shape.”
`qudt:applicableUnit`	Show 15 values `unit:FRACTION` `unit:GR` `unit:NUM` `unit:ONE-PER-ONE` `unit:PERCENT` `unit:PERMILLE` `unit:PERMITTIVITY_REL` `unit:PPB` `unit:PPM` `unit:PPQ` `unit:PPT` `unit:PPTH` `unit:PPTM` `unit:PSU` `unit:UNITLESS`
`qudt:hasDimensionVector`	`qkdv:A0E0L0I0M0H0T0D1`
`qudt:latexSymbol`	\(\varepsilon\)
`qudt:plainTextDescription`	“The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle. In a two-body problem with inverse-square-law force, every orbit is a Kepler orbit. The eccentricity of this Kepler orbit is a positive number that defines its shape.”
`rdfs:comment`	“Applicable units are those of quantitykind:DimensionlessRatio”
`rdfs:isDefinedBy`	http://qudt.org/3.2.0/vocab/quantitykind
`rdfs:label`	“Eccentricity Of Orbit”@en
`skos:broader`	`quantitykind:DimensionlessRatio`

Generated 2026-03-25T09:17:53.599-04:00