ICelestialBodyInformation#

class ansys.stk.core.stkobjects.ICelestialBodyInformation#: The interface represents information associated with a celestial body.

Overview#

Methods

Return the last computed direction vector in ICRF.

Properties

`identifier`	Get the identification of the star as per star catalog.
`catalog_name`	Get a name of the star catalog.
`right_ascension`	Right ascention. Use the `Angle` dimension.
`declination`	Declination. Use the `Angle` dimension.
`parallax`	Trigonometric parallax. Use the `Angle` dimension.
`velocity`	Radial velocity.
`visual_magnitude`	Visual magnitude.
`b_minus_v`	Johnson B-V color index.
`effective_temperature`	Star’s effective temperature. Use the `Temperature` dimension.
`magnitude_to_irradiance_conversion_factor`	Magnitude to irradiance conversion factor is not given directly in any catalog. This factor converts the Planck function radiance to a rescaled irradiance at Earth’s distance from the star. Unitless.

from ansys.stk.core.stkobjects import ICelestialBodyInformation

property ICelestialBodyInformation.identifier: str#: Get the identification of the star as per star catalog.

property ICelestialBodyInformation.catalog_name: str#: Get a name of the star catalog.

property ICelestialBodyInformation.right_ascension: float#: Right ascention. Use the Angle dimension.

property ICelestialBodyInformation.declination: float#: Declination. Use the Angle dimension.

property ICelestialBodyInformation.parallax: float#: Trigonometric parallax. Use the Angle dimension.

property ICelestialBodyInformation.visual_magnitude: float#: Visual magnitude.

property ICelestialBodyInformation.b_minus_v: float#: Johnson B-V color index.

property ICelestialBodyInformation.effective_temperature: float#: Star’s effective temperature. Use the Temperature dimension.

property ICelestialBodyInformation.magnitude_to_irradiance_conversion_factor: float#: Magnitude to irradiance conversion factor is not given directly in any catalog. This factor converts the Planck function radiance to a rescaled irradiance at Earth’s distance from the star. Unitless.

ICelestialBodyInformation.get_last_computed_direction_in_icrf(self) → ICartesian3Vector#

Return the last computed direction vector in ICRF.