ICelestialBodyInformation#
- class ansys.stk.core.stkobjects.ICelestialBodyInformation#
The interface represents information associated with a celestial body.
Overview#
Return the last computed direction vector in ICRF. |
Johnson B-V color index. |
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Get a name of the star catalog. |
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Declination. Use the |
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Starβs effective temperature. Use the |
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Get the identification of the star as per star catalog. |
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Magnitude to irradiance conversion factor is not given directly in any catalog. This factor converts the Planck function radiance to a rescaled irradiance at Earthβs distance from the star. Unitless. |
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Trigonometric parallax. Use the |
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Right ascention. Use the |
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Radial velocity. |
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Visual magnitude. |
Import detail#
from ansys.stk.core.stkobjects import ICelestialBodyInformation
Property detail#
- property ICelestialBodyInformation.effective_temperature: float#
Starβs effective temperature. Use the
Temperature
dimension.
- property ICelestialBodyInformation.identifier: str#
Get the identification of the star as per star catalog.
- 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 Earthβs distance from the star. Unitless.
- property ICelestialBodyInformation.parallax: float#
Trigonometric parallax. Use the
Angle
dimension.
Method detail#
- ICelestialBodyInformation.get_last_computed_direction_in_icrf(self) ICartesian3Vector #
Return the last computed direction vector in ICRF.
- Returns:
ICartesian3Vector