Statements (67)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Photographer
gptkb:observatory |
| gptkbp:bfsLayer |
3
|
| gptkbp:bfsParent |
gptkb:Photographer
gptkb:Hubble_Space_Telescope gptkb:software gptkb:observatory |
| gptkbp:contributed_to |
astronomical research
|
| gptkbp:designed_by |
gptkb:NASA
|
| gptkbp:enhances |
Hubble's imaging capabilities
|
| gptkbp:features |
multi-wavelength imaging
multiple filters for different wavelengths |
| gptkbp:frequency |
200 nm to 2.5 µm
|
| gptkbp:has_ability |
UV, visible, and near-infrared observations
|
| gptkbp:has_symbol |
162 arcseconds by 162 arcseconds
|
| https://www.w3.org/2000/01/rdf-schema#label |
Wide Field Camera 3
|
| gptkbp:is_capable_of |
multi-band imaging
capturing images in ultraviolet, visible, and near-infrared light |
| gptkbp:is_equipped_with |
a wide variety of filters
|
| gptkbp:is_implemented_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:is_known_for |
its versatility in imaging modes
|
| gptkbp:is_part_of |
Hubble Space Telescope's instruments
|
| gptkbp:is_used_for |
gptkb:observatory
studying distant galaxies observing star formation examining exoplanets investigating cosmic phenomena |
| gptkbp:launch_date |
gptkb:2009
|
| gptkbp:launched |
May 2009
|
| gptkbp:lighting |
gptkb:2009
|
| gptkbp:operated_by |
gptkb:Space_Telescope_Science_Institute
|
| gptkbp:provides |
high-resolution imaging
|
| gptkbp:replaced_by |
gptkb:Wide_Field_Camera_2
|
| gptkbp:resolution |
up to 0.04 arcseconds
0.04 arcseconds |
| gptkbp:significance |
its contributions to the study of dark energy
its role in the discovery of exoplanets its contributions to the study of the structure of the universe its contributions to the understanding of galaxy formation its contributions to the study of the habitability of exoplanets its role in the observation of exoplanet atmospheres its role in the observation of gravitational lensing its contributions to the study of asteroid belts its contributions to the study of cosmic rays its contributions to the study of galaxy clusters its contributions to the study of meteor showers its contributions to the study of solar wind its contributions to the study of the heliosphere its contributions to the study of the solar system its role in the observation of comets its role in the observation of nebulae its role in the observation of quasars its role in the observation of solar flares its role in the observation of supernovae its role in the observation of the Milky Way its role in the observation of the cosmic web its role in the study of black holes its contributions to the study of cosmic microwave background radiation its contributions to the study of stellar evolution its role in the observation of the formation of stars. its role in the observation of magnetic fields in space its role in the observation of the interstellar medium its contributions to the study of the early universe its role in the observation of planetary atmospheres |
| gptkbp:successor |
gptkb:Wide_Field_Camera_2
|
| gptkbp:uses |
gptkb:Hubble_Space_Telescope
|
| gptkbp:viewpoint |
162 arcminutes
|