Statements (57)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:exoplanet
|
| gptkbp:atmosphere |
gptkb:unknown
not confirmed potentially hydrogen-rich |
| gptkbp:availability |
publicly available through NASA archives
|
| gptkbp:average_temperature |
high due to proximity to host star
|
| gptkbp:comparison_with_other_planets |
compared to other hot Jupiters.
|
| gptkbp:contains_star |
G-type star
|
| gptkbp:country |
gptkb:Giant
gptkb:Kepler-24_system likely formed in situ |
| gptkbp:discovered_by |
gptkb:Kepler_Space_Telescope
|
| gptkbp:discovery |
gptkb:NASA_Ames_Research_Center
transit method |
| gptkbp:discovery_year |
gptkb:2010
|
| gptkbp:distance_from_earth |
approximately 1,200 light years
|
| gptkbp:eccentricity |
low
|
| gptkbp:exoplanet_catalog |
listed in NASA's exoplanet archive
|
| gptkbp:first_appearance |
gptkb:2009
|
| gptkbp:growth_habit |
not likely due to extreme conditions
|
| gptkbp:has_radius |
approximately 1.5 times that of Earth
|
| gptkbp:hosts |
gptkb:Kepler-24
|
| https://www.w3.org/2000/01/rdf-schema#label |
Kepler-24b
|
| gptkbp:last_appearance |
gptkb:2013
|
| gptkbp:lighting |
analyzed for transit events
minimal due to distance from Earth |
| gptkbp:mass |
1.1 times that of the Sun
1.2 times that of the Sun approximately 2.5 times that of Earth between 1 and 10 Jupiter masses |
| gptkbp:metallicity |
similar to solar metallicity
|
| gptkbp:module |
about 0.1 days
|
| gptkbp:next_event |
planned for atmospheric study
|
| gptkbp:orbital_altitude |
very close to its star
complex due to host star's gravity |
| gptkbp:orbital_inclination |
approximately 88 degrees
|
| gptkbp:orbital_period |
not in resonance with other planets
0.65 days possible due to close orbit |
| gptkbp:planetary_migration |
theory suggests inward migration
|
| gptkbp:potential_for_moons |
gptkb:unknown
|
| gptkbp:publications |
numerous studies published on its characteristics
|
| gptkbp:research |
high brightness of host star
collected by Kepler mission photometry used for detection |
| gptkbp:research_importance |
helps understand hot Jupiter formation
|
| gptkbp:research_interest |
high among exoplanet scientists
|
| gptkbp:rotation_period |
gptkb:unknown
|
| gptkbp:semi_major_axis |
0.015 AU
|
| gptkbp:spectroscopic_analysis |
not yet conducted
|
| gptkbp:surface |
higher than Earth's
|
| gptkbp:system |
approximately 4 billion years
|
| gptkbp:transmission |
gptkb:significant
|
| gptkbp:type |
gptkb:hot_Jupiter
|
| gptkbp:year |
less than one Earth day
|
| gptkbp:bfsParent |
gptkb:Kepler_mission
|
| gptkbp:bfsLayer |
4
|