Statements (225)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:astronomy
|
| gptkbp:analysis |
gptkb:Kepler_Science_Operations_Center
gptkb:Kepler_pipeline Kepler Data Analysis Pipeline light curve plots statistical analysis of light curves light curve graphs |
| gptkbp:analytics |
gptkb:Kepler_Pipeline
Kepler Data Analysis Software Kepler Light Curve Generator |
| gptkbp:capacity |
over 500 terabytes
|
| gptkbp:collaboration |
gptkb:SETI_Institute
global research teams involved multiple countries |
| gptkbp:collaborations |
gptkb:NASA_Ames_Research_Center
international research teams universities and institutions collaborated with various observatories |
| gptkbp:collaborative_projects |
K2 mission
|
| gptkbp:collaborator |
gptkb:University_of_California
gptkb:SETI_Institute gptkb:Harvard-Smithsonian_Center_for_Astrophysics gptkb:NASA_Ames_Research_Center gptkb:Space_Telescope_Science_Institute international research teams various universities and research institutions |
| gptkbp:collection |
4 years
2009-2013 continuous monitoring transit method transit photometry |
| gptkbp:community |
gptkb:astronomy
astronomers worldwide astronomers and astrophysicists |
| gptkbp:community_engagement |
outreach programs
|
| gptkbp:community_outreach |
gptkb:educational_programs
public lectures and presentations |
| gptkbp:conference |
presentations and discussions
|
| gptkbp:contributed_to |
Kepler-186f discovery
Kepler-22b discovery |
| gptkbp:contribution |
understanding of planetary systems
enhanced understanding of planetary systems improved understanding of planetary systems |
| gptkbp:contribution_to_astrobiology |
identifying potentially habitable planets
|
| gptkbp:cooling_system |
passive thermal control system
|
| gptkbp:country |
gptkb:Kepler-22b
over 2,300 over 2,600 exoplanets |
| gptkbp:data_analysis_team |
Kepler Science Team
|
| gptkbp:data_type |
FITS
light curves |
| gptkbp:data_usage |
gptkb:exoplanet
gptkb:public_outreach gptkb:scientific_research educational purposes publicly available data public research projects |
| gptkbp:design |
3.5 years
|
| gptkbp:designed_by |
gptkb:NASA
|
| gptkbp:dimensions |
4.5 m x 2.7 m x 2.4 m
|
| gptkbp:discovered_by |
over 2,600 exoplanets
over 2,300 exoplanets |
| gptkbp:discovery |
gptkb:Kepler-186f
gptkb:Kepler-1649c gptkb:Kepler-16b gptkb:Kepler-22b gptkb:Kepler-186c gptkb:Kepler-90i gptkb:Kepler-20e gptkb:Kepler-452b transit method Kepler-11 system first Earth-size planet in habitable zone. diverse range of exoplanets |
| gptkbp:discovery_count |
over 2,300 exoplanets
|
| gptkbp:final_data_release |
gptkb:2019
|
| gptkbp:focus |
transiting exoplanets
|
| gptkbp:frequency |
X-band
S-band |
| gptkbp:funding |
gptkb:NASA's_Discovery_Program
$600 million NASA budget |
| gptkbp:future_prospects |
follow-up observations of exoplanets
|
| gptkbp:has_ability |
high precision photometry
|
| gptkbp:has_mission |
exoplanet discovery
|
| gptkbp:has_view_of |
115 square degrees
|
| gptkbp:historical_interpretation |
statistical methods
involves complex algorithms |
| gptkbp:historical_legacy |
foundation for future missions
|
| https://www.w3.org/2000/01/rdf-schema#label |
Kepler Space Telescope
|
| gptkbp:image_processing |
light curve analysis
automated algorithms Kepler Science Office |
| gptkbp:impact |
revolutionized exoplanet research
increased interest in exoplanet research influenced future exoplanet missions increased exoplanet detection rate enhanced understanding of solar systems revolutionized exoplanet studies |
| gptkbp:inspiration |
inspired public interest in astronomy
|
| gptkbp:instrument |
gptkb:radio_station
|
| gptkbp:instrumentation |
gptkb:radio_station
|
| gptkbp:instruments |
CCD detectors
|
| gptkbp:is_a |
gptkb:astronomy
|
| gptkbp:is_considered |
statistical validation methods
|
| gptkbp:is_observed_in |
stars
over 500,000 stars |
| gptkbp:launch_date |
gptkb:2009
March 7, 2009 |
| gptkbp:launch_mass |
1,000 kg
|
| gptkbp:launch_platform |
gptkb:United_Launch_Alliance
|
| gptkbp:launch_site |
gptkb:Cape_Canaveral_Air_Force_Station
|
| gptkbp:launch_vehicle |
gptkb:Delta_II_7920-10_L
gptkb:Delta_II_7920-10_C |
| gptkbp:launched |
gptkb:NASA
March 7, 2009 |
| gptkbp:legacy |
inspired future missions
pioneered exoplanet research |
| gptkbp:lighting |
May 2009
|
| gptkbp:located_in |
heliocentric orbit
|
| gptkbp:location |
gptkb:star
heliocentric orbit |
| gptkbp:mass |
1,000 kg
1,000 kilograms about 1,000 kg |
| gptkbp:mission |
gptkb:2018
gptkb:NASA_Ames_Research_Center November 2018 completed exoplanet discovery K2 mission identify habitable zones identify potential habitable planets |
| gptkbp:mission_duration |
4 years
approximately 9 years 3.5 years |
| gptkbp:mission_type |
exoplanet discovery
|
| gptkbp:named_after |
gptkb:Johannes_Kepler
|
| gptkbp:notable_achievements |
first Earth-size planet in habitable zone
|
| gptkbp:notable_exoplanet |
gptkb:Kepler-16b
gptkb:Kepler-22b gptkb:Kepler-452b |
| gptkbp:notable_feature |
high precision photometry
|
| gptkbp:notable_work |
gptkb:Kepler-186f
gptkb:Kepler-16b gptkb:Kepler-22b gptkb:Kepler-20e gptkb:Kepler-452b discovery of the Kepler-186f planet |
| gptkbp:observational_goals |
characterize exoplanet atmospheres
|
| gptkbp:observed_stars |
over 500,000
|
| gptkbp:observing_strategy |
continuous observation
|
| gptkbp:operated_by |
gptkb:NASA_Ames_Research_Center
gptkb:NASA |
| gptkbp:operates_in |
November 2018
|
| gptkbp:operational_challenges |
spacecraft anomalies
reaction wheel failures |
| gptkbp:operational_use |
gptkb:NASA
|
| gptkbp:orbit_type |
heliocentric orbit
|
| gptkbp:orbital_altitude |
647 kilometers
|
| gptkbp:orbital_inclination |
90 degrees
|
| gptkbp:orbital_period |
372 days
|
| gptkbp:planetary_candidates |
over 4,700 candidates identified
|
| gptkbp:power_source |
solar panels
|
| gptkbp:primary_mission |
gptkb:Kepler_Mission
gptkb:K2_Mission K2 mission |
| gptkbp:primary_use |
detect Earth-size planets
|
| gptkbp:product_quality |
high precision
|
| gptkbp:provides_information_on |
gptkb:Kepler_Data_Release_25
gptkb:Kepler_Pipeline gptkb:NASA_Exoplanet_Archive gptkb:Mikulski_Archive_for_Space_Telescopes publicly available open access policy Kepler Science Office open access to researchers detecting transits statistical analysis of planet occurrence |
| gptkbp:public_interest |
increased public awareness of space exploration
|
| gptkbp:publications |
over 1,000
numerous peer-reviewed articles hundreds of peer-reviewed papers Kepler Science Conference papers |
| gptkbp:release_frequency |
quarterly
|
| gptkbp:released |
gptkb:Kepler_Data_Release_25
publicly available multiple data releases |
| gptkbp:research |
4 years
2009-2013 transit method photometric measurements transit photometry field rotation long-term monitoring long-term monitoring of stars limited to a specific field of view brightness of stars long-duration monitoring 4 years of continuous observation differential photometry |
| gptkbp:resolution |
4 arcseconds
20 parts per million |
| gptkbp:retired |
gptkb:2018
|
| gptkbp:scientific_goals |
detect Earth-like planets
detect Earth-size planets identify Earth-like planets characterize the diversity of planetary systems detect Earth-sized planets |
| gptkbp:scientific_instruments |
gptkb:radio_station
CCD detectors CCD array |
| gptkbp:sensor |
CCD (Charge-Coupled Device)
|
| gptkbp:status |
retired
|
| gptkbp:storage |
onboard solid-state drives
|
| gptkbp:student_enrollment |
long-term storage
|
| gptkbp:successor |
gptkb:TESS
|
| gptkbp:team |
gptkb:William_Borucki
|
| gptkbp:total_exoplanets_confirmed |
over 2,300
|
| gptkbp:type |
gptkb:astronomy
|
| gptkbp:view |
115 square degrees
|
| gptkbp:bfsParent |
gptkb:The_National_Aeronautics_and_Space_Administration
gptkb:NASA_Ames_Research_Center gptkb:NASA |
| gptkbp:bfsLayer |
3
|