Statements (185)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:spacecraft
gptkb:observatory |
| gptkbp:bfsLayer |
3
|
| gptkbp:bfsParent |
gptkb:NASA
|
| gptkbp:aims_to |
find exoplanets around bright stars
|
| gptkbp:analysis |
interactive tools
software packages citizen science performed by the TESS Science Team |
| gptkbp:collaborates_with |
ground-based observatories
|
| gptkbp:collaborations |
gptkb:spacecraft
gptkb:Harvard-Smithsonian_Center_for_Astrophysics gptkb:MIT gptkb:NASA's_Goddard_Space_Flight_Center gptkb:NASA's_Exoplanet_Exploration_Program various universities global research community international astronomers multi-wavelength studies global observatories TESS Follow-up Observing Program |
| gptkbp:collection |
continuous monitoring
|
| gptkbp:committee |
expert panel
|
| gptkbp:communication |
gptkb:physicist
to Earth to Earth via the Tracking and Data Relay Satellite System |
| gptkbp:community |
gptkb:observatory
exoplanet researchers |
| gptkbp:community_engagement |
outreach programs
|
| gptkbp:community_involvement |
citizen science projects
|
| gptkbp:contributed_to |
the study of planetary atmospheres
|
| gptkbp:contribution |
exoplanet science
|
| gptkbp:data_privacy |
open data policy
|
| gptkbp:data_type |
FITS
light curves |
| gptkbp:data_usage |
research and education
every 30 days NASA's MIT |
| gptkbp:discovered_by |
over 200
over 2,000 candidate exoplanets TESS Object of Interest (TOI) list numerous exoplanets |
| gptkbp:elevation |
350 km
approximately 108,000 kilometers |
| gptkbp:events |
ground-based telescopes
|
| gptkbp:filming_location |
gptkb:theorem
|
| gptkbp:filmography |
gptkb:4
|
| gptkbp:focus |
nearby stars
|
| gptkbp:focuses_on |
nearby stars
|
| gptkbp:frequency |
every 3 months
|
| gptkbp:full_name |
gptkb:Transiting_Exoplanet_Survey_Satellite
|
| gptkbp:future_plans |
extended mission
|
| gptkbp:has |
four wide-field cameras
|
| gptkbp:has_ability |
high precision photometry
|
| gptkbp:has_expansion |
over 2,000
|
| gptkbp:has_feature |
automated
|
| gptkbp:has_impact_on |
exoplanet science
|
| gptkbp:has_mission |
high
multidisciplinary science operations regularly published |
| gptkbp:has_programs |
TESS Follow-up Observing Program
|
| gptkbp:has_symbol |
24 degrees
|
| gptkbp:has_website |
light curve analysis
available for researchers |
| https://www.w3.org/2000/01/rdf-schema#label |
TESS
|
| gptkbp:image |
gptkb:NASA's_Ames_Research_Center
automated pipelines |
| gptkbp:impact |
gptkb:significant
high global research enhanced understanding of planetary systems |
| gptkbp:instrument |
gptkb:Photographer
photometers photometric sensors high-precision photometers |
| gptkbp:is_a_resource_for |
available online
workshops and seminars |
| gptkbp:is_designed_to |
identify Earth-sized planets
|
| gptkbp:is_equipped_with |
a star tracker
|
| gptkbp:is_evaluated_by |
peer review
|
| gptkbp:is_expected_to |
hundreds of Earth-like planets
|
| gptkbp:is_observed_in |
northern hemisphere
southern hemisphere ground-based telescopes transiting exoplanets transit photometry focuses on nearby stars. more than 200,000 stars the southern and northern hemispheres transiting exoplanets around bright stars |
| gptkbp:is_part_of |
gptkb:NASA's_Explorers_Program
gptkb:NASA's_Exoplanet_Exploration_Program exoplanet exploration NASA's mission portfolio |
| gptkbp:is_recognized_for |
discovering new exoplanets
|
| gptkbp:is_reflected_in |
10 centimeters
|
| gptkbp:is_supported_by |
gptkb:NASA's_Astrophysics_Division
NASA's funding |
| gptkbp:is_utilized_in |
astronomers worldwide
|
| gptkbp:key |
gptkb:NASA's_Exoplanet_Exploration_Program
|
| gptkbp:launch_date |
April 18, 2018
|
| gptkbp:launch_site |
gptkb:Cape_Canaveral_Space_Force_Station
|
| gptkbp:launch_vehicle |
gptkb:bird
|
| gptkbp:launched |
gptkb:Space_X_Falcon_9_rocket
gptkb:NASA April 18, 2018 |
| gptkbp:legacy |
foundation for future missions
|
| gptkbp:lighting |
time series data
May 2018 July 25, 2018 automated algorithms |
| gptkbp:located_in |
gptkb:MIT
|
| gptkbp:media_coverage |
full sky
|
| gptkbp:mission |
gptkb:Kepler's_discoveries
gptkb:2020 approved exoplanet discovery highly successful exoplanet survey highly elliptical identify habitable zones study stellar variability |
| gptkbp:mission_duration |
2 years
two years |
| gptkbp:monitors |
the brightness of stars
|
| gptkbp:named_after |
gptkb:Transiting_Exoplanet_Survey_Satellite
the TESS acronym |
| gptkbp:objective |
discover exoplanets
detect exoplanets detect transiting exoplanets |
| gptkbp:operated_by |
gptkb:MIT
gptkb:NASA |
| gptkbp:operates_in |
the visible light spectrum
|
| gptkbp:operational_status |
active
2022 or beyond |
| gptkbp:orbital_period |
gptkb:television_series
over 5000 atmospheric studies 13.7 days |
| gptkbp:part_of |
gptkb:NASA's_Explorers_Program
understand the prevalence of life in the universe |
| gptkbp:partnerships |
international collaborations
|
| gptkbp:primary_source |
search for exoplanets
|
| gptkbp:products |
gptkb:James_Webb_Space_Telescope
high fidelity |
| gptkbp:provides |
light curves for stars
|
| gptkbp:provides_information_on |
gptkb:Research_Institute
open access transit method NASA's archive |
| gptkbp:publishes |
gptkb:academic_journal
gptkb:Research_Institute numerous numerous papers |
| gptkbp:receives_funding_from |
gptkb:NASA's_Astrophysics_Division
NASA budget |
| gptkbp:recognizes |
light curves
|
| gptkbp:reign_end |
13.7 days
|
| gptkbp:released |
gptkb:football_club
public access open access publicly available occurs every few months |
| gptkbp:research |
new discoveries
transit method photometric measurements new insights into planet formation two-year survey brightness of stars |
| gptkbp:resolution |
high
|
| gptkbp:scientific_goals |
characterize exoplanets
George R. Ricker |
| gptkbp:successor |
gptkb:Kepler_space_telescope
gptkb:Kepler |
| gptkbp:targets |
200,000
bright stars over 200,000 stars |
| gptkbp:team |
scientists and engineers
|
| gptkbp:technology |
advanced optics
|
| gptkbp:uses |
photometry
transit photometry high-precision photometry |
| gptkbp:viewpoint |
24 degrees
24 degrees by 24 degrees |