Statements (76)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:exoplanet
|
| gptkbp:apparent_magnitude |
gptkb:12.5
|
| gptkbp:atmosphere |
hydrogen and helium
hydrogen-rich atmosphere contains sodium and potassium. may have clouds. |
| gptkbp:availability |
data available in exoplanet databases.
|
| gptkbp:average_temperature |
approximately 1500 K
|
| gptkbp:collaborations |
involves international collaborations.
|
| gptkbp:collection |
ongoing data collection efforts.
|
| gptkbp:community |
actively studied by the research community.
|
| gptkbp:contains_star |
gptkb:Milky_Way
G-type main-sequence star. |
| gptkbp:contribution |
contributes to our understanding of planetary systems.
|
| gptkbp:country |
formed in a gaseous disk.
part of the HAT-P-22 system. |
| gptkbp:declination |
+30° 12' 00''
|
| gptkbp:discovered_by |
HATNet
HATNet Project |
| gptkbp:discovery |
transit method
G. W. Henry et al. |
| gptkbp:discovery_year |
gptkb:2010
gptkb:2011 |
| gptkbp:distance_from_earth |
approximately 124 light-years.
|
| gptkbp:eccentricity |
0.0
0.0 indicates a circular orbit. |
| gptkbp:exoplanet_catalog |
listed in various exoplanet catalogs.
|
| gptkbp:exoplanet_research |
important for understanding exoplanets.
|
| gptkbp:exoplanetary_science |
contributes to exoplanetary science.
|
| gptkbp:future_prospects |
promises further discoveries.
|
| gptkbp:growth_habit |
not habitable.
|
| gptkbp:has_luminosity |
interacts with its host star.
exists in a dynamic stellar environment. |
| gptkbp:has_radius |
1.1 times the radius of Jupiter
1.2 times the radius of Jupiter |
| gptkbp:hosts |
HAT-P-22
|
| https://www.w3.org/2000/01/rdf-schema#label |
HAT-P-22 b
|
| gptkbp:is_explored_in |
subject of planetary exploration missions.
|
| gptkbp:lighting |
observed light curve shows transits.
shows variability during transits. used to determine size and orbit. |
| gptkbp:location |
constellation Pegasus
|
| gptkbp:mass |
1.5 times the mass of Jupiter
0.5 times the mass of Jupiter 1.1 times the mass of the Sun. 1.1 times the radius of the Sun. more massive than Earth. significantly larger than Earth. |
| gptkbp:migration |
likely migrated inward.
|
| gptkbp:next_event |
planned for further study.
|
| gptkbp:notable_galaxies |
1.2-meter telescope.
|
| gptkbp:observational_programs |
part of various observational programs.
|
| gptkbp:orbital_altitude |
subject to gravitational influences.
|
| gptkbp:orbital_inclination |
88.5 degrees
close to edge-on. |
| gptkbp:orbital_period |
3.2 days
not in orbital resonance. |
| gptkbp:planetary_characteristics |
characterized by high temperatures.
|
| gptkbp:publications |
numerous scientific papers published.
|
| gptkbp:research |
collected by multiple observatories.
difficult to observe due to brightness. requires advanced telescopes. |
| gptkbp:research_importance |
important for studying hot Jupiters.
|
| gptkbp:research_interest |
of great interest to astronomers.
|
| gptkbp:right_ascension |
00h 22m 36.0s
|
| gptkbp:semi_major_axis |
0.045 AU
|
| gptkbp:spectroscopic_data |
obtained from follow-up spectroscopy.
|
| gptkbp:spectroscopy_techniques |
used to analyze atmospheric composition.
|
| gptkbp:storage |
obtained from ground-based observations.
|
| gptkbp:surface |
higher than Earth's surface gravity.
|
| gptkbp:transit_frequency |
transits occur regularly.
|
| gptkbp:transmission |
approximately 1.5%.
|
| gptkbp:type |
gptkb:hot_Jupiter
|
| gptkbp:yearly_orbit |
completes an orbit around its star in 3.2 days.
|
| gptkbp:yearly_temperature |
high due to proximity to host star.
|
| gptkbp:yearly_variation |
0.1%
|