Hitomi (ASTRO-H)

E384066

Hitomi (ASTRO-H) was a Japanese X-ray astronomy satellite designed to study high-energy phenomena in the universe, such as black holes, galaxy clusters, and supernova remnants.

All labels observed (3)

How this entity was disambiguated

Statements (49)

Predicate Object
instanceOf Japanese spacecraft
X-ray astronomy satellite
artificial satellite
space telescope
abbreviation ASTRO-H
linked to: Hitomi (ASTRO-H)
alsoKnownAs Hitomi
cosparId 2016-012A
countryOfOrigin Japan
demonstratedCapability high-resolution X-ray spectroscopy
developedBy JAXA
developedInCollaborationWith Canadian Space Agency
ESA
NASA
endOfMission 2016-04-28
equippedWith Hard X-ray Imager
linked to: Hard X-ray Detector

Soft Gamma-ray Detector
Soft X-ray Imager
Soft X-ray Spectrometer
linked to: X-ray Spectrometer
failureCause attitude control anomaly
spacecraft breakup
failureDate 2016-03-26
inclination 31 degrees
launchCountry Japan
launchDate 2016-02-17
launchSite Tanegashima Space Center
launchVehicle H-IIA 202
missionType X-ray astronomy
astrophysics observatory
nameMeaning pupil of the eye in Japanese
notableResult high-resolution X-ray spectroscopy of the Perseus cluster
operator Japan Aerospace Exploration Agency
orbitType low Earth orbit
predecessor Suzaku (ASTRO-E2)
primaryObjective study high-energy phenomena in the universe
program JAXA ASTRO series
researchField X-ray astronomy
high-energy astrophysics
spaceAgency JAXA
spectralRange hard X-ray band
soft X-ray band
soft gamma-ray band
status mission failed
studies active galactic nuclei
black holes
cosmic plasmas
galaxy clusters
large-scale structure of the universe
supernova remnants
successor XRISM

How these facts were elicited

Referenced by (3)

Full triples — surface form annotated when it differs from this entity's canonical label.

Suzaku partOfProgram Astro series of Japanese X-ray astronomy satellites
linked to: Hitomi (ASTRO-H)
Hitomi (ASTRO-H) abbreviation ASTRO-H
linked to: Hitomi (ASTRO-H)