Statements (54)
Predicate | Object |
---|---|
gptkbp:instanceOf |
space observatory
|
gptkbp:collaborations |
gptkb:University_of_Leicester
gptkb:University_of_California gptkb:Max_Planck_Institute_for_Extraterrestrial_Physics NASA |
gptkbp:dataUsage |
XMM-Newton_Science_Archive
|
gptkbp:fieldOfUse |
30 arcminutes
|
https://www.w3.org/2000/01/rdf-schema#label |
XMM-Newton satellite
|
gptkbp:instrument |
X-ray telescopes
|
gptkbp:launchDate |
December 10, 1999
|
gptkbp:launched |
gptkb:European_Space_Agency
|
gptkbp:location |
Earth_orbit
|
gptkbp:mission |
X-ray astronomy
low_Earth_orbit |
gptkbp:notableFeature |
study of the evolution of galaxies
study of the cosmic web study of the lifecycle of stars study of the formation of galaxies research on neutron stars examination of the effects of cosmic rays on star formation. analysis of the impact of supernovae on star formation study of the relationship between galaxies and their dark matter halos analysis of stellar populations in galaxies analysis of the chemical composition of stars detection of dark matter discovery of new black holes examination of the evolution of supernovae examination of the structure of the universe exploration of the cosmic microwave background investigation of active galactic nuclei investigation of the effects of dark energy investigation of the intergalactic medium investigation of the physics of black holes mapping of the hot gas in galaxy clusters observation of supermassive black holes research on the cosmic evolution of galaxies research on the properties of quasars study of cosmic X-ray background study of the dynamics of galaxy clusters study of the environment around black holes study of the interaction between galaxies and their environment investigation of the role of black holes in galaxy formation investigation of the role of magnetic fields in galaxy formation research on the formation of large-scale structures |
gptkbp:operationalStatus |
active
|
gptkbp:powers |
solar panels
|
gptkbp:primaryMission |
10 years
|
gptkbp:resolution |
0.5 arcseconds
|
gptkbp:scientificName |
study black holes
investigate supernova remnants observe galaxy clusters examine the hot gas in the universe |
gptkbp:type |
X-ray data
|
gptkbp:weight |
3,800 kg
|