|
gptkbp:instanceOf
|
Astronomical Object
|
|
gptkbp:canBe
|
Isolated
Binary System Member
Cooler than Stars
Ejected from Star System
Free-floating
Hotter than Planets
Older than Planets
Younger than Stars
|
|
gptkbp:canBurn
|
gptkb:Deuterium
|
|
gptkbp:cannotBurn
|
gptkb:Hydrogen
|
|
gptkbp:canOrbit
|
gptkb:star
|
|
gptkbp:canSustain
|
Deuterium Fusion
|
|
gptkbp:compatibleWith
|
concert hall
Main Sequence Star
|
|
gptkbp:composition
|
gptkb:Hydrogen
gptkb:Helium
Metals
|
|
gptkbp:discoveredBy
|
1995
|
|
gptkbp:doesNotSustain
|
Hydrogen Fusion
|
|
gptkbp:emits
|
Radio Waves
Infrared Radiation
|
|
gptkbp:firstConfirmed
|
gptkb:Teide_1
|
|
gptkbp:form
|
From Disk Instability
From Molecular Cloud
|
|
gptkbp:foundIn
|
gptkb:Milky_Way
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Brown Dwarf
|
|
gptkbp:mayInclude
|
gptkb:Atmosphere
gptkb:Lithium
gptkb:Magnetic_Field
gptkb:Storms
Clouds
Weather
Companions
Ammonia in Atmosphere
Cloud Bands
Methane in Atmosphere
Water Vapor in Atmosphere
|
|
gptkbp:range
|
13 to 80 Jupiter Masses
|
|
gptkbp:sometimesCalled
|
Failed Star
|
|
gptkbp:spectralType
|
L
M
T
Y
|
|
gptkbp:studiedBy
|
gptkb:Infrared_Telescopes
Astronomers
|
|
gptkbp:subclassOf
|
Substellar Object
|
|
gptkbp:temperature
|
~250 to 2500 Kelvin
|
|
gptkbp:bfsParent
|
gptkb:K.D._Miller
|
|
gptkbp:bfsLayer
|
6
|