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gptkbp:instance_of
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gptkb:star
|
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gptkbp:apparent_magnitude
|
5.25
approximately 4.5
|
|
gptkbp:average_temperature
|
approximately 9,000 K
|
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gptkbp:controls
|
gptkb:theorem
|
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gptkbp:depicted_in
|
gptkb:theorem
|
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gptkbp:distance
|
approximately 100 light years
|
|
gptkbp:has_spectral_type
|
gptkb:A0_V
B-type main-sequence star
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|
https://www.w3.org/2000/01/rdf-schema#label
|
Lambda Herculis B
|
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gptkbp:is_a_source_of
|
visible light
|
|
gptkbp:is_analyzed_in
|
its spectral lines
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gptkbp:is_approximately
|
2.5 times the mass of the Sun
|
|
gptkbp:is_involved_in
|
stellar interactions
|
|
gptkbp:is_known_for
|
its stability
|
|
gptkbp:is_often_compared_to
|
other A-type stars
|
|
gptkbp:is_part_of
|
gptkb:Lambda_Herculis_system
multiple star system
the local stellar neighborhood
the spectral class A
the binary star classification
|
|
gptkbp:located_in
|
constellation Hercules
|
|
gptkbp:members
|
the Milky Way's stellar population
|
|
gptkbp:orbital_period
|
about 5.5 days
|
|
gptkbp:scientific_classification
|
a white star
|
|
gptkbp:targets
|
stellar spectroscopy
|
|
gptkbp:type_of
|
gptkb:star
|
|
gptkbp:bfsParent
|
gptkb:mythological_figure
|
|
gptkbp:bfsLayer
|
3
|