gptkbp:instance_of
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gptkb:star
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gptkbp:can_be_used_to
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determine distances in the universe
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gptkbp:characterized_by
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periodic brightness changes
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gptkbp:example
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gptkb:Mira_(Omicron_Ceti)
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gptkbp:exhibits
|
pulsation modes
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gptkbp:has_brightness_range
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magnitude 2 to 10
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gptkbp:has_spectral_type
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M7 to M9
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https://www.w3.org/2000/01/rdf-schema#label
|
Mira-type variable star
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gptkbp:is_found_in
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gptkb:the_Milky_Way_galaxy
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gptkbp:is_known_for
|
its variability in brightness
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gptkbp:is_located_in
|
constellation Cetus
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gptkbp:is_observed_in
|
amateur astronomers
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gptkbp:is_often_associated_with
|
red giants
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gptkbp:is_part_of
|
the class of long-period variable stars
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gptkbp:is_related_to
|
gptkb:Cepheid_variables
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gptkbp:is_studied_in
|
astrophysics
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gptkbp:named_after
|
the star Mira (Omicron Ceti)
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gptkbp:period
|
approximately 331 days
|
gptkbp:bfsParent
|
gptkb:R_Cygni
gptkb:S_Cygni
gptkb:T_Cygni
gptkb:U_Cygni
gptkb:V_Cygni
gptkb:V_Hydrae
gptkb:R_Herculis
gptkb:S_Herculis
gptkb:T_Herculis
gptkb:V_Herculis
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gptkbp:bfsLayer
|
6
|