RR Lyrae Stars

GPTKB entity

Statements (45)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:bfsLayer 3
gptkbp:bfsParent gptkb:star
gptkbp:adaptation from main sequence to horizontal branch
gptkbp:age approximately 10 billion years
gptkbp:application stellar evolution and galactic dynamics
gptkbp:associated_with gptkb:Type_I_Cepheid_variables
gptkbp:average_temperature around 5,000 to 7,500 K
gptkbp:color yellow to orange
gptkbp:contains gptkb:Type_II_Cepheid_variables
gptkbp:contributed_to cosmological distance ladder
gptkbp:contribution understanding of stellar populations
gptkbp:discovered_by 1901
the constellation Lyra
gptkbp:distribution found in the halo of the Milky Way
gptkbp:example RR Lyrae, XZ Cygni, and V1 in M3
gptkbp:features strong hydrogen lines
gptkbp:has_color B-V index around 0.3 to 0.5
gptkbp:has_luminosity approximately 100 times that of the Sun
gptkbp:has_spectral_type A to F type
gptkbp:has_variants radial pulsation
gptkbp:historical_period typically 0.5 to 1 day
gptkbp:historical_significance first standard candles for distance measurement
https://www.w3.org/2000/01/rdf-schema#label RR Lyrae Stars
gptkbp:instrument 0.3 to 2.0 magnitudes
gptkbp:is_found_in globular clusters
gptkbp:is_observed_in amateur astronomers
various galaxies
gptkbp:is_used_for distance measurement in astronomy
gptkbp:lighting due to pulsation
characteristic sawtooth shape
approximately 10 to 16 magnitude
periodic and regular
gptkbp:mass 0.5 to 1.0 solar masses
gptkbp:metallicity typically low metallicity
gptkbp:mode fundamental and first overtone modes
gptkbp:named_after gptkb:RR_Lyrae
gptkbp:notable_traits short pulsation periods and low metallicity
gptkbp:origin horizontal branch stars
gptkbp:photography Johnson and Cousins systems
gptkbp:range up to 100,000 light-years
gptkbp:research photometry and spectroscopy
faintness and variability
gptkbp:strategic_importance stellar population studies
gptkbp:type pulsating variable star