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RS Comae Berenices

RR Lyrae variable star in the constellation Coma Berenices
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RS Comae Berenices

Summary

RS Comae Berenices is a RR Lyrae variable[1].

Key Facts

  • RS Comae Berenices's instance of is recorded as RR Lyrae variable[2].
  • RS Comae Berenices's constellation is recorded as Coma Berenices[3].
  • RS Comae Berenices's catalog code is recorded as [SHM2017] J198.66493+17.19691[4].
  • RS Comae Berenices's catalog code is recorded as RS Com[5].
  • RS Comae Berenices's catalog code is recorded as 2MASS J13143959+1711492[6].
  • RS Comae Berenices's catalog code is recorded as LINEAR 8680084[7].
  • RS Comae Berenices's catalog code is recorded as SDSS J131439.57+171148.7[8].
  • RS Comae Berenices's catalog code is recorded as [DCD2013] CSS J131439.5+171148[9].
  • RS Comae Berenices's catalog code is recorded as Gaia DR2 3936953979146081792[10].
  • RS Comae Berenices's catalog code is recorded as TIC 282783705[11].
  • RS Comae Berenices's catalog code is recorded as ATO J198.6649+17.1968[12].
  • RS Comae Berenices's type of variable star is recorded as RR Lyrae variable with asymmetric light curves[13].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.858'}[14].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.523'}[15].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.680'}[16].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.355'}[17].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.223'}[18].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.969'}[19].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.848'}[20].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.814'}[21].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.62'}[22].
  • RS Comae Berenices's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.6213'}[23].
  • RS Comae Berenices's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0474'}[24].
  • RS Comae Berenices's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-18'}[25].
  • RS Comae Berenices's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q11929860', 'amount': '+9.38'}[26].

Body

Designation and Status

RS Comae Berenices's instance of is recorded as RR Lyrae variable[2].

History and Context

Catalog codes include [SHM2017] J198.66493+17.19691[4], RS Com[5], 2MASS J13143959+1711492[6], LINEAR 8680084[7], SDSS J131439.57+171148.7[8], and [DCD2013] CSS J131439.5+171148[9].

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

  1. [2] ↑ . SIMBAD. wikidata.org.
  2. [3] ↑ . VizieR. wikidata.org.
  3. [4] ↑ . SIMBAD. wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . SIMBAD. wikidata.org.
  8. [9] ↑ . SIMBAD. wikidata.org.
  9. [10] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . SIMBAD. wikidata.org.
  12. [13] ↑ . Machine-learned Identification of RR Lyrae Stars from Sparse, Multi-band Data: The PS1 Sample. wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  14. [15] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  15. [16] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  16. [17] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  17. [18] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  18. [19] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  19. [20] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  20. [21] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  21. [22] ↑ . Probing the outer galactic halo with RR Lyrae from the Catalina surveys. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  25. [26] ↑ . Exploring the variable sky with LINEAR. II. Halo structure and substructure traced by RR Lyrae stars to 30 kpc. wikidata.org.

Class ancestry

  1. [1] ↑ . Wikidata. wikidata.org.

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Use these citations when quoting this entity in research, articles, AI prompts, or wherever provenance matters. We aggregate Wikidata + Wikipedia + authoritative open-data sources; the stitched, scored, cross-referenced view is what 4ort.xyz contributes.

APA 4ort.xyz Knowledge Graph. (2026). RS Comae Berenices. Retrieved May 3, 2026, from https://4ort.xyz/entity/rs-comae-berenices
MLA “RS Comae Berenices.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/rs-comae-berenices.
BibTeX @misc{4ortxyz_rs-comae-berenices_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{RS Comae Berenices}}, year = {2026}, url = {https://4ort.xyz/entity/rs-comae-berenices}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): RS Comae Berenices — https://4ort.xyz/entity/rs-comae-berenices (retrieved 2026-05-03)

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