La Superba

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Variable star in the constellation Canes Venatici

title: "La Superba" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["semiregular-variable-stars", "canes-venatici", "carbon-stars", "stars-with-proper-names", "objects-with-variable-star-designations", "henry-draper-catalogue-objects", "bright-star-catalogue-objects", "hipparcos-objects", "durchmusterung-objects", "asymptotic-giant-branch-stars"] description: "Variable star in the constellation Canes Venatici" topic_path: "science/astronomy" source: "https://en.wikipedia.org/wiki/La_Superba" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0

::summary Variable star in the constellation Canes Venatici ::

| image = |image=Canes Venatici constellation map.svg|alt=|float=center|width=280 |label=|position=right |mark=Red circle.svg|mark_width=10|mark_link=La Superba |x=570|y=240 | caption = Location of Y Canum Venaticorum (circled in red) | epoch=J2000.0 | constell=Canes Venatici | ra= | dec= | appmag_v=+4.86 to +7.32 | type = AGB | class = C54J(N3) | r-i=1.38 | v-r=1.75 | b-v=2.54 | u-b=6.62 | variable = SRb | radial_v=15.30 | prop_mo_ra=−2.968 | prop_mo_dec=13.063 | parallax= 3.2222 | p_error=0.1744 | parallax_footnote= | absmag_v = −1.203 | mass = 1.2 | radius = 315 La Superba's database entry at VizieR. | rotation = | luminosity = 4,4009,400{{cite journal | display-authors=1 | last1=Chandler | first1=Colin Orion | last2=McDonald | first2=Iain | last3=Kane | first3=Stephen R. | title=The Catalog of Earth-Like Exoplanet Survey Targets (CELESTA): A Database of Habitable Zones Around Nearby Stars | journal=The Astronomical Journal | volume=151 | issue=3 | pages=59 | year=2016 | bibcode=2016AJ....151...59C | arxiv=1510.05666 | doi=10.3847/0004-6256/151/3/59 | s2cid=119246448 | doi-access=free }} | temperature = 2,600 - 3,200 | gravity = +0.23 | metal_fe = −0.21 | age_myr = names=La Superba, Y Canum Venaticorum, HR 4846, HD 110914, BD+46°1817, FK5 1327, HIP 62223, SAO 44317, GC 17342, 152 Schjellerup | Simbad = Y+CVn

La Superba (Y CVn, Y Canum Venaticorum) is a strikingly red giant star in the constellation Canes Venatici. It is faintly visible to the naked eye, and the red colour is very obvious in binoculars. The 19th century astronomer Angelo Secchi, impressed with its beauty, gave the star its common name, which is accepted by the International Astronomical Union.

Visibility

::figure[src="https://upload.wikimedia.org/wikipedia/commons/b/b0/Y_Canum_Venaticorum_RGB.jpg" caption="Y Canum Venaticorum in optical light"] ::

La Superba is a semiregular variable star, varying by about a magnitude over a roughly 160-day cycle, but with slower variation over a larger range. Periods of 194 and 186 days have been suggested, with a resonance between the periods.

Y CVn is one of the reddest stars known, and it is among the brightest of the giant red carbon stars. It is the brightest of known J-stars, which are a very rare category of carbon stars that contain large amounts of carbon-13 (carbon atoms with 7 neutrons instead of the usual 6).

Properties

::figure[src="https://upload.wikimedia.org/wikipedia/commons/4/40/Y_Canum_Venaticorum_light_curve.png" caption="Y Canum Venaticorum light curve, including RGB photoelectric measurements"] ::

Calculations with La Superba's luminosity and effective temperature give it a radius of about . If it were placed at the position of the Sun, the star's surface would extend beyond Earth's orbit.

La Superba's temperature is believed to be about , making it one of the coolest stars known. When infrared radiation is included, Y CVn has a bolometric luminosity several thousand times that of the Sun. The mass of this type of star is difficult to determine; it would initially have been around and somewhat less now due to mass loss. An estimate from Jim Kaler gives the star a luminosity between and radius between based on an assumed temperature of 3,000 K, and the author then classified it as a C7 or CN5 supergiant star although its mass is too low to be a true supergiant.

Observations in the 60 and 100 micron infrared bands by the IRAS satellite showed that Y CVn is surrounded by a dust shell 0.9 parsecs in diameter. This is one of the most prominent circumstellar dust shells detected in the IRAS all-sky survey.

Evolution

::figure[src="https://upload.wikimedia.org/wikipedia/commons/3/32/Y_Canum_Venaticorum.jpg" caption="Y CVn and the [[Sun]] at the same distance; rendered with [[Celestia"] ::

After stars up to a few times the mass of the sun have finished fusing hydrogen to helium in their core, they start to burn hydrogen in a shell outside a degenerate helium core, and expand dramatically into the red giant state. Once the core reaches a high enough temperature, it ignites violently in the helium flash, which begins helium core burning on the horizontal branch. Once even the core helium is exhausted, a degenerate carbon-oxygen core remains. Fusion continues in both hydrogen and helium shells at different depths in the star, and the star increases luminosity on the asymptotic giant branch (AGB). La Superba is currently an AGB star.

In the AGB stars, fusion products are moved outwards from the core by strong deep convection known as a dredge-up, thus creating a carbon abundance in the outer atmosphere where carbon monoxide and other compounds are formed. These molecules tend to absorb radiation at shorter wavelengths, resulting in a spectrum with even less blue and violet compared to ordinary red giants, giving the star its distinguished red color.

La Superba is most likely in the final stages of fusing its remaining secondary fuel (helium) into carbon and shedding its mass at the rate of about a million times that of the Sun's solar wind. It is also surrounded by a 2.5 light year-wide shell of previously ejected material, implying that at one point it must have been losing mass as much as 50 times faster than it is now. La Superba thus appears almost ready to eject its outer layers to form a planetary nebula, leaving behind its core in the form of a white dwarf.

References

References

  1. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S.
  2. (2022). "Investigating dust properties in AGB wind-ISM interaction regions". Astronomy and Astrophysics.
  3. (2011). "Search for and study of hot circumstellar dust envelopes". Astronomy Reports.
  4. {{SIMBAD link
  5. (2002). "VizieR On-line Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues.
  6. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters.
  7. {{cite Gaia DR3. 1542553623374596352
  8. (2017). "VizieR Online Data Catalog: Tycho-2 red giant branch and carbon stars (Gontcharov, 2011)". VizieR On-line Data Catalog.
  9. (1 August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics.
  10. (2009-01-01). "Circumstellar 12C/13C Isotope Ratios from Millimeter Observations of CN and CO: Mixing in Carbon- and Oxygen-Rich Stars". The Astrophysical Journal.
  11. (2014). "Evidence of a Mira-like tail and bow shock about the semi-regular variable V CVn from four decades of polarization measurements". Astronomy & Astrophysics.
  12. (2007). "Binocular Astronomy". Springer.
  13. (1994). "Angelo Secchi and the Discovery of Carbon Stars". The MK Process at 50 Years. A Powerful Tool for Astrophysical Insight Astronomical Society of the Pacific Conference Series.
  14. "Superbo: Traduzione e significato in Italiano {{!}} Dizionario di Inglese {{!}} Corriere.it".
  15. "International Astronomical Union | IAU".
  16. Jim Kaler. "La Superba".
  17. (1993). "Circumstellar Shells Resolved in IRAS Survey Data. II. Analysis". The Astrophysical Journal.
  18. (2002). "S-Process Nucleosynthesis in Carbon Stars". The Astrophysical Journal.
  19. (2007). "The formation of a detached shell around the carbon star Y CVn". Monthly Notices of the Royal Astronomical Society.

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semiregular-variable-starscanes-venaticicarbon-starsstars-with-proper-namesobjects-with-variable-star-designationshenry-draper-catalogue-objectsbright-star-catalogue-objectshipparcos-objectsdurchmusterung-objectsasymptotic-giant-branch-stars