# Beta Cancri
**Beta Cancri** (β Cancri, abbreviated Beta Cnc or β Cnc) is an orange giant star, the brightest star in the constellation Cancer, carrying the IAU-approved proper name **Tarf**. It is a K-type giant of spectral class K4 III with an apparent visual magnitude of 3.53, visible to the naked eye, and it hosts a confirmed gas-giant planet, Beta Cancri b, announced in 2014.[1](https://asteriastar.com/stars/tarf) • [2](https://science.nasa.gov/exoplanet-catalog/beta-cancri-b/)
| Key fact | Detail |
|---|---|
| Designations | β Cancri (Bayer), 17 Cancri (Flamsteed), HR 3249, HD 69267, HIP 40526[1](https://asteriastar.com/stars/tarf) • [3](https://theplanets.org/stars/tarf-%CE%B2-cancri/) |
| Spectral class | K4 III, an orange giant; some catalogs add a barium-star suffix (K4III Ba1)[1](https://asteriastar.com/stars/tarf) |
| Brightness | Apparent magnitude 3.53; the brightest star in Cancer, a faint zodiacal constellation[1](https://asteriastar.com/stars/tarf) • [4](https://opdtechnologies.com/celestial/cancer/) |
| Distance | About 290 light-years by one estimate, 303.4 light-years (93.02 pc) in another compilation[5](https://astrosud.nc/etoiles/tarf/) • [1](https://asteriastar.com/stars/tarf) |
| Planet | Beta Cancri b, a gas giant of minimum mass 7.8 Jupiter masses in a 605-day orbit, found by radial velocity[6](https://arxiv.org/abs/1405.2127) |
## Name
The name Tarf comes from the Arabic الطرف, Al-Ṭarf, meaning "the eyes of the lion". It was originally one of the traditional lunar stations, a set of stellar markers through which the Moon appears to pass, and referred to the pair ε Leonis and ο Leonis. The name nevertheless came into common use for β Cancri because it was published that way in the Yale Bright Star Catalogue.[7](https://www.heavensremember.top/en/stars/tarf)
## Stellar properties
Beta Cancri is classified as an orange giant of spectral type K4 III, meaning a cool, evolved star of luminosity class III. The NASA Exoplanet Archive lists a stellar radius of 47.20 solar radii and an effective temperature of 4,092.10 K for bet Cnc, and notes that some of these stellar parameters may be biased by the blend with a companion.[8](https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=bet+Cnc+b&type=CONFIRMED_PLANET) A French observing guide estimates the diameter at about 36 times the Sun's, with a stated typical precision of 10 to 20 percent for such estimates.[5](https://astrosud.nc/etoiles/tarf/)
The star is also described as a variable and double giant star.[9](https://theskylive.com/sky/stars/tarf-beta-cancri-star)
Distance estimates differ between compilations: about 290 light-years in one observing guide and 303.4 light-years (93.02 parsecs) in a Gaia-based summary, which also lists a Gaia parallax of 10.1026 ± 0.3141 milliarcseconds.[5](https://astrosud.nc/etoiles/tarf/) • [1](https://asteriastar.com/stars/tarf) The NASA Exoplanet Archive gives a distance of 97.775 ± 0.550 parsecs with a parallax of 10.1991 ± 0.0571 milliarcseconds.[8](https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=bet+Cnc+b&type=CONFIRMED_PLANET)
## Planetary system
**Beta Cancri b.** A planetary companion to β Cancri was reported in 2014 by B.-C. Lee of the Korea Astronomy and Space Science Institute and colleagues, from a radial-velocity survey of evolved stars carried out with the Bohyunsan Observatory Echelle Spectrograph (BOES) between 2003 and 2013.[6](https://arxiv.org/abs/1405.2127) The companion has a minimum mass of 7.8 Jupiter masses in a 605-day orbit with an eccentricity of 0.08.[6](https://arxiv.org/abs/1405.2127) NASA's exoplanet catalog describes it as a gas giant orbiting 1.7 AU from its star with a period of 1.7 years and an estimated radius of 1.12 Jupiter radii.[2](https://science.nasa.gov/exoplanet-catalog/beta-cancri-b/)
The detection rests on more than the radial-velocity curve. HIPPARCOS photometry of the star shows no variations at periods close to those in the radial-velocity data, the bisector velocity span shows no strong correlation with the radial velocities, and the star shows weak or no core reversal in the Ca II H lines, indicating that it is an inactive star. Together these checks support a planetary rather than a stellar-activity origin for the signal.[6](https://arxiv.org/abs/1405.2127)
The same survey reported companions around two other K giants, μ Leonis and β Ursae Minoris, making β Cancri part of a small set of evolved stars with confirmed giant planets found by that program.[6](https://arxiv.org/abs/1405.2127)
## A multiple system
The NASA Exoplanet Archive lists a second stellar entry, bet Cnc B, with a radius of 0.64 solar radii and an effective temperature of 4,003 K, and notes that the system's multiplicity has been discussed in the literature; it also cautions that some stellar parameters may be biased by the companion blend.[8](https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=bet+Cnc+b&type=CONFIRMED_PLANET)
## Place in Cancer
Cancer is one of the faintest zodiacal constellations, and Tarf is its brightest star at about magnitude 3.5, marking one outer part of the traditional Crab figure.[4](https://opdtechnologies.com/celestial/cancer/) For observers, the star is best placed on January evenings; from southern locations such as [New Caledonia](https://www.edgepedia.org/new-caledonia) it culminates high in the sky and is an easy naked-eye object even under city skies.[5](https://astrosud.nc/etoiles/tarf/) The same constellation contains the Beehive Cluster (Messier 44), the older open cluster M67, and the nearby planetary system 55 Cancri, a Sun-like star with five known planets.[4](https://opdtechnologies.com/celestial/cancer/) • [10](https://science.nasa.gov/resource/our-solar-systems-cousin/)
## References
1. [Tarf — Star, Asteria Star (SIMBAD and Gaia DR3 data)](https://asteriastar.com/stars/tarf)
2. [Beta Cancri b, NASA Science Exoplanet Catalog](https://science.nasa.gov/exoplanet-catalog/beta-cancri-b/)
3. [Tarf (β Cancri) Star - Features & Facts, The Planets](https://theplanets.org/stars/tarf-%CE%B2-cancri/)
4. [Cancer, OPD Technologies Celestial Archive](https://opdtechnologies.com/celestial/cancer/)
5. [Tarf - ASTROSUD](https://astrosud.nc/etoiles/tarf/)
6. [Lee, B.-C. et al. (2014). Planetary companions in K giants beta Cancri, mu Leonis, and beta Ursae Minoris. Astronomy & Astrophysics 566, A67.](https://arxiv.org/abs/1405.2127)
7. [Tarf — star of Crab, IAU Catalog of Star Names account](https://www.heavensremember.top/en/stars/tarf)
8. [bet Cnc Overview, NASA Exoplanet Archive](https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=bet+Cnc+b&type=CONFIRMED_PLANET)
9. [Tarf - β Cancri - Star in Cancer, TheSkyLive](https://theskylive.com/sky/stars/tarf-beta-cancri-star)
10. [Our Solar System's Cousin?, NASA Science](https://science.nasa.gov/resource/our-solar-systems-cousin/)
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*Topic: Encyclopedia › Places and geography › Extraterrestrial places › Exoplanets and nearby star systems › Bright naked-eye stars with planets*
*Initially written Oct 15, 2026 · Edited: Oct 25, 2026*
*Copyright 2026 EdgeChat AI, a subsidiary of Biostate AI.*
License: Edgepedia Community License 1.0, https://www.edgepedia.org/edgepedia/license