R Hydrae

Not to be confused with Rho Hydrae.
R Hydrae
Location of R Hydrae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra
Right ascension 13h 29m 42.782s[1]
Declination −23° 16′ 52.77″[1]
Apparent magnitude (V) 3.5 to 10.9 (variable)[2]
Characteristics
Spectral type M6e/M9e:[3]
B−V color index 1.317±0.254[4]
Variable type Mira[2] (period 388.87 days)
Astrometry
Radial velocity (Rv)−10.0±0.6[5] km/s
Proper motion (μ) RA: −57.68 mas/yr[1]
Dec.: +12.86 mas/yr[1]
Parallax (π)7.93 ± 0.18 mas[6]
Distance482±33 ly
(148±10 pc)[7]
Absolute magnitude (MV)+0.95[4]
Details
Mass2[8] M☉
Radius377[7][a] R☉
Luminosity10,000[8] L☉
Temperature2,830[8] K
Age0.5–1.0[8] Gyr
Other designations
R Hya, BD−22° 3601, HD 117287, HIP 65835, HR 5080, SAO 181695, WDS 13297-2317A[9]
Database references
SIMBADdata

R Hydrae, abbreviated R Hya,[2] is a single[10] star in the equatorial constellation of Hydra, about 2.7° to the east of Gamma Hydrae.[11] It is a Mira-type variable[2] that ranges in apparent visual magnitude from 3.5 down to 10.9 over a period of 389 days. At maximum brightness the star can be seen with the naked eye, while at minimum a telescope of at least 5 cm is needed. This star is located at a distance of approximately 480 light-years from the Sun[7] but is drifting closer with a radial velocity of −10 km/s.[5]

This is an aging red giant star with a stellar classification of M6e/M9e:,[3] currently near the thermal-pulsing tip of the asymptotic giant branch.[8] The 1998 detection of weak technicium (Tc) lines in the spectrum suggests the star has recently gone through a third dredge-up.[12] However, a 2010 study failed to detect technicium in the atmosphere, indicating this oxygen-rich AGB star is Tc-poor.[13] O. J. Eggen found the star is a likely member of the Hyades supergroup, which suggests an age of 500 million to one billion years and a mass double that of the Sun.[8]

A visual band light curve for R Hydrae, from AAVSO data[14]

The first record of observations for this star was in 1662 by Johannes Hevelius. It was found to be variable by Giacomo Filippo Maraldi in 1702; thereafter he tracked its various appearances until 1712. The evidence suggests the period of variability during this period was ~495 days. In between 1770 and 1950, the period declined linearly down to 385 days. It has remained fairly stable since that time. The decline may be due to a prior thermal pulse caused by a helium flash under a hydrogen-fusing shell.[jargon] The period change would have been accompanied by a decrease in the stellar radius. An alternative explanation is a relaxation of the stellar envelope brought on by a change in the structure within the star.[8]

The bow shock around R Hya[15]

An extended emission component has been detected in the infrared that indicates a detached, expanding dust shell surrounds the star. The inner boundary of this shell is located at 60–100 times the stellar radius, and it extends outward to at least 1,000 times the radius[12] with an expansion velocity of ~8 km/s.[16] The data indicate a mass loss rate of 2×10−7 M☉·yr−1, which declined by a factor of 20 around the year 1788.[16] Observations using the Spitzer Space Telescope show an extended double shell with a spiral structure, which extends out to 300″. It forms a bow shock where it interacts with the surrounding interstellar medium. The orientation of this feature is consistent with the star's proper motion.[17]

  1. ^ a b c Cite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference AAVSO was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Keenan_et_al_1974 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference Anderson_Francis_2012 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference Gontcharov2006 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference rraql was invoked but never defined (see the help page).
  7. ^ a b c Cite error: The named reference montarges was invoked but never defined (see the help page).
  8. ^ a b c d e f g Cite error: The named reference Zijlstra_et_al_2002 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference Pourbaix2008 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference Sinnott_Perryman_1997 was invoked but never defined (see the help page).
  12. ^ a b Cite error: The named reference Hashimoto_et_al_1998 was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference Uttenthaler_Lebzelter_2010 was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference aavso was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference spitzer was invoked but never defined (see the help page).
  16. ^ a b Cite error: The named reference Decin_et_al_2008 was invoked but never defined (see the help page).
  17. ^ Cite error: The named reference Speck_et_al_2006 was invoked but never defined (see the help page).


Cite error: There are <ref group=lower-alpha> tags or {{efn}} templates on this page, but the references will not show without a {{reflist|group=lower-alpha}} template or {{notelist}} template (see the help page).