Astronomy:HE 1219-0312
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Virgo |
| Right ascension | 12h 21m 34.143s[1] |
| Declination | −03° 28′ 39.64″[1] |
| Apparent magnitude (V) | 15.94[2] |
| Characteristics | |
| Evolutionary stage | Metal-poor star[citation needed] |
| Spectral type | CEMP[citation needed] |
| Astrometry | |
| Proper motion (μ) | RA: −2.817[1] mas/yr Dec.: −8.763[1] mas/yr |
| Parallax (π) | 0.0893 ± 0.042[1] mas |
| Distance | approx. 40,000 ly (approx. 11,000 pc) |
| Details | |
| Mass | 0.8[3] M☉ |
| Radius | 2.5[1] R☉ |
| Luminosity | 6.3[1] L☉ |
| Surface gravity (log g) | 2.05[3] cgs |
| Temperature | 5,100[3] K |
| Metallicity [Fe/H] | −2.96[4] dex |
| Age | 13.6[3] Gyr |
| Other designations | |
HE 1219-0312, 2MASS J12213413-0328396 | |
| Database references | |
| SIMBAD | data |
HE 1219-0312 is an extremely metal-poor star in the constellation Virgo, The star is located at around 41,400 light years away from earth.[1]
It is thought to be a second generation, Population II or metal-poor star ([Fe/H] = -2.96), The star was found in the sample of extremely metal-poor halo stars from the Hamburg/ESO Survey by W. Hayek and collaborators. The group's research was published in the July 2, 2009 issue of The Astrophysical Journal.[4]
If the age of the star HE 1219-0312 was confirmed at 17.6 billion years, that this star will be the oldest star in the universe.[4]
Elemental abundance
The abundance of two strongly r-process enhanced in two metal-poor stars, BPS CS29491-0069 and HE 1219-0312 was detected by HERES project, which there was ([Fe/H] = -2.51, [r/Fe] = +1.1) and ([Fe/H] = -2.96, [r/Fe] = +1.5).[4]
the analysis based on high-quality VLT/UVES spectra and MARCS model atmosphere was detected these eighteen heavy elements in the spectrum of HE 1219–0312 with an case of Th II 4019A line.[4]
Radioactive dating for HE 1219–0312 with the observed thorium and rare-earth elements abundance pairs results in an average age of 9.5 billion years, when based on solar r-process residuals, that Age of the star HE 1219-0312 was 17.6 billion years, so, we puts the age of HE 1219-0312 into 13.6 billion years to avoid to exceed the universe's age.[4]
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ Beers, Timothy C.; Flynn, Chris; Rossi, Silvia; Sommer-Larsen, Jesper; Wilhelm, Ronald; Marsteller, Brian; Lee, Young Sun; De Lee, Nathan et al. (2007). "Broadband UBVRCIC Photometry of Horizontal-Branch and Metal-poor Candidates from the HK and Hamburg/ESO Surveys. I.". The Astrophysical Journal Supplement Series 168 (1): 128. doi:10.1086/509324. Bibcode: 2007ApJS..168..128B.
- ↑ 3.0 3.1 3.2 3.3 Reggiani, Henrique; Ji, Alexander P.; Schlaufman, Kevin C.; Frebel, Anna; Necib, Lina; Nelson, Tyler; Hawkins, Keith; Galarza, Jhon Yana (2022). "The Chemical Composition of Extreme-velocity Stars". The Astronomical Journal 163 (6): 252. doi:10.3847/1538-3881/ac62d9. Bibcode: 2022AJ....163..252R.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 Kratz, Hayek; Pfeiffer, Wiesendahl (2009). "The Hamburg/ESO R-process enhanced star survey (HERES). IV. Detailed abundance analysis and age dating of the strongly r-process enhanced stars CS 29491-069 and HE 1219-0312". The Astronomical Journal 504 (2): 524. doi:10.1051/0004-6361/200811121. Bibcode: 2009A&A...514..511H.
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