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AS 209
View on Wikipedia Image of protoplanetary disk that surrounds AS 209. Here we can see the prominent rings around the star | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Ophiuchus |
| Right ascension | 16h 49m 15.303s[1] |
| Declination | –14° 22′ 08.64″[1] |
| Apparent magnitude (V) | 11.28[2] |
| Characteristics | |
| Evolutionary stage | pre-main sequence |
| Spectral type | K4Ve[2] |
| Variable type | T Tauri[3] |
| Astrometry | |
| Proper motion (μ) | RA: -7.366 mas/yr[1] Dec.: -23.658 mas/yr[1] |
| Parallax (π) | 8.2477±0.0290 mas[1] |
| Distance | 395 ± 1 ly (121.2 ± 0.4 pc) |
| Details | |
| Mass | 0.9[4] M☉ |
| Luminosity | 1.5[4] L☉ |
| Age | 0.5-1.0[4] Myr |
| Other designations | |
| V1121 Oph, HIP 82323, TYC 5641-480-1, IRAS 16464-1416, AS 209, PDS 92[2] | |
| Database references | |
| SIMBAD | data |
AS 209 is a young pre-main-sequence K-type star located in the Ophiuchus star formation region about 126 parsecs from the Sun. It has a mass of 0.9 solar masses and a luminosity of 1.5 solar luminosity. It is only somewhere between 0.5-1.0 million years old. Surrounding AS 209 is a remarkable protoplanetary disk. This disk is separated into several distinct parts. There the central core and extending from it lies two prominent rings at 75 AU and 135 AU. These rings have different widths and depths with the inner one being narrower and shallower.[4][5][6]
AS 209 was found to be a variable star in 1968.[9] and it was given the variable star designation V1121 Ophiuchi, in 1970.[10] The International Variable Star Index classifies it as both a classical T Tauri star and a T Tauri star showing periodic variability due to starspots.[3] The Hipparcos data for the star shows periodic variability.[11] S. A. Artemenko et al. determined that the period is 8.60 days, in 2012.[12]
The gap of the outer disk suggest that there might be a Saturn-like (0.7 Saturn mass) exoplanet orbiting the star at a distance of 62 AU. There may also be a second planet with 0.1 Jupiter masses orbiting closer to the star than the first planet. The discovery of such planets around a young less than a million year old star shows that giant planets are able to form far from their stars on wide orbits.[4]
References
[edit]- ^ a b c d Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b c "EM* AS 209". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 28 May 2025.
- ^ a b "V1121 Oph". AAVSO. Retrieved 29 May 2025.
- ^ a b c d e Fedele, D.; Tazzari, M.; Booth, R.; Testi, L.; Clarke, C. J.; Pascucci, I.; Kospal, A.; Semenov, D.; Bruderer, S.; Henning, Th; Teague, R. (2018-02-01). "ALMA continuum observations of the protoplanetary disk AS 209 - Evidence of multiple gaps opened by a single planet". Astronomy & Astrophysics. 610: A24. arXiv:1711.05185. Bibcode:2018A&A...610A..24F. doi:10.1051/0004-6361/201731978. ISSN 0004-6361.
- ^ Fedele, D.; Bollati, F.; Lodato, G. (2023). "Kinematics signature of a giant planet in the disk of AS 209". Astronomy and Astrophysics. 672: A125. arXiv:2302.11028. Bibcode:2023A&A...672A.125F. doi:10.1051/0004-6361/202244486.
- ^ "ALMA Spots Circumplanetary Disk around Young Star AS 209 | Sci.News". Sci.News: Breaking Science News. 2022-08-09. Retrieved 2025-05-28.
- ^ "ASAS-SN Variable Stars Database". ASAS-SN Variable Stars Database. ASAS-SN. Retrieved 29 May 2025.
- ^ EAS (1997). "The HIPPARCOS and TYCHO catalogues". Astrometric and Photometric Star Catalogues Derived from the ESA Hipparcos Space Astrometry Mission. ESA SP Series. 1200. Noordwijk, Netherlands: ESA Publications Division. Bibcode:1997ESASP1200.....E. ISBN 9290923997. Retrieved 15 October 2022.
- ^ Zaitseva, G. V. (1968). "Photoelectric Observations of RW Aur Type Stars". Peremennye Zvezdy. 16: 435. Bibcode:1968PZ.....16..435Z.
- ^ Kukarkin, B. V.; Kholopov, P. N.; Perova, N. B. (October 1970). "57th Name-List of Variable Stars" (PDF). Information Bulletin on Variable Stars. 480: 1. Bibcode:1970IBVS..480....1K. Retrieved 29 May 2025.
- ^ Koen, Chris; Eyer, Laurent (March 2002). "New periodic variables from the Hipparcos epoch photometry". Monthly Notices of the Royal Astronomical Society. 331 (1): 45–59. arXiv:astro-ph/0112194. Bibcode:2002MNRAS.331...45K. doi:10.1046/j.1365-8711.2002.05150.x. Retrieved 29 May 2025.
- ^ Artemenko, S. A.; Grankin, K. N.; Petrov, P. P. (December 2012). "Rotation effects in classical T Tauri stars". Astronomy Letters. 38 (12): 783–792. arXiv:1301.2493. Bibcode:2012AstL...38..783A. doi:10.1134/S1063773712110011. Retrieved 29 May 2025.
