| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus[1] |
| Right ascension | 20h 49m 27.44052s[2] |
| Declination | +33° 36′ 50.9686″[2] |
| Apparent magnitude (V) | 17.8 (estimate)[3] |
| Characteristics | |
| Evolutionary stage | Red dwarf |
| Spectral type | M6.5±0.5[4] |
| Apparent magnitude (B) | 19[5] |
| Apparent magnitude (R) | 16.4[5] |
| Apparent magnitude (G) | 15.379[2] |
| Apparent magnitude (J) | 11.5[6] |
| Apparent magnitude (H) | 10.867±0.021[5] |
| Apparent magnitude (K) | 10.54[6] |
| Astrometry | |
| Proper motion (μ) | RA: –207.809 mas/yr[2] Dec.: –412.215 mas/yr[2] |
| Parallax (π) | 59.7005 ± 0.0434 mas[2] |
| Distance | 54.63 ± 0.04 ly (16.75 ± 0.01 pc)[2] |
| Details[4] | |
| Mass | 0.1009±0.0024 M☉ |
| Radius | 0.123±0.0022 R☉ |
| Luminosity | 0.000835±0.000019 L☉ |
| Surface gravity (log g) | 5.265±0.014 cgs |
| Temperature | 2800±29 K |
| Metallicity [Fe/H] | 0.07±0.1 dex |
| Rotation | 1.34±0.14 d |
| Rotational velocity (v sin i) | 4.8±0.5 km/s |
| Age | 6.6+1.8 −2.4 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
SPECULOOS-3, also known as LSPM J2049+3336, is a red dwarf star (spectral type M6.5) located 54.6 light-years from Earth[4] in the constellation Cygnus. It is one of the smallest known stars, and is much cooler, dimmer and smaller than the Sun, having 0.1 times the mass, 0.08% the Sun's luminosity, and an effective temperature of 2,800 K (2,530 °C), which is less than half of the Sun's temperature (5,772 K).[4] It is orbited by one known exoplanet, and is the second ultra-cool dwarf discovered to have a planetary system, after TRAPPIST-1.[7][8]
Stellar properties
The age of SPECULOOS-3 is constrained at 6.6 billion years, 44% older than the Solar System, with significant margins of error. A bayesian analysis of the star derived a mass of 0.101 M☉, an effective temperature of 2,800 K (2,530 °C; 4,580 °F) and a luminosity of 8.35×10−6 L☉. These characteristics classify SPECULOOS-3 as an ultracool dwarf, which are stars at the end of the main sequence, with low temperatures, low luminosites and sizes similar to Jupiter. It is spinning at a rotational velocity of 4.8 km/s and has a projected rotational period of 1.34 days.[4]
The stellar radius, computed using the Stefan–Boltzmann law, is 0.134 R☉ (93,000 kilometres).[4] This makes SPECULOOS-3 the second-smallest star known to host a transiting planet, just marginally larger than TRAPPIST-1,[4] and its size is similar to that of Jupiter.[9] Its apparent magnitude is estimated at 17.8,[3] which is too faint to be seen by the naked eye.
It was first discovered in 2005 as part of the LSPM-North catalog, whose objective was to map stars in the northern celestial hemisphere with proper motions larger than 0.15" per year and apparent magnitudes smaller than 21m.[3] Its trignometric parallax was first measured in 2014 at 67.5±1.7 mas, translating into a distance of 14.8 parsecs (48.27 ly).[6] Gaia Data Release 3 (2023) published a parallax of 59.7 milliarcseconds, translating into a distance of 16.75 parsecs (54.6 ly).[2] This make this star relatively close to Earth.[10]
Red dwarf stars such as SPECULOOS-3 are the most numerous type of stars, making up 70% of all stars in the Milky Way galaxy. They are expected to live 10 times more than the Sun, with lifespans longer than 100 billion years.[10]
Planetary system
In 2024, an exoplanet was found around the star using the transit method.[11] Named SPECULOOS-3 b, it is an Earth-sized exoplanet that has a radius similar to that of Earth, equivalent to 0.98 Earth radii.[4] It takes only about 17 hours to complete an orbit around SPECULOOS-3, and, because of that proximity, it receives very high levels of radiation and is likely tidally locked, meaning that one side of the planet always faces its host star.[9] Its discovery was made using the SPECULOOS project, and was announced on 15 May 2024 in the academic journal Nature Astronomy.[12]
The mass of SPECULOOS-3 b has been not measured,[4] but the NASA Exoplanet Catalog estimated it at 0.894 ME.[13] Its equilibrium temperature is about 553 K (280 °C; 536 °F), meaning that its dayside is likely formed by solid rock.[4] The planet is an optimal target for characterization with the James Webb Space Telescope, giving more information about the planet's mineralogy[12] and the possibility of hosting an atmosphere.[14]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | — | 0.007330(55) | 0.71912603(57) | — | 89.44±0.39° | 0.977±0.022 R🜨 |
References
- ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
- ^ a b c d e f g 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 Lépine, Sébastien; Shara, Michael M. (2005-03-01). "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)". The Astronomical Journal. 129 (3): 1483–1522. arXiv:astro-ph/0412070. Bibcode:2005AJ....129.1483L. doi:10.1086/427854. ISSN 0004-6256. SPECULOOS-3's database entry at VizieR.
- ^ a b c d e f g h i j k Gillon, Michaël; Pedersen, Peter P.; Rackham, Benjamin V.; Dransfield, Georgina; Ducrot, Elsa; Barkaoui, Khalid; Burdanov, Artem Y.; Schroffenegger, Urs; Gómez Maqueo Chew, Yilen; Lederer, Susan M.; Alonso, Roi; Burgasser, Adam J.; Howell, Steve B.; Narita, Norio; de Wit, Julien (2024-05-15). "Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3". Nature Astronomy: 1–14. arXiv:2406.00794. Bibcode:2024NatAs.tmp...96G. doi:10.1038/s41550-024-02271-2. ISSN 2397-3366.
{{cite journal}}: CS1 maint: bibcode (link) - ^ a b c "LSPM J2049+3336". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved May 26, 2024.
- ^ a b c Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014-04-01). "Trigonometric Parallaxes for 1507 Nearby Mid-to-late M Dwarfs". The Astrophysical Journal. 784 (2): 156. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156. ISSN 0004-637X. SPECULOOS-3's database entry at VizieR.
- ^ Anderson, Natali (2024-05-15). "Earth-Sized Exoplanet Found Orbiting Nearby Ultracool Red Dwarf". Sci.News. Retrieved 2024-05-28.
- ^ "Detection of an Earth-sized exoplanet orbiting the ultracool dwarf star SPECULOOS-3". ScienceDaily. Retrieved 2024-05-28.
- ^ a b Hill, Samantha (2024-05-16). "Found: An Earth-sized exoplanet named SPECULOOS-3 b". Astronomy Magazine. Retrieved 2024-05-26.
- ^ a b "Discovery Alert: An Earth-sized World and Its Ultra-cool Star - NASA Science". science.nasa.gov. Retrieved 2024-05-26.
- ^ "The Extrasolar Planet Encyclopaedia — SPECULOOS-3 b". Extrasolar Planets Encyclopaedia. Paris Observatory. Retrieved May 26, 2024.
- ^ a b "Astronomers discover new Earth-sized world orbiting an ultra-cool star". phys.org. May 15, 2024. Retrieved 2024-05-26.
- ^ "SPECULOOS-3 b - NASA Science". science.nasa.gov. Retrieved 2024-05-26.
- ^ Lea, Robert (2024-05-15). "Earth-size planet discovered around cool red dwarf star shares its name with a biscuit". Space.com. Retrieved 2024-05-29.
This page was last edited on 4 June 2024, at 16:02