Discovery | |
---|---|
Discovered by | Conzo G. & Moriconi M. and Sgro L. et al. |
Discovery site | Transiting Exoplanet Survey Satellite |
Discovery date | February 26, 2024 |
Transit | |
Designations | |
TIC 393818343 b | |
Orbital characteristics | |
Epoch J2000.0 | |
0.1291 ± 0.0021 AU (19,310,000 ± 310,000 km) | |
Eccentricity | 0.6058 ± 0.0023 |
16.24921 ± 0.00010 d | |
Inclination | 89.6 ± 0.30 |
2459810.145 ± 0.015 | |
1.69 ± 0.49 | |
Star | TOI-6883 |
Physical characteristics | |
1.087 ± 0.023 RJ | |
Mass | 4.34 ± 0.15 MJ |
Temperature | 805.5 ± 9.6 K (532.35 ± 9.60 °C; 990.23 ± 17.28 °F) |
TOI-6883 b is a Jupiter-like extrasolar planet orbiting TOI-6883, a Sun-like star in the Delphinus constellation 307 light years (94.17 pc) from Earth.
It was discovered in 2024 by Italian amateur astronomers Giuseppe Conzo and Mara Moriconi using the transit method with TESS data. At the beginning, a single transit event was identified, so the extrasolar planet was first classified as a candidate with TOI-6883.01 [1] nomenclature. The discovery describes a planet with a radius of 1.087 times that of Jupiter, but without details of the orbital period.
The planet was confirmed by the professional astronomers of SETI team led by Lauren Sgro, who fully characterised it using the radial velocity method and the orbital period was identified. TOI-6883 b revolves around its star in about 16.25 days at a distance of 0.123 AU (astronomical units) with a very eccentric orbit. [2]
Delphinus is a small constellation in the Northern Celestial Hemisphere, close to the celestial equator. Its name is the Latin version for the Greek word for dolphin (δελφίς). It is one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations recognized by the International Astronomical Union. It is one of the smaller constellations, ranked 69th in size. Delphinus' five brightest stars form a distinctive asterism symbolizing a dolphin with four stars representing the body and one the tail. It is bordered by Vulpecula, Sagitta, Aquila, Aquarius, Equuleus and Pegasus.
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Epsilon Eridani b, also known as AEgir [sic], is an exoplanet approximately 10.5 light-years away orbiting the star Epsilon Eridani, in the constellation of Eridanus. The planet was discovered in 2000, and as of 2024 remains the only confirmed planet in its planetary system. It orbits at around 3.5 AU with a period of around 7.6 years, and has a mass around 0.6 times that of Jupiter. As of 2023, both the Extrasolar Planets Encyclopaedia and the NASA Exoplanet Archive list the planet as 'confirmed'.
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WASP-121, also known as CD-38 3220 and formally named Dilmun, is a magnitude 10.4 star located approximately 858 light-years away in the constellation Puppis. WASP-121 has a mass and radius similar to the Sun's. It hosts one known exoplanet.
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TOI-1452 b is a confirmed super-Earth exoplanet, possibly a water world, orbiting a red-dwarf star TOI-1452 about 100 light-years away in the Draco constellation. The exoplanet is about 70% larger in diameter than Earth, and roughly five times as massive.
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