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WD 1202−232 (LP 852-7) metal-polluted single candidate 1–7 11.47 direct imaging 2024 similar to solar system giant planets in age and separation [39] WD 2105−82 (LAWD 83) metal-polluted single candidate 1–2 34.62 direct imaging 2024 similar to solar system giant planets in age and separation [39] GALEX J071816.4+373139: massive single ...
A small sample of (candidate) exoplanets exist with a temperature below 500 K, which could be spectroscopically confirmed as Y-dwarfs in the future. These exoplanets are Epsilon Indi Ab (275 K), [31] WD 1202–232b, WD 2105–82b (both low temperature), [32] GALEX J071816.4+373139b (400 K), [33] and WD 0310–688b (248 +84 −61 K). [34]
Motion interpolation of seven images of the HR 8799 system taken from the W. M. Keck Observatory over seven years, featuring four exoplanets. This is a list of extrasolar planets that have been directly observed, sorted by observed separations.
One orbits around WD 1202−232 (LP 852-7) and the other around WD 2105−82 (LAWD 83). If confirmed they would be the first directly imaged planets that likely formed from circumstellar disk material, representing a new population of directly imaged giant planets that are more similar to solar system giants in age and probably also in their ...
A My Passport Essential SE Edition External Hard Drive with 1 TB capacity. My Passport is a series of portable external hard drives and solid state drives produced by Western Digital.
This spiral galaxy article is a stub. You can help Wikipedia by expanding it.
NGC 1090 is a barred spiral galaxy located in the constellation Cetus.. NGC 1090 has a pseudo inner ring. The disc has a very low surface brightness. NGC 1090 is not part of a galaxy group, even though it appears close to NGC 1087, M-77 (), NGC 1055, NGC 1073, and five other small irregular galaxies.
NGC 1052 is located at a distance of around 63 million light years from the Milky Way, [4] and has a LINER-type active galactic nucleus which signals the intense starburst activity in the galaxy's center [5] that were confirmed with observations with better resolution showing a number of star-forming regions and young star clusters.