Un observatorio amateur para estudios profesionales.Estudios de Exoplanetas, fotometría de asteroides, supernovas, ocultación de objetos estelares, astrofotografía, el Observatorio Anunaki al servicio de astrónomos profesionales.
The Bode galaxy, also known as Spiral Galaxy M81 or NGC 3031, is a spiral galaxy located 12 million light years in the constellation Ursa Major. The Bode galaxy is presumed to contain approximately 250 billion stars, being slightly smaller Continue Reading
The galaxy Messier 105 (also known as Object Messier 105, M105 or NGC 3379) is an elliptical galaxy in the constellation Leo. It was discovered by Pierre Méchain in 1781. M105 is the brightest elliptical galaxy in the Leo I Continue Reading
Messier 95 (also known as M95 or NGC 3351) is a barred spiral galaxy about 38 million light years[citation needed] in the constellation Leo. It was discovered by Pierre Méchain in 1781 and cataloged by Charles Messier 4 days later. Continue Reading
Messier 96 (also known as NGC 3368) is a barred spiral galaxy 34 million light years away in the constellation Leo. It was discovered by Pierre Méchain in 1781. It is the brightest member of the M96 Galaxy Group and Continue Reading
The SNR IC 443 is located in the galactic anticenter direction, close to the galactic plane. Many objects lie in the same region of sky: the HII region S249, several young stars, and an older SNR (G189.6+3.3). Image obtained from Continue Reading
IC 1848 is a nebula located in our Milky Way that is also known as the Soul Nebula. It houses an immense number of stars, as well as open clusters. It is located in the Cassiopeia constellation, next to another Continue Reading
The Triangulum galaxy (also known as spiral galaxy M33, Messier Object 33, Messier 33, M33 or NGC 598) is a spiral galaxy located in the Triangulum constellation. With between 30,000 and 40,000 million stars, it is small compared to its Continue Reading
TOI-1181 b is a gas giant exoplanet that orbits an F-type star. Its mass is 1.18 Jupiters and it takes 2.1 days to complete one orbit of its star. Its discovery was announced in 2022. https://arxiv.org/abs/2201.09963 Observations of TOI-1181 b Continue Reading
The discovery of a brown dwarf (M2 = 67 ± 2MJ and R2 = 1.11 ± 0.03RJ) on an eccentric (e=0.3362 ± 0.0005), short period orbit (P = 7.200861±0.000005 days) transiting and occulting the M dwarf TOI-2119. The rotation period Continue Reading
TOI-564 b is a gas giant exoplanet that orbits a G-type star. Its mass is 1.463 Jupiters, it takes 1.7 days to complete one orbit of its star, and is 0.02734 AU from its star. Its discovery was announced in Continue Reading