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.
NGC 5907 is a spiral galaxy in the constellation Draco located 40 million light-years away. Of apparent magnitude 10.38, its surface brightness is 13.4 mag/arcsec. It was discovered by William Herschel in 1788. NGC 5907 appears edge-on from our perspective, Continue Reading
Messier 94, also known as NGC 4736 is a spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781, and catalogued by Charles Messier 2 days later. The structure of M94 is characterized by three Continue Reading
The Whirlpool Galaxy, also known as Object Messier 51, is a classic spiral galaxy located in the constellation Canes Venatici (hunting dog). It is one of the best-known spiral galaxies in the sky. The famous “Whirlpool galaxy” or Messier 51 Continue Reading
NGC 4559 is a spiral galaxy located in the Coma Berenices constellation within reach of amateur telescopes, at a distance of between 20 and 35 million light years (more possibly the latter distance based on its redshift). It is a Continue Reading
NGC 4565, also known as the Needle Galaxy, is a spiral galaxy located in the constellation of Coma Berenices at a distance of 47 million light years, easily visible with small telescopes. It is a member of the Coma I Continue Reading
The Owl Nebula, also known as Messier 97 or NGC 3587, is a planetary nebula located in the constellation Ursa Major. It was discovered by Pierre Méchain in 1781. The name Owl Nebula was coined by Lord Rosse, who first Continue Reading
M108 is a spiral galaxy of type Sc in the constellation Ursa Major. Shown almost in profile, this shows little or no prominence or bulb with no strongly noticeable center, being a heterogeneous collection of features referred to as very Continue Reading
CTB 1 is a supernova remnant located in the Cassiopeia constellation. It is thought to be the remnants of a massive star that underwent a supernova explosion, expelling its outer layers into the interstellar medium and leaving behind a compact Continue Reading
Messier 106 (also known as NGC 4258) is an intermediate spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781. M106 is at a distance of about 22 to 25 million light-years away from Earth. Continue Reading
NGC 1499 is an emission nebula in the constellation Perseus 1000 light years away. It is located south of the constellation. Due to its shape, it is also called the California Nebula, since it remembers the outline of that state Continue Reading