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The ESO Supernova Planetarum & Visitor Centre is located at the Science Campus Garching. The campus is home to the Ludwig-Maximilians University of Munich and the Technical University of Munich, in addition to more than 80 independent scientific institutions and international science companies, 6 000 staff members and 14 000 students.
Paranal Observatory is an astronomical observatory operated by the European Southern Observatory (ESO). It is located in the Atacama Desert of Northern Chile on Cerro Paranal at 2,635 m (8,645 ft) altitude, 120 km (70 mi) south of Antofagasta.
On the Trail of a Cosmic Cat — ESO Photo Release; NGC 6334 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images; Astronomy Picture of the Day - Wide Angle: The Cat's Paw Nebula 2010 April 21; Cat's Paw Nebula at Constellation Guide
iras f21392-3423, 2masx j21421214-3409436, mcg-06-47-012, pgc 67199, eso 403- g 016 [1] NGC 7110 is a barred spiral galaxy in the constellation of Piscis Austrinus . Its velocity with respect to the cosmic microwave background is 5044 ± 20 km/s, which corresponds to a Hubble distance of 74.39 ± 5.22 Mpc (~243 million light-years ). [ 1 ]
NGC 6453 is a globular cluster approximately 37,000 light-years away from Earth in the constellation of Scorpius. [3] [2]The cluster is located approximately 1 kpc (~3,260 light-years) from the Galactic Center, [5] which results in confounded view of the cluster from the Solar System due to many intervening clouds of cosmic dust.
eso 291- g001, mcg-07-47-020, pgc 70588, vv 771 [1] NGC 7496 is a barred spiral galaxy located in the constellation Grus . It is located at a distance of about 60 million light-years from Earth, which, given its apparent dimensions, means that it is 75,000 light years across.
UGC 11861 is a barred spiral galaxy in the constellation of Cepheus.Its velocity with respect to the cosmic microwave background is 1334 ± 10 km/s, which corresponds to a Hubble distance of 19.68 ± 1.39 Mpc (~64.2 million light-years). [1]
HIP 65426 b, formally named Najsakopajk, [3] is a super-Jupiter exoplanet orbiting the star HIP 65426. It was discovered on 6 July 2017 by the SPHERE consortium using the Spectro-Polarimetric High-Contrast Exoplanet Research (SPHERE) instrument belonging to the European Southern Observatory (ESO), [5] [6] being the first planet discovered by the SPHERE instrument. [7]