A cosmic quartet
Space can be a lonely place. But not so for this quartet of galaxies making up HCG 86 and observed here with ESO’s VLT Survey Telescope (VST). The four galaxies located approximately 270 million light years from Earth in the Sagittarius constellation, are seen from Earth as arranged in triangular shape, with three of them on a straight line and one underneath; the bright objects to the right of the elongated galaxy are not part of the quartet.
HCG stands for Hickson Compact Group, and is used to describe groups of four to ten galaxies where members are physically very close to each other. Because of their compactness, such groups are ideal environments to study galactic interactions, which can sometimes lead to galaxies merging with each other.
This image of HCG 86 was taken by a team of astronomers led by Rossella Ragusa of the Istituto Nazionale di Astrofisica in Italy as part of the VST Early-type Galaxy Survey (VEGAS) programme. “With VST we are able to investigate very faint structures in the galaxies' outskirts, which are the relics of past gravitational interactions and merging events,” says Ragusa. In particular, by mapping the light distribution in and around the group’s galaxies in this study, the team concluded that these faint structures are the leftovers of satellite galaxies gobbled by the group approximately seven billion years ago.
Located at ESO’s Paranal Observatory in Chile, the VST is one of the world’s largest survey telescopes, devoted to mapping the sky in visible light wavelengths. 2021 marks the anniversary of its first decade of operation, a period during which it has helped to search for planets outside the Solar System and probe the structure of our galaxy and the wider Universe.Telif:
ESO/Ragusa, Spavone et al.
|Yayın tarihi:||26 Temmuz 2021 06:00|
|Boyut:||4691 x 3229 px|
|Tür:||Local Universe : Galaxy : Type : Interacting|
|Uzaklık:||270 milyon ışık yılı|
|Position (RA):||19 51 59.28|
|Position (Dec):||-30° 49' 32.80"|
|Field of view:||15.64 x 10.76 arcminutes|
|Yönelim:||Kuzey yönü -0.0° sol derece kadar dik konumdan sapma göstermektedir|
Renkler & Filtreler
|480 nm||VLT Survey Telescope|
|625 nm||VLT Survey Telescope|
|770 nm||VLT Survey Telescope|