Benutzer-Werkzeuge

Webseiten-Werkzeuge


трипскан

Unterschiede

Hier werden die Unterschiede zwischen zwei Versionen angezeigt.

Link zu dieser Vergleichsansicht

Beide Seiten der vorigen Revision Vorhergehende Überarbeitung
Nächste Überarbeitung
Vorhergehende Überarbeitung
трипскан [2025/08/23 02:42]
57.141.6.21 alte Version wiederhergestellt (2025/08/17 23:57)
трипскан [2025/08/25 05:16] (aktuell)
57.141.6.29 alte Version wiederhergestellt (2025/08/19 03:11)
Zeile 1: Zeile 1:
 ====== трипскан ====== ====== трипскан ======
-An uncertain future [[https://tripscan.info/|трип скан]]+An uncertain future [[https://tripscan.info/|трипскан вход]]
  
 Scientists initially identified KiDS J0842+0059 in 2018 using the VLT Survey Telescope (VST) at the Paranal Observatory in Chile. That observation revealed that the galaxy was populated by very old stars but only provided an estimate of its mass and size, so a more detailed observation was required to confirm it was a relic. The Large Binocular Telescope used for this confirmation can render very sharp images due to its ability to compensate for atmospheric turbulence, which otherwise can make it difficult for Earth-based telescopes to focus on distant objects. Scientists initially identified KiDS J0842+0059 in 2018 using the VLT Survey Telescope (VST) at the Paranal Observatory in Chile. That observation revealed that the galaxy was populated by very old stars but only provided an estimate of its mass and size, so a more detailed observation was required to confirm it was a relic. The Large Binocular Telescope used for this confirmation can render very sharp images due to its ability to compensate for atmospheric turbulence, which otherwise can make it difficult for Earth-based telescopes to focus on distant objects.
трипскан.1755909769.txt.gz · Zuletzt geändert: 2025/08/23 02:42 von 57.141.6.21