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трипскан
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Ci-dessous, les différences entre deux révisions de la page.
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трипскан [2025/07/10 17:45] 45.11.20.63 créée |
трипскан [2025/07/11 16:03] (Version actuelle) 46.8.110.226 |
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| ====== трипскан ====== | ====== трипскан ====== | ||
| - | An uncertain future | + | An uncertain future [[https://tripscan.info/|трипскан сайт]] |
| - | [[https://tripscan.info/|трипскан]] | + | |
| 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. | ||
| The newly found fossil galaxy joins a group of only a handful of others that have been observed at the same level of detail, the most pristine of which — called NGC 1277 — was confirmed by the Hubble Space Telescope in 2018. | The newly found fossil galaxy joins a group of only a handful of others that have been observed at the same level of detail, the most pristine of which — called NGC 1277 — was confirmed by the Hubble Space Telescope in 2018. | ||
трипскан.txt · Dernière modification: 2025/07/11 16:03 par 46.8.110.226
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