ESO研讨会“拉西拉天文台-从落成到未来”报告

IF 0.3 Q4 COMMUNICATION
I. Saviane, B. Leibundgut, L. Schmidtobreick
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引用次数: 0

摘要

智利天文台的历史背景是由Católica de Chile Pontificia university的Bárbara Silva给出的。美国天文学家最早的天文观测地点是在19世纪末和20世纪初进行的,他们确定了位于Copiapó附近和拉塞雷纳北部的阿塔卡马沙漠是夜间观测的潜在绝佳地点。1958年的国际地球物理年再次引起了美国天文学家的注意,j rgen Stock(最初为芝加哥大学工作,后来为天文学大学研究协会工作)进行的现场勘探发现,Vicuña周围的山脉可能是天文台的地点。在美国国家科学基金会选择Cerro Tololo作为他们的南站之后,ESO也产生了兴趣(通过Stock的前顾问Otto Heckmann,当时的ESO总干事)。这与把ESO天文台放在非洲南部的最初计划相比,是一个相当突然的变化。几年内,拉西拉山被选中并开发。席尔瓦在演讲结束时展示了一张邮票,邮票上是智利邮政于1973年发行的ESO 1米望远镜。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Report on the ESO Workshop "The La Silla Observatory — From Inauguration to the Future"
The historical context of astronomical observatories in Chile was given by Bárbara Silva from the Pontificia Universidad Católica de Chile. The earliest astronomical site explorations by US astronomers were carried out around the end of the 19th and the beginning of the 20th centuries and identified the Atacama Desert around Copiapó and north of La Serena as potentially excellent sites for nighttime observations. The International Geophysical Year in 1958 brought the Chilean sites to the attention of American astronomers again and site explorations by Jürgen Stock — originally for the University of Chicago and later for the Association of Universities for Research in Astronomy (AURA) — identified mountains around Vicuña as possible observatory sites. After the US National Science Foundation selected Cerro Tololo as their southern station, ESO also became interested (through Stock’s former advisor Otto Heckmann, then ESO Director General). This was a rather abrupt change from the original plan to place the ESO observatory in southern Africa. Within a few years the La Silla mountain was selected and developed. Silva finished her presentation by displaying a stamp showing the ESO 1-metre telescope, which was issued by the Chilean Postal Office in 1973.
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Jurnal The Messenger
Jurnal The Messenger COMMUNICATION-
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