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原始链接: https://news.ycombinator.com/item?id=39673087
标题:网络哈勃:利用现代天文学技术了解宇宙距离
摘要:哈勃太空望远镜(HST)和斯皮策太空望远镜(Spitzer)一直是推进现代天文学的重要工具,为研究河外现象提供了前所未有的能力。 通过利用配备最先进仪器的天基望远镜的力量,我们已经能够探测宇宙最遥远的区域,观察最高频率的事件,并研究物质和暗物质的特性。 Among the major contributions provided by HST and Spitzer include the calibration of the Hubble diagram and measurements of the Hubble Constant。 Additionally, these missions have facilitated direct detections of protoplanetary disks, protostellar cores, active galactic nuclei, high redshift galaxies, Type Ia supernovae, gravitational lenses, galaxy clusters, and other important objects critical to understanding the evolution of structures in the universe。 通过这张海报展示,我们将探讨天文学家如何利用 HST 和斯皮策来研究宇宙结构形成及其后续生长过程的基本方面,包括揭示重子和非重子暗物质特性细节的观测、大质量晕的组装过程、 and the merger histories of galaxy clusters。 Finally, we will examine the latest results from ongoing and upcoming Joint Space-Ground Array (JSGA) campaigns aimed at studying these key features of cosmic large scale structure and its relationship to dark matter。
Keywords: Hubble Space Telescope, Spitzer Space Telescope, extragalactic phenomena, matter, dark matter, active galactic nucleus, high redshift galaxies, galaxy clusters, gravitational lens, galaxy cluster assembly, JSGA, Joint Space-Ground Array。
Introduction: Over the past several decades, astronomers have employed optical and near-IR techniques to establish the Hubble sequence and calibrate Hubble diagrams。 Such efforts revealed the existence of dark energy, dark matter, and dark matter halos, leading to an updated picture of cosmic structure formation in a flat universe (Riess et al。 , 1998; Perlmutter & Schmidt, 1999)。 然而,关于分配方面存在许多悬而未决的问题
It all started with knowing the distance from the earth to the sun. Nobody had a clue until Richer and Cassini got within 10% in 1672. Then we nailed it down in 1769 with James Cook's voyage to Tahiti, the primary purpose of which was to observe the transit of Venus from the other side of the world.
From there if you know basic geometry, you can observe the nearby stars shift a bit when the earth goes around the sun (parallax), but that only works to about 10k light years.
Then, we discovered a couple unbelievably convenient astrophysics hacks: Cepheid variables (Henrietta Swan Leavitt, 1908) and Type 1A supernovae (Subrahmanyan Chandrasekhar, 1935, the namesake of the Chandra X-Ray Observatory). These allowed us to move out a couple more rungs on the ladder.
From there, the relationship between redshift and distance becomes significant and that takes us to the edge.
https://www.uwa.edu.au/science/-/media/Faculties/Science/Doc...
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