500 likes | 533 Views
Prof. Adam Riess. Prof. Saul Perlmutter. Prof. Brian Schmidt. 宣告及讚詞 2006 年邵逸夫天文學獎 得獎人 2006 年邵逸夫天文學獎將平均分配予 索爾 ‧ 普密特 Saul Perlmutter 亞當 ‧ 利斯 Adam Riess 和 布萊 ‧ 施米茲 Brian Schmidt 為表彰他們發現宇宙膨脹的速度在增加,顯示即使沒有物質與任何輻射,空間的能量密度仍然大於零。. Precision Cosmology 精準 宇宙學.
E N D
Prof. Adam Riess Prof. Saul Perlmutter Prof. Brian Schmidt
宣告及讚詞 2006年邵逸夫天文學獎 得獎人 2006年邵逸夫天文學獎將平均分配予 索爾‧普密特 Saul Perlmutter 亞當‧利斯 Adam Riess 和布萊‧施米茲 Brian Schmidt 為表彰他們發現宇宙膨脹的速度在增加,顯示即使沒有物質與任何輻射,空間的能量密度仍然大於零。
Precision Cosmology 精準 宇宙學 Credit: James Wadsley, McMaster University, Hamilton, Ontario
Island Universe 島宇宙 Galaxy 星系 M81 M82 Credit: Johannes Schedler
Credit: Jerry Lodriguss Edwin Hubble 哈勃
Prism 稜鏡 Spectrum 光譜 Credit: www.bistr-o-mathik.org
Stellar Fingerprint 星際指紋 Spectral Lines 譜線 Credit: NOAO/AURA/NSF
接近 Blueshift 藍移 遠離 Redshift 紅移 Redshift 紅移 Blueshift 藍移 Credit: Addison Wesley
Expanding Universe膨脹宇宙 Cosmological Redshift 宇宙紅移 Credit: Alfred T. Kamajian
Big Bang 大爆炸 Inflation 暴脹 Credit: Shigemi Numazawa
Shape of the Universe 宇宙的形狀 Flat 平坦式 Closed 封閉式 Open 開放式 Credit: WMAP, Stuart Levy (National Center for Supercomputing Applications) and Tamara Munzner (Stanford University)
High-Z Supernova Search Team Supernova Cosmology Project VS 對奕
均速膨脹 減速膨脹 加速膨脹 ?????
Supernova Explosion 超新星爆發 Credit: ESA, NASA and Felix Mirabel
SN 1994D Type Ia SupernovaIa 型超新星 Credit: NASA, ESA, The Hubble Key Project Team, and The High-Z Supernova Search Team
Supernova Remnant - Cassiopeia A 超新星殘骸-仙后座 A Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration
Credit: European Space Agency and Justyn R. Maund (University of Cambridge)
Type Ia Supernovae as Standard Candle Ia 型超新星 作為 標準燭光 Credit: David Emmite
Supernova 超新星 1987A Credit: NASA, P. Challis, R. Kirshner (Harvard-Smithsonian Center for Astrophysics) and B. Sugerman (STScI)
Mauna Kea 基亞山 8.2m Subaru Telescope 昴宿望遠鏡 10m Keck Observatory 凱克天文台 Credit: Wei-Hao Wang
Looking To The End of Time 遙望時間的盡頭 Hubble Deep Field 哈勃深空 Astroarcheology 天文考古學 Credit: R. Williams (STScI), the Hubble Deep Field Team and NASA
Hubble Ultra Deep Field哈勃極度深空 Credit: NASA, ESA, S. Beckwith (STScI) and the HUDF Team
Zoo of Oddball Galaxies 古怪星系園 Credit: NASA, ESA, and S. Beckwith (STScI) and the HUDF Team
Data Fitting
2dF Redshift Survey A Census of the 1-Billion light Neighbourhood
Galaxy Cluster 星系團Abell 1689 Gravitational Lensing 重力透鏡 Credit: NASA, N. Benitez(JHU), T. Broadhurst(Hebrew Univ.), H. Ford(JHU), M. Clampin(STScI), G. Hartig(STScI), G. Illingworth (UCO/Lick Obs.) and the ACS Science Team and ESA
Dark Forces of Nature 自然的黑暗力量 Dark Matter 黑暗物質 Credit: ESA, NASA and Jean-Paul Kneib (Observatoire Midi-Pyrénées, France/Caltech, USA)
1E 0657-56 Bullet Cluster 子彈星系團 Credit: NASA, CXC, ESO, CfA, STScI, Magellan, U.Arizona, M.Markevitch, D.Clowe
Wilkinson Microwave Anisotropy Probe (WMAP) 威爾金森探測器 Credit: NASA, WMAP
Cosmic Background Radiation 宇宙背景輻射 Credit: WMAP Science Team
A Brief History of the Universe 宇宙簡史 Dark Energy Accelerated Expansion 黑暗能量加速膨脹 Development of Galaxies, Planets, etc. 星系、行星等形成 Afterglow Light Pattern 爆炸餘暉圖案 Inflation 暴脹 The Big Bang 大爆炸 WMAP 威爾金森 探測器 Dark Ages 黑暗時代 1st Stars 首批恆星 Expansion 膨脹 Birth 誕生 Now 現在 13.7 billion years 137億年 Credit: NASA/WMAP Science Team
Credit: Don Dixon, Dmitry Krasny, Lawerence M. Krauss, Max Tegmark
4% Ordinary Matter 22% Dark Matter 74% Dark Energy Credit: Princeton
Cosmological Constant 宇宙常數 Λ
Quintessence第五元素 Credit: Don Dixon
Credit: Jana Brenning, Robert R. Caldwell (Dartmouth College), Paul J.Steinhardt
Extra-dimension 多維時空
Supernova Remnant 超新星殘骸 RCW 86 Credit: NASA, CXC, Univ. of Utrecht, ESA, Univ. of Utrecht, J.Vink et al.