"Manusia tanpa pertolongan Yang Maha Pencipta Alam Raya bagaikan butiran debu Cosmos" 
~Arip~ 
Frontiers and Controversies in Astrophysics
| Lecture 7 - Direct Imaging of Exoplanets | 
Overview:
Class begins with a problem on transits and learning what  information astronomers    obtain through observing them. For example, radii of stars can be  estimated.    Furthermore, applying the Doppler shift method, one can find the mass  of a    star. Finally, a star's density can be calculated. A second method  for identifying    planets around stars is introduced: the astrometry method. The method  allows    for an extremely accurate assessment of a star's precise position in  the sky.    Special features of the astrometry method are discussed and a number  of problems    are solved. A short summary is given on the three methods astronomers  use    to identify exoplanets. Class ends with an overview of upcoming space  missions     and the hope of detecting the presence of biological activity on  other planet.
Problem sets/Reading assignment:
None assignedCourse Media
Transcript
htmlAudio
mp3Low Bandwidth Video
mov [100MB]High Bandwidth Video
mov [500MB]Resources:
Class Notes - Lecture 7 [PDF]Midterm Exam 1 Preparation Handout [PDF]
Sample Midterm Exam (2006) [PDF]
Test "Article" for Sample Midterm (2006) [PDF]
Sample Midterm Exam Solutions (2006) [PDF]
Section Activity 2: Planet Density [PDF]
Section Activity 2: Planet Density Answers [PDF]
Sumber:
1. The University of Yale Open Course Ware
2. Professor Bailyn's guide to Extrasolar Planet Websites
http://www.astro.yale.edu/bailyn/astro160/planets.html
Ucapan Terima Kasih:
1. Bapak. Prof. Dr. Ing. H. B. J. Habibie.
2. Departemen Pendidikan Nasional
3. Kementrian Riset dan Teknologi
4. Lembaga Penerbangan dan Antariksa Nasional
Disusun Ulang Oleh:
Arip Nurahman
Department of Physics, Indonesia University of Education
&
Follower Open Course Ware at MIT-Harvard University, Cambridge. U.S.A.
Semoga Bermanfaat dan Terima Kasih
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