Wednesday, March 20, 2013

Palomar Observatory Visit



Found a video of the mirror cleaning process done by the team at the Palomar observatory from 2006.

As a supplement to the tour, I decided to look around to see what discoveries were made using the instruments at the Palomar observatory, and also to check what ongoing projects are being run through there.

The first methane Brown Dwarf was discovered Gliese 229B in 1995. It has discovered many of the dwarf planets on the outskirts of our solar system including Eris (which triggered events that lead to a new classification of planets known as dwarf planets of which Pluto was placed into), Sedna, Quaoar, and Orcus as well as around 40 other Kuiper belt objects. Discovery of comet Shoemaker-Levy 9 in 1993 which was the first celestial object that we were able to observe impacting another body in space that happened to be the atmosphere of a Jupiter. There have been many discovered supernova in distant galaxies here, and Fritz Zwicky gathered the first evidence of dark matter in the 1930’s.
From 1949-1958, the Palomar observatory began with their first major project to make a comprehensive photographic survey of the night sky. This project was known as POSS-I (Palomar Observatory Sky Survey). Here they scanned the night sky from a declination of +90 degrees to -27 degrees for all Right Ascensions.  With help from partners in Australia and Chile, they were able to extend the declination to  -45 degrees through two extension projects. This survey gave the first catalog of galaxy clusters which allowed for the structure of the Universe to be mapped. Merging galaxies, new globular clusters, and neighboring dwarf galaxies to our own were discovered along with the first optical identification of quasars.
Other projects followed this including a search for supernova from 1959-1975 that resulted in 183 exploding stars as well as others found in the plates created from the POSS-I. A series of surveys from 1960-1977 were also made that listed numerous asteroids within our solar system known as the Leiden survey. This resulted in the discovery of over 6000 asteroids spanning 35 nights of study. From 1962-1971, there was the proper motion survey that was conducted to determine the motion of stars that were discovered close to our own.
In 1985, the second night sky survey began (POSS-II) and lasted until the year 2000. It used advances in technology to capture the night sky in 3 different spectrums (blue, red, and infrared) and worked to move sky surveys into the digital age. Over 1billion stars, 50 million galaxies, 100 supernovae, dozens of asteroids and comets, over 100 quasars, and 20 thousand galaxy clusters were discovered through this second survey.
From 2001-2003, JPL worked on the Near Earth Asteroid Tracker Survey that resulted in the discovery of 189 asteroids near Earth and 20 comets.
Currently, the observatory is still in use and has not lost its value in the Astronomy community. It is currently in projects to observe gamma-ray bursts, exoplanets, quasars, blackholes, weather patterns on Saturn’s moon Titan, near-Earth asteroids, Kuiper belt objects, and a new sky survey known as Palomar Transient Factory (PTF), plus all the observations that scientists around the world can now make thanks to remote viewing resultant from the digital age.



Resources

2 comments:

  1. Thanks for finding all this info about the projects, and the video. That is quite some process. I, too, did a little research for my post because I couldn't remember much of what our tour guide said. But I didn't find what I was looking for. I did come across this cool link, though, if you are interested in other caltech research and black holes: http://www.black-holes.org/

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  2. 4 points. sometimes it doesn't take a big telescope to make a cool discovery. those all sky surveys were done with the 48" diameter telescope, not the 200".

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