Automated Planet Finder
The telescope uses high-precision radial velocity measurements to measure the gravitational reflex motion of nearby stars caused by the orbiting of planets. The design goal is to detect stellar motions as small as one meter per second, comparable to a slow walking speed. The main targets will be stars within about 100 light years of the Earth.
Early tests show that the performance of the Ken and Gloria Levy Doppler Spectrometer is meeting the design goals. The spectrometer has high throughput and is meeting the design sensitivity of (1.0 m/s), similar to the radial velocity precision of HARPS and HIRES.
Construction
Parts for the telescopes were constructed by international companies:
- The mirror blank was cast in Russia.
- The blank was optical figured in Maryland, USA.
- Assembly was performed in Arizona, USA.
- The dome was built in Australia.
- The spectrograph was designed and built in California.
- It is located on Mount Hamilton in California.
Collaboration with Breakthrough Listen
The telescope is also being used to search for optical signals coming from laser transmissions from hypothetical extraterrestrial civilizations (search for extraterrestrial intelligence - SETI). This undertaking is performed for the heavily funded Breakthrough Listen project of the Berkeley SETI Research Center.
See also
References
- ^ "Telescopes of the Lick Observatory". University of California Observatories. 2015. Retrieved 2016-08-23.
- ^ Steven S. Vogt et al., APF - The Lick Observatory Automated Planet Finder, 26 February 2014.
- ^ Powell, Hugh. "Major gift supports crucial piece of Automated Planet Finder". UC Santa Cruz. Archived from the original on 2008-06-13.
- ^ Perlman, David (August 21, 2010). "Automated Planet Finder telescope seeks life". San Francisco Chronicle.
- ^ UCO Director Newsletters: Newsletter #6 October 2009
- ^ "Mt. Hamilton Telescopes: Carnegie Double Astrograph".
- ^ Zhang, Sarah (20 July 2015). "A Russian Tycoon Is Spending $100 Million to Hunt for Aliens". Wired.