Δημοσιεύτηκε στις 28 Οκτ 2016
From
2009 through 2015, the SETI Institute used the Allen Telescope Array to
observe stars with high probability of hosting exoplanets. Nearby stars
were chosen based on radial velocity observations that indicate
planets, and a more distant set of stars were chosen from the Kepler
Space Telescope's list of probable and confirmed exoplanets. By
choosing stars that have planets we hoped to improve our chances for
finding ET in our radio telescope observations. In this talk Dr. Harp
will describe the novel technologies developed for this search by the
SETI Institute and what we have learned from the last six years of SETI
observations. Dr. Harp will also consider future directions the SETI
Institute may take to improve on this search in the coming years.
2009 through 2015, the SETI Institute used the Allen Telescope Array to
observe stars with high probability of hosting exoplanets. Nearby stars
were chosen based on radial velocity observations that indicate
planets, and a more distant set of stars were chosen from the Kepler
Space Telescope's list of probable and confirmed exoplanets. By
choosing stars that have planets we hoped to improve our chances for
finding ET in our radio telescope observations. In this talk Dr. Harp
will describe the novel technologies developed for this search by the
SETI Institute and what we have learned from the last six years of SETI
observations. Dr. Harp will also consider future directions the SETI
Institute may take to improve on this search in the coming years.
Κατηγορία
Άδεια
- Τυπική άδεια YouTube
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