The detection algorithms crafted by Jenkins and his colleagues, first identify and remove known sources of stellar oscillation, then uses an adaptive, wavelet-based matched filter to remove the non-white (1/f) noise typical of starlight. As a result, Kepler can accurately measure the minuscule dip in a star's light output when an orbiting planet circles in front of its side facing Earth.
Called the "transit" method, Kepler constantly records the output from over 100,000 stars in its 18 degree field of view, and can typically detect the dip in luminosity caused by an Earth-sized planet with about 6-1/2 hours of observation. Unfortunately, a typical habitable planet circling a solar-like star only orbits it about once a year, and since three transits are needed to verify a planet's presence, Kepler was given a three and half year mission time—six months to spot the 1,235 planets it is now tracking and three more years of constant observation to verify that they indeed are planets and not anomalies. (Other telescopes, including the Spitzer Space Telescope, are also being enlisted to perform the verification task on the 1,235 candidates.)
Once a planet is detected, its signature can be analyzed from the variation in the stars' output—especially when the planet is just passing by the edge of the star at which point its atmosphere can be analyzed for Earth-like qualities. From its period, a planet's orbital size can be calculated as well as the mass of the star (using Johannes Kepler's Third Law, after which the spacecraft was named). The amount of the star's brightness dip reveals the size of the planet, which together with its orbit size and the temperature of the star reveals the temperature of the planet itself.
Artist's rendition of Kepler spacecraft.
Credit: NASA/Kepler mission/Wendy Stenzel
Kepler hardware consists of a nearly one-meter wide Schmidt mirror-style visible-light telescope with a giant image array at its focal point, consisting of 42 charge coupled devices (CCDs) each housing over 2.25 million pixels for a total of 95 mega pixels. To allow constant monitoring, Kepler was put into an orbit that prevents our sun or moon from obstructing its view. And in a final concession to meet its budgetary constraints, its orientation was made single-purpose—Kepler will always point in its current direction, even after it completes its primary mission in November 2012. (However, at current consumption levels, Kepler will likely operate for a total of 10 years).
Now that Kepler has located an abundance of candidates, groups affiliated with the Search for Extraterrestrial Intelligence (SETI) are aiming their radio telescopes specifically at the detected planets to look for sinusoidal waveforms in the 1-to-11 GHz range where nature seems never to tread. In particular, the Allen Telescope Array operated by the SETI Institute plans to begin looking for the trademark signature of alien civilizations starting next month.
Thank you for the article and the specs - it is amazing that just this little spot in just this one little galaxy is producing so much - especially when this device with it's current algorithms - I am sure they will be improved - has a limited resolution, and will not see any planets like our own. I am not even sure it any of our planets would be seen although perhaps Saturn and Jupiter would (this would be nice to know). Regarding the uniqueness of Earth - I don't buy it as the one thing we have learned as we actually learn about the cosmos is how insignificant we are - can we really be alone?
It is just awesome to see continued success of NASA projects, if we could contemplate the odds of probabilities and the scale of space, distance, and time scales been are considered; for 2 civilizations to be aware of each other.
It is so remote that my head spins in just tinking of the possibilities...
Great research. I'm very interested in everything we can learn about our universe, even though I don't believe for a second that this will make any difference for finding other intelligent life. Most people don't seem to realize how unique our planet is. I highly doubt there is even 1 among those 988 planets that could support life if it was transplanted there. Let alone that it could develop by accident--a still completely unproven idea, and not for lack of trying.
While it is a disappointment that we are out of the manned space flight business for the moment, I can't fathom seeing our total space program as being anything but an incredible amount of scientific success.
It blows my mind to consider that we can detect planets at such staggering distances.
This is something mind boggling. Hats of to those engineers to first conceptualize such a instrument and building the same!
With persistent efforts like this we will sure find some response to our quest for the life elsewhere in this universe.
Very informative article with technical details and beautiful pictures. Good to see the success achieved by the scientists and the angineers in making new discoveries by means of technological advancements.
Again, US$500 million is a great amount of money! :)
A great news from NASA and SETI. Many planets in space and there will be life in many. THe scientists at NASA and SETI are doing it so finely. 21st centuary will identifi Alien family and make friends with them.
David Patterson, known for his pioneering research that led to RAID, clusters and more, is part of a team at UC Berkeley that recently made its RISC-V processor architecture an open source hardware offering. We talk with Patterson and one of his colleagues behind the effort about the opportunities they see, what new kinds of designs they hope to enable and what it means for today’s commercial processor giants such as Intel, ARM and Imagination Technologies.