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National Aeronautics and Space Administration




                                                                                                                                NASAfacts
             Kepler: NASA’s First Mission Capable of
             Finding Earth-Size Planets
             Kepler is the first space mission to search for Earth-   the drop in brightness when a gnat flies across a
             size planets in the habitable zone of other stars in     headlight seen from many miles away. Measuring
             our neighborhood of the galaxy. Kepler is a special-     repeated transits, with a regular period, duration
             purpose spacecraft that precisely measures the light     and change in brightness, enables the detection of
             variations from thousands of distant stars, looking      planets and their orbits. Kepler seeks planets the size
             for sequences of planetary transits. When a planet       of Earth in the habitable zone around other stars
             passes in front of its parent star, as seen from our     similar to our Sun.
             solar system, it blocks a small fraction of the light
             from that star—this is known as a transit. Searching     The centuries-old quest for other worlds like our
             for transits of distant “Earths” is like looking for     Earth has been rejuvenated in the past decade by
                                                                                              the intense excitement and
                                                                                              popular interest surrounding
                                                                                              the discovery of more than
                                                                                              400 giant planets orbiting
                                                                                              stars beyond our solar
                                                                                              system. With the exception
                                                                                              of the pulsar planets, most
                                                                                              of the extrasolar planets
                                                                                              detected to date are gas
                                                                                              giants like Jupiter. The
                                                                                              challenge is to find Earth-
                                                                                              like planets, which are 30-
                                                                                              600 times less massive than
                                                                                              Jupiter. Kepler is specifically
                                                                                              designed to search for
                                                                                              Earths in the habitable
                                                                                              zone of solar-like stars out
                                                                                              to distances of about three
                                                                                              thousand light years.

                                                                                               Expected Results
                                                                                               Kepler is monitoring over
                                                                                               100,000 stars similar to our
                                                                                               Sun for brightness changes
                                                                                               produced by planetary
                                                                                               transits. At the beginning
                                                                                               of the mission, planets of
                                                                                               all sizes orbiting very close
                                                                                               to their stars will be found.
                                                                                               After three years, the Kepler
                                                                                               scientists will be able to
                                                                                               discover planets with orbits
                                                                                               of one year, that is, those in
                                                                                               the habitable zone of stars
NASA Photo




                                                                                               like the Sun. If Earth-size
             NASA’s Kepler Mission launches, March 6, 2009.                                    planets in the habitable zone

             FS-2009-12-01-ARC                                                                                                       1209-2000
used are charged coupled devices (CCDs) similar to those found
                                                                             in consumer digital cameras. However, unlike an ordinary digital
                                                                             camera with a few megapixels, Kepler’s detector array has
                    planet
                                                                             95 megapixels.
                                          star
                                                                             Scientific Community Involvement
   brightness




                                                 light curve
                                                                             There are three ways for the broader scientific community to
                                                                             participate in the mission via NASA Research Opportunities.
                                  time                                       Scientists have been invited to propose to:
                                                                                  •	 Conduct complementary investigations that support the
Kepler will find planets by looking for tiny dips in the brightness of
                                                                                     planetary detection science of Kepler;
a star caused by planetary transits.
                                                                                  •	 Use Kepler to observe other types of astrophysically
                                                                                     interesting objects in its field of view, such as variable stars,
are common, then life may be ubiquitous in our galaxy. On the
                                                                                     quasars and galaxies; and
other hand, if no terrestrial planets are found, then “Earths” may
                                                                                  •	 Analyze the unique Kepler data archive for phenomena
be rare.
                                                                                     relating to stellar activity.
Three or more transits of a given star—all with a consistent                 The archive will contain many years of continuous observations of
period, brightness change and duration—provide a rigorous                    stars with unprecedented photometric precision. For example, such
method of detection and confirmation. The data reveal the                    data are useful for estimating how often stars like our Sun could
planet’s:                                                                    cause a climate change like that which brought on the mini-ice age
          •	 Size from the brightness change and size of the star;           in the 17th century.
          •	 Orbital period from the time between transits;                  Education and Public Outreach Program
          •	 Orbital size from the mass of the star, the period, and
                                                                             The EPO program leverages pre-existing collaborations, networks,
             using Kepler’s third law;
                                                                             and team experience to maximize the development and impact of
          •	 Temperature from the planet’s orbit and the temperature
                                                                             EPO products and activities. It includes:
             of the star.
                                                                                  •	 Formal Programs–Hands On Universe for grades 9-12; and
From these data, scientists can calculate the fraction of stars that
                                                                                     Great Explorations in Math and Science (GEMS) Space
have planets, and the distributions of planetary sizes and orbits
                                                                                     Science Sequence for grades 3-5 and 6-8. GEMS reaches
for many different types of stars.
                                                                                     thousands of teachers through over 80 GEMS sites/centers
The results will tell us how often planets occur in the habitable                    nationwide and worldwide;
zone of other stars. If common, then hundreds of Earth-size                       •	 Informal Programs–Exhibits and programs for science and
planets in the habitable zone and thousands outside the habitable                    technology museums and planetaria; and
zone will be detected.                                                            •	 Public Outreach Programs–Kits for amateur astronomers
                                                                                     via the Night Sky Network; nationally broadcast science
The Spacecraft                                                                       documentaries; and StarDate radio programs.
The Kepler spacecraft contains a single instrument called a                  Mission Organization and Status
photometer, that is, a light meter, which can simultaneously                 The Kepler Mission was competitively selected in December 2001 as
measure the brightness variations of over 100,000 stars with a               NASA’s tenth Discovery mission. NASA Ames Research Center is
precision of about 20 parts per million (ppm). This precision                responsible for the data analysis and scientific interpretation of the
allows detection of Earth-like transits, which cause a change in             data, the development of the ground system and management of the
brightness of 84 ppm of solar-like stars. The transits last for a            operations phase. NASA’s Jet Propulsion Laboratory managed the
few hours to about half of a day. The photometer is so sensitive             development phase. Ball Aerospace and Technologies Corporation
that planets as small as Mars can be detected when they occur                developed the photometer and spacecraft and supports mission
in short-period orbits, like those of many of the giant planets              operations.
already discovered. So as not to miss any transits, Kepler is staring
at the same star field in the Cygnus-Lyra region for the entire              Kepler Discovery Mission
mission.
                                                                             Science Principal Investigator          Project Manager
With an aperture of nearly one meter in diameter, Kepler is the              William Borucki                         Roger Hunter
largest Schmidt-type telescope ever launched. Schmidt optics                 NASA Ames Research Center               NASA Ames Research Center
have an unusually large field of view. The amount of sky viewed
is equivalent to an open hand held at arm’s length. The detectors            Learn more at the Kepler web site: http://kepler.nasa.gov

National Aeronautics and Space Administration
Ames Research Center
Moffett Field, California 94035 - 1000
www.nasa.gov

                                                                         2                Kepler: Finding Earth-Size Planets           NASA Facts

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Kepler: NASA’s First Mission Capable of Finding Earth-Size Planets (fact sheet)

  • 1. National Aeronautics and Space Administration NASAfacts Kepler: NASA’s First Mission Capable of Finding Earth-Size Planets Kepler is the first space mission to search for Earth- the drop in brightness when a gnat flies across a size planets in the habitable zone of other stars in headlight seen from many miles away. Measuring our neighborhood of the galaxy. Kepler is a special- repeated transits, with a regular period, duration purpose spacecraft that precisely measures the light and change in brightness, enables the detection of variations from thousands of distant stars, looking planets and their orbits. Kepler seeks planets the size for sequences of planetary transits. When a planet of Earth in the habitable zone around other stars passes in front of its parent star, as seen from our similar to our Sun. solar system, it blocks a small fraction of the light from that star—this is known as a transit. Searching The centuries-old quest for other worlds like our for transits of distant “Earths” is like looking for Earth has been rejuvenated in the past decade by the intense excitement and popular interest surrounding the discovery of more than 400 giant planets orbiting stars beyond our solar system. With the exception of the pulsar planets, most of the extrasolar planets detected to date are gas giants like Jupiter. The challenge is to find Earth- like planets, which are 30- 600 times less massive than Jupiter. Kepler is specifically designed to search for Earths in the habitable zone of solar-like stars out to distances of about three thousand light years. Expected Results Kepler is monitoring over 100,000 stars similar to our Sun for brightness changes produced by planetary transits. At the beginning of the mission, planets of all sizes orbiting very close to their stars will be found. After three years, the Kepler scientists will be able to discover planets with orbits of one year, that is, those in the habitable zone of stars NASA Photo like the Sun. If Earth-size NASA’s Kepler Mission launches, March 6, 2009. planets in the habitable zone FS-2009-12-01-ARC 1209-2000
  • 2. used are charged coupled devices (CCDs) similar to those found in consumer digital cameras. However, unlike an ordinary digital camera with a few megapixels, Kepler’s detector array has planet 95 megapixels. star Scientific Community Involvement brightness light curve There are three ways for the broader scientific community to participate in the mission via NASA Research Opportunities. time Scientists have been invited to propose to: • Conduct complementary investigations that support the Kepler will find planets by looking for tiny dips in the brightness of planetary detection science of Kepler; a star caused by planetary transits. • Use Kepler to observe other types of astrophysically interesting objects in its field of view, such as variable stars, are common, then life may be ubiquitous in our galaxy. On the quasars and galaxies; and other hand, if no terrestrial planets are found, then “Earths” may • Analyze the unique Kepler data archive for phenomena be rare. relating to stellar activity. Three or more transits of a given star—all with a consistent The archive will contain many years of continuous observations of period, brightness change and duration—provide a rigorous stars with unprecedented photometric precision. For example, such method of detection and confirmation. The data reveal the data are useful for estimating how often stars like our Sun could planet’s: cause a climate change like that which brought on the mini-ice age • Size from the brightness change and size of the star; in the 17th century. • Orbital period from the time between transits; Education and Public Outreach Program • Orbital size from the mass of the star, the period, and The EPO program leverages pre-existing collaborations, networks, using Kepler’s third law; and team experience to maximize the development and impact of • Temperature from the planet’s orbit and the temperature EPO products and activities. It includes: of the star. • Formal Programs–Hands On Universe for grades 9-12; and From these data, scientists can calculate the fraction of stars that Great Explorations in Math and Science (GEMS) Space have planets, and the distributions of planetary sizes and orbits Science Sequence for grades 3-5 and 6-8. GEMS reaches for many different types of stars. thousands of teachers through over 80 GEMS sites/centers The results will tell us how often planets occur in the habitable nationwide and worldwide; zone of other stars. If common, then hundreds of Earth-size • Informal Programs–Exhibits and programs for science and planets in the habitable zone and thousands outside the habitable technology museums and planetaria; and zone will be detected. • Public Outreach Programs–Kits for amateur astronomers via the Night Sky Network; nationally broadcast science The Spacecraft documentaries; and StarDate radio programs. The Kepler spacecraft contains a single instrument called a Mission Organization and Status photometer, that is, a light meter, which can simultaneously The Kepler Mission was competitively selected in December 2001 as measure the brightness variations of over 100,000 stars with a NASA’s tenth Discovery mission. NASA Ames Research Center is precision of about 20 parts per million (ppm). This precision responsible for the data analysis and scientific interpretation of the allows detection of Earth-like transits, which cause a change in data, the development of the ground system and management of the brightness of 84 ppm of solar-like stars. The transits last for a operations phase. NASA’s Jet Propulsion Laboratory managed the few hours to about half of a day. The photometer is so sensitive development phase. Ball Aerospace and Technologies Corporation that planets as small as Mars can be detected when they occur developed the photometer and spacecraft and supports mission in short-period orbits, like those of many of the giant planets operations. already discovered. So as not to miss any transits, Kepler is staring at the same star field in the Cygnus-Lyra region for the entire Kepler Discovery Mission mission. Science Principal Investigator Project Manager With an aperture of nearly one meter in diameter, Kepler is the William Borucki Roger Hunter largest Schmidt-type telescope ever launched. Schmidt optics NASA Ames Research Center NASA Ames Research Center have an unusually large field of view. The amount of sky viewed is equivalent to an open hand held at arm’s length. The detectors Learn more at the Kepler web site: http://kepler.nasa.gov National Aeronautics and Space Administration Ames Research Center Moffett Field, California 94035 - 1000 www.nasa.gov 2 Kepler: Finding Earth-Size Planets NASA Facts