How Many Habitable Planets are Out There?

Kepler-186f was the first rocky planet to be found within the habitable zone — the region around the host star where the temperature is right for liquid water. This planet is also very close in size to Earth. Even though we may not find out what’s going on at the surface of this planet anytime soon, it’s a strong reminder of why new technologies are being developed that will enable scientists to get a closer look at distant worlds. (Credits: NASA Ames/SETI Institute/JPL-Caltech)

MOUNTAIN VIEW, Calif. (SETI Institute PR) – Thanks to new research using data from the Kepler space telescope, it’s estimated that there could be as many as 300 million potentially habitable planets in our galaxy. Some could even be pretty close, with several likely within 30 light-years of our Sun. The findings will be published in The Astronomical Journal, and research was a collaboration of scientists from NASA, the SETI Institute, and other organizations worldwide.

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Carbon-rich Exoplanets Might be Made of Diamonds

llustration of a carbon-rich planet with diamond and silica as main minerals. Water can convert a carbide planet into a diamond-rich planet. In the interior, the main minerals would be diamond and silica (a layer with crystals in the illustration). The core (dark blue) might be iron-carbon alloy. (Credit: Shim/ASU/Vecteezy)

TEMPE, Ariz. (Arizona State University PR) — As missions like NASA’s Hubble Space Telescope, TESS  and Kepler continue to provide insights into the properties of exoplanets (planets around other stars), scientists are increasingly able to piece together what these planets look like, what they are made of and if they could be habitable or even inhabited.

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Fifty New Planets Confirmed in Machine Learning First

  • New machine learning algorithm designed by astronomers and computer scientists from University of Warwick confirms new exoplanets in telescope data
  • Sky surveys find thousands of planet candidates, and astronomers have to separate the true planets from fake ones
  • Algorithm was trained to distinguish between signs of real planets and false positives
  • New technique is faster than previous techniques, can be automated, and improved with further training

WARWICK, UK (University of Warwick PR) — Fifty potential planets have had their existence confirmed by a new machine learning algorithm developed by University of Warwick scientists.

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NASA’s Planet Hunter Completes Its Primary Mission

TESS exoplanet satellite (Credit: NASA)

by Francis Reddy
NASA’s Goddard Space Flight Center

Greenbelt, Md. — On July 4, NASA’s Transiting Exoplanet Survey Satellite (TESS) finished its primary mission, imaging about 75% of the starry sky as part of a two-year-long survey. In capturing this giant mosaic, TESS has found 66 new exoplanets, or worlds beyond our solar system, as well as nearly 2,100 candidates astronomers are working to confirm.  

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NASA’s TESS Delivers New Insights Into an Ultrahot World

This illustration shows how planet KELT-9 b sees its host star. Over the course of a single orbit, the planet twice experiences cycles of heating and cooling caused by the star’s unusual pattern of surface temperatures. Between the star’s hot poles and cool equator, temperatures vary by about 1,500 F (800 C). This produces a “summer” when the planet faces a pole and a “winter” when it faces the cooler midsection. So every 36 hours, KELT-9 b experiences two summers and two winters. [Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA)]

By Francis Reddy
NASA’s Goddard Space Flight Center

Greenbelt, Md. — Measurements from NASA’s Transiting Exoplanet Survey Satellite (TESS) have enabled astronomers to greatly improve their understanding of the bizarre environment of KELT-9 b, one of the hottest planets known.

“The weirdness factor is high with KELT-9 b,” said John Ahlers, an astronomer at Universities Space Research Association in Columbia, Maryland, and NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “It’s a giant planet in a very close, nearly polar orbit around a rapidly rotating star, and these features complicate our ability to understand the star and its effects on the planet.”

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NASA’s TESS, Spitzer Missions Discover a World Orbiting a Unique Young Star

This illustration depicts one interpretation of the planet AU Mic b and its young red dwarf host star. The system lies about 32 light-years away in the southern constellation Microsopium. [Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA).]

GREENBELT, Md. (NASA PR) — For more than a decade, astronomers have searched for planets orbiting AU Microscopii, a nearby star still surrounded by a disk of debris left over from its formation. Now scientists using data from NASA’s Transiting Exoplanet Survey Satellite (TESS) and retired Spitzer Space Telescope report the discovery of a planet about as large as Neptune that circles the young star in just over a week.

The system, known as AU Mic for short, provides a one-of-a-kind laboratory for studying how planets and their atmospheres form, evolve and interact with their stars.

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A Mirror Image of Earth and Sun

This artist’s concept depicts select planetary discoveries made to date by NASA’s Kepler space telescope. (Credit: NASA/W. Stenzel)

The star Kepler-160 and its companion KOI-456.04 are more reminiscent of the Sun-Earth system than any previously known exoplanet-star pair

Göttingen, Germany (Max Planck Institute PR) — The star Kepler-160 is probably orbited by a planet less than twice the size of the Earth with a star-planet distance that could permit planetary surface temperatures conducive to life. The newly discovered exoplanet, which was found by a team of scientists led by the Max Planck Institute for Solar System Research (MPS) in Göttingen is more than just another potentially habitable world.

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NASA’s TESS Presents Panorama of Southern Sky

GREENBELT, Md. (NASA PR) — The glow of the Milky Way — our galaxy seen edgewise — arcs across a sea of stars in a new mosaic of the southern sky produced from a year of observations by NASA’s Transiting Exoplanet Survey Satellite (TESS). Constructed from 208 TESS images taken during the mission’s first year of science operations, completed on July 18, the southern panorama reveals both the beauty of the cosmic landscape and the reach of TESS’s cameras.

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NASA Instrument to Probe Planet Clouds on European Mission

This artist’s concept shows the European Space Agency’s ARIEL spacecraft on its way to Lagrange Point 2 (L2) — a gravitationally stable, Sun-centric orbit — where it will be shielded from the Sun and have a clear view of the sky. NASA’s JPL will manage the mission’s CASE instrument. (Credits: ESA/STFC RAL Space/UCL/Europlanet-Science Office)

PASADENA, Calif. (NASA PR) — NASA will contribute an instrument to a European space mission that will explore the atmospheres of hundreds of planets orbiting stars beyond our Sun, or exoplanets, for the first time.

The instrument, called the Contribution to ARIEL Spectroscopy of Exoplanets, or CASE, adds scientific capabilities to ESA’s (the European Space Agency’s) Atmospheric Remote-sensing Infrared Exoplanet Large-survey, or ARIEL, mission.

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NASA’s TESS Mission Scores ‘Hat Trick’ With 3 New Worlds

This infographic illustrates key features of the TOI 270 system, located about 73 light-years away in the southern constellation Pictor. The three known planets were discovered by NASA’s Transiting Exoplanet Survey Satellite through periodic dips in starlight caused by each orbiting world. Insets show information about the planets, including their relative sizes, and how they compare to Earth. Temperatures given for TOI 270’s planets are equilibrium temperatures, calculated without the warming effects of any possible atmospheres. (Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger)

By Francis Reddy
NASA’s Goddard Space Flight Center

GREENBELT, Md. (NASA PR) — NASA’s newest planet hunter, the Transiting Exoplanet Survey Satellite (TESS), has discovered three new worlds — one slightly larger than Earth and two of a type not found in our solar system — orbiting a nearby star. The planets straddle an observed gap in the sizes of known planets and promise to be among the most curious targets for future studies.

TESS Object of Interest (TOI) 270 is a faint, cool star more commonly identified by its catalog name: UCAC4 191-004642. The M-type dwarf star is about 40% smaller than the Sun in both size and mass, and it has a surface temperature about one-third cooler than the Sun’s. The planetary system lies about 73 light-years away in the southern constellation of Pictor.

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NASA’s TESS Mission Completes First Year of Survey, Turns to Northern Sky

llustration of L 98-59b, the smallest exoplanet discovered by NASA’s Transiting Exoplanet Survey Satellite. (Credit: NASA’s Goddard Space Flight Center/Ravyn Cullor)

By Ravyn Cullor
NASA’s Goddard Space Flight Center

GREENBELT, Md. (NASA PR) — NASA’s Transiting Exoplanet Survey Satellite (TESS) has discovered 21 planets outside our solar system and captured data on other interesting events occurring in the southern sky during its first year of science. TESS has now turned its attention to the Northern Hemisphere to complete the most comprehensive planet-hunting expedition ever undertaken.

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