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Topic: NASA’s Transiting Exoplanet Survey Satellite

NASA Kepler Space Telescope data reveals around Half of Sun Like Stars could have Rocky, Potentially Habitable Planets

 

NASA - National Aeronautics and Space AdministrationMountain View, CA – Since astronomers confirmed the presence of planets beyond our solar system, called exoplanets, humanity has wondered how many could harbor life. Now, we’re one step closer to finding an answer.

According to new research using data from NASA’s retired planet-hunting mission, the Kepler space telescope, about half the stars similar in temperature to our Sun could have a rocky planet capable of supporting liquid water on its surface.

This illustration depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone. (NASA Ames/JPL-Caltech/T. Pyle)

This illustration depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone. (NASA Ames/JPL-Caltech/T. Pyle)

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NASA’s TESS Satellite images used to create Northern Sky Panorama

 

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – NASA’s Transiting Exoplanet Survey Satellite (TESS) has discovered 74 exoplanets, or worlds beyond our solar system. Astronomers are sifting through some 1,200 additional exoplanet candidates, where potential new worlds await confirmation. More than 600 of these candidates lie in the northern sky.

TESS locates planets by simultaneously monitoring many stars over large regions of the sky and watching for tiny changes in their brightness. When a planet passes in front of its host star from our perspective, it blocks some of the star’s light, causing it to temporarily dim.

This detail of the TESS northern panorama features a region in the constellation Cygnus. At center, the sprawling dark nebula Le Gentil 3, a vast cloud of interstellar dust, obscures the light of more distant stars. A prominent tendril extending to the lower left points toward the bright North America Nebula, glowing gas so named for its resemblance to the continent. (NASA/MIT/TESS and Ethan Kruse (USRA))

This detail of the TESS northern panorama features a region in the constellation Cygnus. At center, the sprawling dark nebula Le Gentil 3, a vast cloud of interstellar dust, obscures the light of more distant stars. A prominent tendril extending to the lower left points toward the bright North America Nebula, glowing gas so named for its resemblance to the continent. (NASA/MIT/TESS and Ethan Kruse (USRA))

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NASA may have discovered a Planet orbiting a White Dwarf

 

NASA - National Aeronautics and Space AdministrationPasadena, CA – An international team of astronomers using NASA’s Transiting Exoplanet Survey Satellite (TESS) and retired Spitzer Space Telescope has reported what may be the first intact planet found closely orbiting a white dwarf, the dense leftover of a Sun-like star, only 40% larger than Earth.

The Jupiter-size object, called WD 1856 b, is about seven times larger than the white dwarf, named WD 1856+534. It circles this stellar cinder every 34 hours, more than 60 times faster than Mercury orbits our Sun.

WD 1856 b, a potential planet the size of Jupiter, orbits its dim white dwarf star every 36 hours and is about seven times larger. (NASA's Goddard Space Flight Center)

WD 1856 b, a potential planet the size of Jupiter, orbits its dim white dwarf star every 36 hours and is about seven times larger. (NASA’s Goddard Space Flight Center)

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NASA’s Transiting Exoplanet Survey Satellite observes new details about Ultrahot World

 

NASA - National Aeronautics and Space AdministrationGreenbelt, 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.”

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). (NASA's Goddard Space Flight Center/Chris Smith (USRA))

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). (NASA’s Goddard Space Flight Center/Chris Smith (USRA))

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NASA’s TESS Satellite, Spitzer Space Telescope find Large World Orbiting Young Star

 

NASA - National Aeronautics and Space AdministrationPasadena, CA – 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 NASA’s 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-kind laboratory for studying how planets and their atmospheres form, evolve and interact with their stars.

This image is an artist's concept of the planet AU Mic b and its young parent star. The faint band of light encircling the pair is a disk of gas and dust from which both the star and the planet formed. (NASA's Goddard Space Flight Center/Chris Smith (USRA))

This image is an artist’s concept of the planet AU Mic b and its young parent star. The faint band of light encircling the pair is a disk of gas and dust from which both the star and the planet formed. (NASA’s Goddard Space Flight Center/Chris Smith (USRA))

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NASA says Young Giant Planets could help answer questions on how Planets Form

 

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA says that for most of human history our understanding of how planets form and evolve was based on the eight (or nine) planets in our solar system. But over the last 25 years, the discovery of more than 4,000 exoplanets, or planets outside our solar system, changed all that.

Among the most intriguing of these distant worlds is a class of exoplanets called hot Jupiters. Similar in size to Jupiter, these gas-dominated planets orbit extremely close to their parent stars, circling them in as few as 18 hours.

This image shows a type of gas giant planet known as a hot Jupiter that orbits very close to its star. Finding more of these youthful planets could help astronomers understand how they formed and if they migrate from cooler climes during their lifetimes. (NASA/JPL-Caltech)

This image shows a type of gas giant planet known as a hot Jupiter that orbits very close to its star. Finding more of these youthful planets could help astronomers understand how they formed and if they migrate from cooler climes during their lifetimes. (NASA/JPL-Caltech)

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NASA’s WFRIST telescope to search for Exoplanets using Microlensing

 

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – NASA’s Wide Field Infrared Survey Telescope (WFIRST) will search for planets outside our solar system toward the center of our Milky Way galaxy, where most stars are. Studying the properties of exoplanet worlds will help us understand what planetary systems throughout the galaxy are like and how planets form and evolve.

Combining WFIRST’s findings with results from NASA’s Kepler and Transiting Exoplanet Survey Satellite (TESS) missions will complete the first planet census that is sensitive to a wide range of planet masses and orbits, bringing us a step closer to discovering habitable Earth-like worlds beyond our own.

NASA's WFIRST will make its microlensing observations in the direction of the center of the Milky Way galaxy. The higher density of stars will yield more exoplanet detections. (NASA's Goddard Space Flight Center/CI Lab)

NASA’s WFIRST will make its microlensing observations in the direction of the center of the Milky Way galaxy. The higher density of stars will yield more exoplanet detections. (NASA’s Goddard Space Flight Center/CI Lab)

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NASA uses Earth Climate Models to Picture Life on Unimaginable Worlds

 

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – In a generic brick building on the northwestern edge of NASA’s Goddard Space Flight Center campus in Greenbelt, Maryland, thousands of computers packed in racks the size of vending machines hum in a deafening chorus of data crunching. Day and night, they spit out 7 quadrillion calculations per second.

These machines collectively are known as NASA’s Discover supercomputer and they are tasked with running sophisticated climate models to predict Earth’s future climate.

Illustration of an exoplanet. (NASA's Goddard Space Flight Center/Chris Smith)

Illustration of an exoplanet. (NASA’s Goddard Space Flight Center/Chris Smith)

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NASA says NESSI Emerges as New Tool for Exoplanet Atmospheres

 

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – The darkness surrounding the Hale Telescope breaks with a sliver of blue sky as the dome begins to open, screeching with metallic, sci-fi-like sounds atop San Diego County’s Palomar Mountain. The historic observatory smells of the oil pumped in to support the bearings that make this giant telescope float ever so slightly as it moves to track the stars.

Since February 2018, scientists have been testing an instrument at the Hale Telescope called the New Mexico Exoplanet Spectroscopic Survey Instrument, or NESSI.

The Hale Telescope is located on Palomar Mountain in San Diego County, California. (NASA/JPL-Caltech)

The Hale Telescope is located on Palomar Mountain in San Diego County, California. (NASA/JPL-Caltech)

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NASA’s TESS Satellite discovers Planet with Two Stars

 

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – In 2019, when Wolf Cukier finished his junior year at Scarsdale High School in New York, he joined NASA’s Goddard Space Flight Center in Greenbelt, Maryland, as a summer intern. His job was to examine variations in star brightness captured by NASA’s Transiting Exoplanet Survey Satellite (TESS) and uploaded to the Planet Hunters TESS citizen science project.

“I was looking through the data for everything the volunteers had flagged as an eclipsing binary, a system where two stars circle around each other and from our view eclipse each other every orbit,” Cukier said.

In this illustration, TOI 1338 b is silhouetted by its host stars. TESS only detects transits from the larger star. (NASA's Goddard Space Flight Center/Chris Smith)

In this illustration, TOI 1338 b is silhouetted by its host stars. TESS only detects transits from the larger star. (NASA’s Goddard Space Flight Center/Chris Smith)

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