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Wide-field Infrared Survey Explorer (WISE, observatory code C51) is a NASA infrared-wavelength astronomical space telescope launched in December 2009, and placed in hibernation mode in February 2011. Earlier this month, NASA cleared the Wide Field Infrared Survey Telescope (WFIRST) to move forward, with the development of engineering test units and models. Get the most up-to-date news by following.

Scientists aren't yet sure, but they think it has something to do with dark energy. WFIRST is the top-ranked large space mission in the 2010 New Worlds, New Horizon Decadal Survey … Beyond helping us answer some of humanity's most enduring questions, WFIRST will also help scientists spot planets orbiting other stars in our galactic neighborhood. WFIRST will be powered by two fixed and four deployable solar panels with a total of 360 sq ft of surface area, generating 4,100 watts. Although we know that dark energy makes up about 68% of our universe, we don't know what it is — only what it does to the universe. Receive mail from us on behalf of our trusted partners or sponsors? The Wide Field Infrared Survey Telescope (WFIRST) is a 2.4m space telescope with a 0.281 deg^2 field of view for near-IR imaging and slitless spectroscopy and a coronagraph designed for > 10^8 starlight suppresion. Fast Infrared Exoplanet Spectroscopy Survey Explorer Launch Date: April 28, 2003 The Galaxy Evolution Explorer was an orbiting space telescope designed to observe the universe in ultraviolet wavelengths to measure the history of star formation in the universe. These exoplanets are numerous. One technique WFIRST will use is called microlensing. But what is causing that acceleration of the expansion of the universe? The coronagraph will enable astronomers to detect and measure properties of planets orbiting other stars. There was a problem. WFIRST is the top-ranked large space mission in the 2010 New Worlds, New Horizon Decadal Survey of Astronomy and Astrophysics. With a slew of calculations, scientists can then figure out such a planet's mass, orbit and orbital period around the lensing star. The Wide Field Infrared Survey Telescope (WFIRST) is a 2.4m space telescope with a 0.281 deg^2 field of view for near-IR imaging and slitless spectroscopy and a coronagraph designed for > 10^8 starlight suppresion. That bent light magnifies the lensing star, making it appear much bigger to us on Earth. The Wide Field Infrared Survey Telescope (WFIRST) is NASA's next flagship telescope. The Wide Field Infrared Survey Telescope (WFIRST) is a 2.4m telescope equipped with a large area, 300-megapixel, near-infrared camera for imaging and slitless spectroscopy and an on-axis, visible-light coronagraph for imaging, polarimetry, and low-resolution spectroscopy of circumstellar disks and nearby giant exoplanets. WFIRST will communicate with Earth via a High Gain Antenna 5.5 ft tall and capable of transmitting 1.375 terabytes of data per day. WFIRST will expand that search to look for planets as far away as we can imagine — thousands of light-years away, near the center of the Milky Way galaxy. Please refresh the page and try again. Expected to launch in the mid-2020s, this instrument will give astronomers a clearer and more expansive view of the universe than ever before, with the ultimate goal of answering some of the biggest mysteries in space.

WFIRST is planned for a mid-decade launch, following into space the James Webb Space Telescope (JWST), currently set to launch in 2021. Through its world-class training curriculum, knowledge-sharing initiatives, development resources, and strategic communications, APPEL Knowledge Services helps ensure NASA’s technical workforce has the skills and knowledge needed to advance mission success. Gaudi is a principal investigator on the WFIRST Formulation Science Working Group.

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