![]() ![]() This data will help ensure that the telescope contributes to our increasing knowledge of planets outside of the Solar System and their potential to support life. ![]() Astrobiologists studying the potential for life on extrasolar planets provide valuable insight into mission requirements for the mission. Many astrobiolgists supported by elements of the Astrobiology Program are involved in the development of the Roman Space Telescope mission. The Roman Space Telescope will make observations that could contribute to the discovery of new worlds beyond our solar system and advance the search for extrasolar planets that could be suitable for life. The Roman Space Telescope is designed for a 6 year mission, and will launch on a EELV out of Cape Canaveral. The Coronagraph Instrument will perform high contrast imaging and spectroscopy of dozens of individual nearby exoplanets. It will perform a microlensing survey of the inner Milky Way to find ~2,600 exoplanets. As the primary instrument, the Wide Field Instrument will measure light from a billion galaxies over the course of the mission lifetime. The Roman Space Telescope will have a field of view that is 100 times greater than the Hubble infrared instrument, capturing more of the sky with less observing time. Roman has been called the “mother” of NASA’s Hubble Space Telescope. ![]() The telescope was initially developed as the Wide Field InfraRed Survey Telescope ( WFIRST), and renamed in 2020 to honor Nancy Grace Roman, NASA’s first Chief of Astronomy. The Roman Space Telescope is currently planned for launch in the mid-2020s. HST has demonstrated clearly that the combination of a powerful facility and peer-reviewed proposals has the greatest impact in advancing the extraordinarily broad field of astrophysics research.Īppendix A of the Roman Space Telescope SDT (2013) report contains ~ 50 potential GO or Guest Investigator science programs, each described in one page, contributed by members of the broader astronomical community.The Nancy Grace Roman Space Telescope – or Roman Space Telescope, for short – is a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics. In an extended mission, the General Observer program would likely become the dominant part of the mission. The General Observer program will provide broad support to many fields of astrophysics in the tradition of HST, no doubt with the same astonishing results of new, creative, field-changing science. Wide Field Instrument Romans Wide Field Instrument (WFI) is a 300-megapixel infrared camera that will allow scientists to explore the cosmos all the way from the edge of our solar system to the farthest reaches of space. While the baseline mission emphasizes the dark-energy and exoplanet measurements, the additional surveys carried out via the General Observer program will exploit it's unique capabilities to substantially broaden the science return of the mission. The Roman Space Telescope will offer a General Observer program that supports community-based observing programs.
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