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Studies

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Large UV / Optical / Infrared Surveyor (LUVOIR)

The Large UV/Optical/IR Surveyor (LUVOIR) is a concept for a highly capable, multi-wavelength observatory with ambitious science goals. This mission would enable a great leap forward in a broad range of astrophysics, from the epoch of reionization, through galaxy formation and evolution, to star and planet formation. LUVOIR also has the major goal of characterizing a wide range of exoplanets, including those that might be habitable — or even inhabited.

LUVOIR is one of four Decadal Survey Mission Concept Studies initiated in January 2016. The study will extend over three years and be will executed by the Goddard Space Flight Center, under the leadership of a Science and Technology Definition Team (STDT) drawn from the community.

Concept for deployment of the 15-m LUVOIR-A observatory.
NASA

The Origins Space Telescope (OST)

The Origins Space Telescope (OST) is one of the four Decadal Survey Mission Concept Studies initiated in January 2016. The study is being executed at Goddard Space Flight Center, under the leadership of a community-based Science and Technology Definition Team.

The OST team is developing two concepts for a Far-Infrared Surveyor mission, as described in the Astrophysics Roadmap. It will address a wide variety of topics that can be studied at Far-IR wavelengths, ranging from Exoplanets to planetary system formation to star-formation on scales both large and small to the rise of metals in the Universe over cosmic time.

Artist 3d concept of the origins space telescope with gray shiny material around a metal tube with a mirror inside the tube
The Origins concept-2 baseline design, consists of a 5.9m diameter (25 sq. meter collecting area), on-axis telescope with a primary composed of 18 lightweight pie-shaped segments arranged in two concentric rings. The telescope is diffraction-limited at 30 microns. All of the telescope optics are shielded and both radiatively and actively cooled to a temperature of ~4.5K. The telescope optical coatings allow for the operation of science instruments spanning the range from 5-600 microns.
NASA/JPL

The Habitable Exoplanet Imaging Mission (HabEx)

The Habitable Exoplanet Imaging Mission (HabEx) is a concept for a mission to directly image planetary systems around Sun-like stars. HabEx will be sensitive to all types of planets; however, its main goal is, for the first time, to directly image Earth-like exoplanets and characterize their atmospheric content. By measuring the spectra of these planets, HabEx will search for signatures of habitability such as water, and be sensitive to gases in the atmosphere possibility indicative of biological activity, such as oxygen or ozone. In addition to the search for life on Earth-like exoplanets, HabEx will enable a broad range of general astrophysics, from studying the earliest epochs of the history of the Universe, to understanding the life cycle and deaths of the most massive stars, which ultimately supply the elements that are needed to support life as we know it.

The Habitable Exoplanet Observatory (HabEx) is a concept for a mission to directly image planetary systems around Sun-like stars. HabEx will be sensitive to all types of planets; however its main goal is, for the first time, to directly image Earth-like exoplanets, and characterize their atmospheric content. By measuring the spectra of these planets, HabEx will search for signatures of habitability such as water, and be sensitive to gases in the atmosphere possibility indicative of biological activity, such as oxygen or ozone.
NASA/JPL

Lynx X-ray Observatory

The Lynx mission concept seeks to provide unprecedented X-ray vision into the universe. Lynx will directly observe the dawn of supermassive black holes, reveal the drivers of galaxy formation, trace stellar activity (including effects on planet habitability), and transform our knowledge of endpoints of stellar evolution. Expanding on the legacy of the Chandra X-ray Observatory, Lynx’s design will include excellent angular resolution, high throughout, a large field-of-view, and high spectral resolution for both point-like and extended sources.

Lynx is a true next-generation X-ray observatory whose design will include excellent angular resolution, high throughput, large field of view, and high spectral resolution for both point-like and extended sources.
NASA

Hubble Completion

The Hubble Space Telescope is in a decaying orbit. To prevent the hazards created by such an event, the Cosmic Origins Program Office has undertaken a study of ways to complete the mission of the great observatory, either by controlled re-entry or placement into a long life orbit.

Hubble's Deployment (1990)
The Hubble Space Telescope is photographed at the moment of release from space shuttle Discovery on April 25, 1990 as part of STS-31, the Space Shuttle's mission to deploy the observatory.
NASA

Other Studies

Astrophysics Roadmap 2013

Telescope image of stars, gas, and dust

Astro2020

Telescope image of a spiral galaxy

2016 Probe-Class Mission Study

Image of a cloud of gas and dust with background stars; half shows visible light, half shows infrared light

2015 COPAG Large Mission Study

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.