\n\t\t\t\t\t\t\t\tThe CUTE Mission: Innovative Design Enables Observations of Extreme Exoplanets from a Small Package\t\t\t\t\t\t\t<\/h1>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n![\"A](\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2024\/02\/cute-orbit031218.jpg?w=1536\")
<\/figure>\n<\/div>\n<\/div>\n<\/div>\n\n\n\nFig 1: Artist\u2019s concept of the CUTE mission on-orbit. CUTE has been operating in a 560 km sun-synchronous orbit since September 2021.<\/figcaption><\/div>\n<\/div>\n\n\t\t\t\t\t\tCredits: <\/span>
\n\t\t\t\t\t\tNASA<\/span>\n\t\t\t\t\t<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nOf the approximately 5,500 exoplanets discovered to date, many have been found to orbit very close to their parent stars. These close-in planets provide a unique opportunity to observe in detail the phenomena critical to the development and evolution of our own solar system, including atmospheric mass loss and interactions with the host star. NASA\u2019s Colorado Ultraviolet Transit Experiment (CUTE) mission, launched in September 2021, employed a new design that enabled exploration of these processes using a small spacecraft for the first time. CUTE provides unique spectral diagnostics that trace the escaping atmospheres of close-in, ultra-hot, giant planets. In addition, CUTE\u2019s dedicated mission architecture enables the survey duration required to characterize atmospheric structure and variability on these worlds.<\/p>\n
Atmospheric escape is a fundamental process that affects the structure, composition, and evolution of many planets. It has operated on all of the terrestrial planets in our solar system and likely drives the demographics of the short-period planet population characterized by NASA\u2019s Kepler mission<\/a>. In fact, atmospheric escape ultimately may be the determining factor when predicting the habitability of temperate, terrestrial exoplanets. Escaping exoplanet atmospheres were first observed<\/a> in the hydrogen Lyman-alpha line (121nm) in 2003. However, contamination by neutral hydrogen in both the intervening interstellar medium and Earth\u2019s upper atmosphere makes obtaining high-quality Lyman-alpha transit measurements for most exoplanets very challenging. By contrast, a host star\u2019s near-ultraviolet (NUV; 250 \u2013 350 nm) flux is two to three orders of magnitude higher than Lyman-alpha, and transit light curves can be measured against a smoother stellar surface intensity distribution.<\/p>\nThis knowledge motivated a team led by Dr. Kevin France at the University of Colorado Laboratory for Atmospheric and Space Physics to design the CUTE mission (Fig 2). The team proposed the CUTE concept to NASA through the ROSES\/Astrophysics Research and Analysis (APRA) Program in February 2016 and NASA funded the project in July 2017. The CUTE instrument pioneered use of two technologies on a small space mission: a novel, rectangular Cassegrain telescope (20cm \u00d7 8cm primary mirror) and a miniature, low-resolution spectrograph operating from approximately 250 \u2013 330 nm. The rectangular telescope was fabricated to accommodate the unique instrument volume of the 6U CubeSat form factor, an adaptation that delivers approximately three times the collecting area of a traditional, circular aperture telescope.\u00a0 The compact spectrograph meets the spectral resolution requirements of the mission while using scaled down component technology adapted from the Hubble Space Telescope.<\/p>\n
\n\n\n![\"Flat](\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2024\/02\/cuteinstall2.jpg?w=512\")
<\/figure>\nFig 2 \u2013 Image of the CUTE science instrument, including rectangular telescope and miniaturized spectrograph, mounted to the spacecraft bus. <\/div>\nCredit: CUTE Team, University of Colorado<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nThis novel instrument design enables CUTE to measure NUV with similar precision as larger missions even in the more challenging thermal and pointing environment experienced by a CubeSat. In addition, the CUTE instrument\u2019s NUV bandpass enables it to measure iron and magnesium ions from highly extended atmospheric layers that ground-based instruments cannot access. The CUTE science instrument is incorporated into a 6U Blue Canyon Technologies spacecraft bus that provides power, command and data handling, attitude control, and communications. This CubeSat platform enables CUTE to observe numerous transits of a given planet. The spectrogram from the CUTE instrument is recorded on a UV-optimized commercial off-the-shelf charge-coupled device (CCD), onboard data processing is performed, and data products are relayed to a ground station at the University of Colorado.<\/p>\n
\n\n\n![\"Several](\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2024\/02\/cuteinstall1.jpg?w=2048\")
<\/figure>\nFig 3 \u2013Graduate student Arika Egan (center) and electrical engineer Nicholas DeCicco (left) install CUTE into the LANDSAT-9 secondary payload dispenser at Vandenberg Space Force Base. <\/div>\nCredit: CUTE Team, University of Colorado<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nCUTE was launched as a secondary payload on NASA\u2019s LANDSAT-9 mission on September 27, 2021 into a Sun-synchronous orbit with a 560 km apogee. CUTE deployed from the payload dispenser (Fig 3) approximately two hours after launch and then deployed its solar arrays. Spacecraft beacon signals were identified by the amateur radio community on the first orbit and communications were established with the ground station at the University of Colorado the following day. On-orbit commissioning of the spacecraft and instrument concluded in February 2022 and the mission has been conducting science operations since that time.<\/p>\n
As of February 2024, CUTE is actively acquiring science and calibration data (Fig 4), and has observed between 6 and 11 transits of seven different exoplanetary systems. Data downlink efficiency is the primary factor limiting the number of targets observed over the course of the mission. CUTE light curves and transit spectroscopy are revealing extended NUV atmospheres on some planets (Fig 5) and potential time variability in the atmospheric transmission spectra of others. For example, observations of the ultra-hot exoplanet, Jupiter WASP-189b, indicate a highly extended atmosphere. Magnesium ions are observed to be gravitationally unbound from the planet, which is evidence for active escape of heavy elements in this system. CUTE data are being archived by the NASA Exoplanet Science Institute (NExScI)<\/a>.<\/p>\n\n\n\n![\"At](\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2024\/02\/zetapup-1d2d-display.png?w=800\")
<\/figure>\nFig 4 \u2013 Flight data from CUTE showing raw CCD observations (top) and calibrated one-dimensional spectra (bottom).<\/div>\nImage credit: France et al (2023)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n\n\n\n![\"Graph](\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2024\/02\/transit-wasp189b-.png?w=721\")
<\/figure>\nFig 5 \u2013 CUTE NUV transit light curve of the ultra-hot exoplanet, Jupiter WASP-189b. This light curve was created from three separate transit visits to the planet. <\/div>\nImage credit: Sreejith, et al (2023)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nCUTE successfully demonstrated the use of a non-circular telescope and miniature spectrograph design for small space missions, an approach that has been subsequently adopted by several NASA and international mission designs, including NASA\u2019s new Monitoring Activity from Nearby sTars with uv Imaging and Spectroscopy (MANTIS) mission<\/a>. CUTE\u2019s demonstration of sub-1% NUV precision has shown that the precision achieved by large UV astronomy missions can also be achieved by a CubeSat. In addition, student training and early-career mentorship have been key ingredients to CUTE\u2019s mission success. So far, over 20 early career students and professionals have trained and participated in CUTE activities\u2014ranging from science to engineering to operations.<\/p>\nPROJECT LEAD<\/h3>\n
Professor Kevin France, Laboratory for Atmospheric and Space Physics\/University of Colorado<\/p>\n
SPONSORING ORGANIZATION<\/h3>\n
Astrophysics Division Astrophysics Research and Analysis Program<\/p>\n
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<\/figure>\n<\/div>\n<\/div>\n<\/div>\n\n\t\t\t\t\t\tNASA<\/span>\n\t\t\t\t\t<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n
Of the approximately 5,500 exoplanets discovered to date, many have been found to orbit very close to their parent stars. These close-in planets provide a unique opportunity to observe in detail the phenomena critical to the development and evolution of our own solar system, including atmospheric mass loss and interactions with the host star. NASA\u2019s Colorado Ultraviolet Transit Experiment (CUTE) mission, launched in September 2021, employed a new design that enabled exploration of these processes using a small spacecraft for the first time. CUTE provides unique spectral diagnostics that trace the escaping atmospheres of close-in, ultra-hot, giant planets. In addition, CUTE\u2019s dedicated mission architecture enables the survey duration required to characterize atmospheric structure and variability on these worlds.<\/p>\n
Atmospheric escape is a fundamental process that affects the structure, composition, and evolution of many planets. It has operated on all of the terrestrial planets in our solar system and likely drives the demographics of the short-period planet population characterized by NASA\u2019s Kepler mission<\/a>. In fact, atmospheric escape ultimately may be the determining factor when predicting the habitability of temperate, terrestrial exoplanets. Escaping exoplanet atmospheres were first observed<\/a> in the hydrogen Lyman-alpha line (121nm) in 2003. However, contamination by neutral hydrogen in both the intervening interstellar medium and Earth\u2019s upper atmosphere makes obtaining high-quality Lyman-alpha transit measurements for most exoplanets very challenging. By contrast, a host star\u2019s near-ultraviolet (NUV; 250 \u2013 350 nm) flux is two to three orders of magnitude higher than Lyman-alpha, and transit light curves can be measured against a smoother stellar surface intensity distribution.<\/p>\n This knowledge motivated a team led by Dr. Kevin France at the University of Colorado Laboratory for Atmospheric and Space Physics to design the CUTE mission (Fig 2). The team proposed the CUTE concept to NASA through the ROSES\/Astrophysics Research and Analysis (APRA) Program in February 2016 and NASA funded the project in July 2017. The CUTE instrument pioneered use of two technologies on a small space mission: a novel, rectangular Cassegrain telescope (20cm \u00d7 8cm primary mirror) and a miniature, low-resolution spectrograph operating from approximately 250 \u2013 330 nm. The rectangular telescope was fabricated to accommodate the unique instrument volume of the 6U CubeSat form factor, an adaptation that delivers approximately three times the collecting area of a traditional, circular aperture telescope.\u00a0 The compact spectrograph meets the spectral resolution requirements of the mission while using scaled down component technology adapted from the Hubble Space Telescope.<\/p>\n This novel instrument design enables CUTE to measure NUV with similar precision as larger missions even in the more challenging thermal and pointing environment experienced by a CubeSat. In addition, the CUTE instrument\u2019s NUV bandpass enables it to measure iron and magnesium ions from highly extended atmospheric layers that ground-based instruments cannot access. The CUTE science instrument is incorporated into a 6U Blue Canyon Technologies spacecraft bus that provides power, command and data handling, attitude control, and communications. This CubeSat platform enables CUTE to observe numerous transits of a given planet. The spectrogram from the CUTE instrument is recorded on a UV-optimized commercial off-the-shelf charge-coupled device (CCD), onboard data processing is performed, and data products are relayed to a ground station at the University of Colorado.<\/p>\n CUTE was launched as a secondary payload on NASA\u2019s LANDSAT-9 mission on September 27, 2021 into a Sun-synchronous orbit with a 560 km apogee. CUTE deployed from the payload dispenser (Fig 3) approximately two hours after launch and then deployed its solar arrays. Spacecraft beacon signals were identified by the amateur radio community on the first orbit and communications were established with the ground station at the University of Colorado the following day. On-orbit commissioning of the spacecraft and instrument concluded in February 2022 and the mission has been conducting science operations since that time.<\/p>\n As of February 2024, CUTE is actively acquiring science and calibration data (Fig 4), and has observed between 6 and 11 transits of seven different exoplanetary systems. Data downlink efficiency is the primary factor limiting the number of targets observed over the course of the mission. CUTE light curves and transit spectroscopy are revealing extended NUV atmospheres on some planets (Fig 5) and potential time variability in the atmospheric transmission spectra of others. For example, observations of the ultra-hot exoplanet, Jupiter WASP-189b, indicate a highly extended atmosphere. Magnesium ions are observed to be gravitationally unbound from the planet, which is evidence for active escape of heavy elements in this system. CUTE data are being archived by the NASA Exoplanet Science Institute (NExScI)<\/a>.<\/p>\n CUTE successfully demonstrated the use of a non-circular telescope and miniature spectrograph design for small space missions, an approach that has been subsequently adopted by several NASA and international mission designs, including NASA\u2019s new Monitoring Activity from Nearby sTars with uv Imaging and Spectroscopy (MANTIS) mission<\/a>. CUTE\u2019s demonstration of sub-1% NUV precision has shown that the precision achieved by large UV astronomy missions can also be achieved by a CubeSat. In addition, student training and early-career mentorship have been key ingredients to CUTE\u2019s mission success. So far, over 20 early career students and professionals have trained and participated in CUTE activities\u2014ranging from science to engineering to operations.<\/p>\n Professor Kevin France, Laboratory for Atmospheric and Space Physics\/University of Colorado<\/p>\n Astrophysics Division Astrophysics Research and Analysis Program<\/p>\n<\/figure><\/figure><\/figure><\/figure>PROJECT LEAD<\/h3>\n
SPONSORING ORGANIZATION<\/h3>\n
Share<\/h2>\n<\/div>\n