Hubbry Logo
search button
Sign in
Colorado Ultraviolet Transit Experiment
Colorado Ultraviolet Transit Experiment
Comunity Hub
History
arrow-down
starMore
arrow-down
bob

Bob

Have a question related to this hub?

bob

Alice

Got something to say related to this hub?
Share it here.

#general is a chat channel to discuss anything related to the hub.
Hubbry Logo
search button
Sign in
Colorado Ultraviolet Transit Experiment
Community hub for the Wikipedia article
logoWikipedian hub
Welcome to the community hub built on top of the Colorado Ultraviolet Transit Experiment Wikipedia article. Here, you can discuss, collect, and organize anything related to Colorado Ultraviolet Transit Experiment. The ...
Add your contribution
Colorado Ultraviolet Transit Experiment

Colorado Ultraviolet Transit Experiment (CUTE) is a small UV space telescope to study selected exoplanets.[1]

It was launched as a rideshare on the Atlas V that launched Landsat 9 on September 27, 2021.[1] Designed to operate for at least 8 months and study 10 exoplanets, CUTE remains operational as of December 2023, 27 months after launch. The spacecraft is expected to remain in orbit until 2027.[2]

CUTE can measure near-UV (255-330 nm) and do low resolution spectroscopy of atmospheric tracers (eg. Fe II, Mg II, Mg I, OH).[3]

The UV sensor is a 2048 x 515 pixel CCD array, with the spectrum lengthwise across the sensor.[4] The 515 pixel width provides tolerance from sensor damage.

See also

[edit]

References

[edit]
  1. ^ a b Johnston, Scott Alan (25 September 2021). "A Tiny, Inexpensive Satellite Will be Studying the Atmospheres of hot Jupiters". Universe Today. Retrieved 13 December 2021.
  2. ^ Werner, Debra (12 December 2023). "Cubesat offers template for future astronomy missions". SpaceNews. Retrieved 13 December 2023.
  3. ^ "Colorado Ultraviolet Transit Experiment (CUTE)". LASP. University of Colorado Boulder. Retrieved 13 December 2023.
  4. ^ Fleming, Brian T.; et al. (2017). The Colorado Ultraviolet Transit Experiment (CUTE): a dedicated cubesat mission for the study of exoplanetary mass loss and magnetic fields. UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XX. Vol. 10397. Proceedings of SPIE. arXiv:1801.02673v1. doi:10.1117/12.2276138. ISBN 978-1-5106-1251-8.
[edit]