Talk:SISTINE
Appearance
This article is rated Start-class on Wikipedia's content assessment scale. It is of interest to the following WikiProjects: | |||||||||||||||||||||||||||||||
|
Created the talk-page
[edit]Created the talk-page for the "SISTINE" article - Enjoy! :) Drbogdan (talk) 14:55, 3 August 2019 (UTC)
Payload
[edit]I propose you create a Payload section that describes the generals of the spectrograph to be used, and how it will measure the desired data. Cheers, Rowan Forest (talk) 21:57, 3 August 2019 (UTC)
- @Rowan Forest: Done - A brief payload sentence was added as follows:
... This suborbital rocket can carry a payload of up to 1200 pounds, which, in the case of SISTINE, includes spectrographic equipment capable of covering the far ultra-violet spectral range of 100 to 160 nm, well suited to study strong atomic emission lines associated with the formation temperatures in the atmospheres of low-mass stars, and their effects on the potential atmospheres of exoplanets ...[1]
- should be ok - at least for starters? - iac - Enjoy! :) Drbogdan (talk) 23:04, 3 August 2019 (UTC)
References
- ^ Staff (2019). "36.333 UG France/University of Colorado - Suborbital Imaging Spectrograph for Transition region Irradiance from Nearby Exoplanet host stars (SISTINE)". NASA. Retrieved 3 August 2019.
Categories:
- Start-Class Astronomy articles
- Low-importance Astronomy articles
- Start-Class Astronomy articles of Low-importance
- Start-Class Rocketry articles
- Low-importance Rocketry articles
- WikiProject Rocketry articles
- Start-Class spaceflight articles
- Low-importance spaceflight articles
- WikiProject Spaceflight articles