ROSES-2019 Clarifications, corrections and amendments

Subscribe to the ROSES-2019 RSS feed for amendments, clarifications, and corrections here.

Potential proposers should also subscribe to the SMD NSPIRES mailing lists (by logging in at http://nspires.nasaprs.com/ and checking the appropriate boxes under Account Management and Email Subscriptions) and may also subscribe to a ROSES-2019 due date Google calendar. Instructions may be found at https://science.nasa.gov/researchers/sara/library-and-useful-links (link from the words due date calendar).

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The image is divided horizontally by an undulating line between a cloudscape forming a nebula along the bottom portion and a comparatively clear upper portion. Speckled across both portions is a starfield, showing innumerable stars of many sizes. The smallest of these are small, distant, and faint points of light. The largest of these appear larger, closer, brighter, and more fully resolved with 8-point diffraction spikes. The upper portion of the image is blueish, and has wispy translucent cloud-like streaks rising from the nebula below. The orangish cloudy formation in the bottom half varies in density and ranges from translucent to opaque. The stars vary in color, the majority of which have a blue or orange hue. The cloud-like structure of the nebula contains ridges, peaks, and valleys – an appearance very similar to a mountain range. Three long diffraction spikes from the top right edge of the image suggest the presence of a large star just out of view.

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