1 min read

Changes to C.22 OREx PSP Start date and the Participating Scientist Orientation Meeting

Program element C.22, the OSIRIS REx Participating Scientists Program has been modified. The estimated start date (in sections 2.4 and 4) and dates of the Participating Scientist Orientation Meeting (in section 2.7) have been delayed by a month. New text is in bold and deleted text is struck through. The Step-2 due date remains unchanged at 07/11/2017.

Share

Details

Last Updated
May 22, 2023
Editor
NASA Science Editorial Team

Related Terms

Explore More

2 min read

Approval to Exceed GSA Lodging for LPSC 2022

Article2 years ago
2 min read

Approval to Exceed GSA Lodging for AGU 2021

Article2 years ago
2 min read

Amendment 40: Revised Text and Budget for D.9 NuSTAR General Observer Program Cycle 8

Article3 years ago
Keep Exploring

Discover More Topics From NASA

James Webb Space Telescope

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.

Perseverance Rover

Parker Solar Probe

Juno