PPT-Photometric analysis of Martian moon Phobos with the HRSC o

A Pasewaldt 1 K Willner 2 J Oberst 12 Frank Scholten 1 M Wählisch 1 KD Matz 1 T Roatsch 1 H Hoffmann 1 A Grechishev 3 . Martian Terraforming 2For the past several decades, scientists have worked to develop a plan for terraforming (i.e. making more like Earth) other planetary bodies within our solar system. Mar Phobos. – The Age of . Phobos. and its Largest Crater Stickney. 1. N. Schmedemann. 1. , . G. Michael. 1. ,. B. A. Ivanov. 2. , . J. Murray. 3. and G. Neukum. 1. ,. . 1. Institute of Geological Sciences, . Outline. 1.) Step 1 – TV3 Calibration. 2.) Step 2 – SMOV4 (+ Cycle 17 Calibration). 3.) Step 3 – Final Calibration (present analysis). - More data. - New flat fields. - Astrodrizzle. - Precise calibration. Compiled by David Beaty, Lars Borg, David Draper, Walter Kiefer, Jim Papike, Kevin Righter, Chip Shearer, Sue Smrekar, Jeff Taylor . Correspondence author: Dave Beaty . (JPL/Caltech), . David.W.Beaty@jpl.nasa.gov. Solanum lycopersicum. Seed Germination in Microgravity. . Sabrina Benitez (Co-Principal Investigator). Juan Pablo Flanagan (Co-Principal Investigator). Sofia Escobar (Co-Principal Investigator). Laura Nikstad (Teacher Facilitator) . 8.30.11 DO NOW. There are over fifty members in my family;. Yet none quarrel. We all live merrily.. Four leaders have we, all with a bride;. Each has a son who has great pride.. We also have servants who make funny gestures;. CS5670 : Computer Vision. Noah Snavely. A Single Image: Shape from Shading. Assume is 1 for now.. What can we measure from one image?. is the angle between N and L. Add assumptions:. Phobos. C. omparison of two Endmember Chronologies. The Age and Cratering History of . Phobos. , Sept 21 2015. Outline. Background:. dating of planetary surfaces from measurements of crater size-frequency distributions. Apostolos Christou. Armagh Observatory and Planetarium. Northern Ireland, UK. DPS . 49 ● . Provo, Utah. ● . Oct 18, 2017. Email: . aac@arm.ac.uk. ● . Population control of Martian Trojans. Precurso. r Strategy An. alysis Group (P-SAG) . (jointly sponsored by MEPAG and SBAG). Executive Summary for MEPAG. Oct. 4, 2012. JPL CL#12-. 2401. HISTORY. Last MEPAG meeting: Feb. 27-28. Chartered March 1 by SMD and HEOMD to produce rapid inputs to MPPG.. Announcements. Project 4 (stereo) released today, due Friday, April 1, at 8pm. To be done in groups of 2. Recap: . Lambertian (Diffuse) Reflectance. I . : observed image intensity. k. d. . : object albedo. Mars is the forth planet from the . sun. Mars has two moons in orbit. The names of the moons are called Phobos and Deimos. Mars is currently 218.27 million KMs from the sun. Mars’ diameter is 6,779kms. two moons . of . Mars . with sample return . from . Phobos. Hirdy Miyamoto (. Univ. Tokyo) on behalf of MMX team. NOTE ADDED BY JPL WEBMASTER: This content has not been approved or adopted by, NASA, JPL, or the California Institute of Technology. This document is being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.. „4.5. Light . sources. “. With the agreed objective to allow all light source technologies in all lamps (functions) the text of section 4.5.1. condenses significantly. 4.5. Light sources. 4.5.1. Restrictions on light sources .