Pioneer and Voyager Jupiter encounter orbit reconstruction in the ICRF system
This paper discusses the effort to determine the gravity field of Jupiter and its Galilean satellites and to improve the ephemerides of those bodies.
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This paper discusses the effort to determine the gravity field of Jupiter and its Galilean satellites and to improve the ephemerides of those bodies.
STARDUST is a mission to flyby the comet Wild-2 in early 2004 and return samples of the coma to Earth.
The Galileo mission includes an Io flyby, insertion in Jupiter orbit, and ten close satellite flybys at altitudes as low as 250 km. The required orbit determination and navigation are described.
This introduction to the accompanying articles by the Ulysses investigators provides basic information on the experiments, the spacecraft and the trajectory. In addition, the scientific context of the encouter is reviewed based on the preliminary analyses of the Ulysses observations and a rudimentary comparison with the earlier Pioneer and Voyager results.
NASA's Near Earth Asteroid Rendezvous (NEAR) mission is planning a close flyby of the steroid 253 Mathilde in June 1997.
Each space mission follows the process cycle of design, development, intergration and test, launch and operation, science analysis and archive. The desire for more frequent and cost effective missions has motivated various new research and development efforts to reduce the design to launch period and the operarion/analysis costs.
INTRODUCTION: The purpose of this investigation was to evaluate if MultiColor Imaging (MCI) can replace color fundus photography (CFP) as a diagnostic screening tool during spaceflight. MCI significantly reduces crew time (approx. 115 minutes/session, 36 hours/year) by eliminating nominal on-orbit fundoscopy sessions, while also providing the option to capture a larger field of view (55 vs. 35). METHODS: A comprehensive PubMed literature search was conducted using the following key words: multicolor, multispectral, imaging, retina, choroid, optic nerve, optic disc, and papilledema. Publications were filtered based on optic nerve and chorioretinal pathologies matching those seen during or immediately after spaceflight: optic disc edema (ODE), cotton wool spots (CWS), retinal hemorrhage, pigment epithelial detachment (PED), and serous chorioretinopathy (SCR). In a separate effort, 44 multicolor images (30 abnormal) of terrestrial patients were graded and compared to corresponding color fundus images acquired at the Doheny Eye Centers and UCLA. RESULTS: The search identified 340 articles; 9 describing MCI in relevant pathologies, 6 comparing MCI to CFP. MCI is superior in detecting CWS (1 paper), PED (2 papers), retinal hemorrhages (2 papers), and choroidal folds (1 paper), and can better delineate extent or boundaries of subretinal fluid and identify areas of RPE damage in SCR (2 papers). On MCI, ODE was described as a hyperreflective ring with a green shift and indistinct disc margins, with equaldetectability as using CFP (3 papers). Grading at Doheny Eye Institute confirmed these findings. DISCUSSION: MCI can effectively detect all retinal and optic nerve findings detectable by CFP during and immediately post-spaceflight and represents a suitable replacement as an on-orbit diagnostic screening tool. Additionally, by eliminating the nominal on-orbit fundoscopy sessions, dozens of crew hours are spared per year by utilizing MCI.
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