SSolar System Exploration: A Vision for the Next 100 Years

can be from 1 year for reaching Mars orbit, to almost. 10 years for the Huygens probe into Titan's atmosphere, to even multiple decades for the Voyager ...







Journal of Space Exploration
The conclusion has shown that by selecting specific Asteroid orbits, it is possible to explore uncovered space regions, including interstellar and intergalactic ...
Interstellar Mapping and Acceleration Probe (IMAP): A New NASA ...
IMAP investigates two critical and interrelated frontiers of research in Heliophysics, the acceleration of energetic particles (EPs) in ...
DIRECT FUSION DRIVE - Princeton Plasma Physics Laboratory
DFD employs a unique plasma heating system to produce nuclear fusion engines in the range of 1 to 10 MW, ideal for human solar-system ...
Study on Libration Points of the Sun and the Interstellar Medium for ...
A study of possible libration points between the Sun and the nearby Centauri star system has been conducted. The two-centre problem was used to model the ...
The uncertain interstellar medium of high-redshift quiescent galaxies
The aim of the present paper is to further explore the richness of the APO Catalog for studying DIB correlations, with a par- ticular focus on unexplored ...
SCIENCE AND ENABLING TECHNOLOGIES FOR THE ...
This model has a dust temperature of Td = 21 K, which is a few Kelvin lower than the mass-weighted Td typi- cally used for SF galaxies (Scoville ...
Modelling Interstellar Complex Molecules
The interstellar probe would use a customized Star 20B to provide 1.56 km/s of burn at perihelion, enabling an escape from the solar system at ~ ...
ER INTERSTELLAR MISSION (VIM)
Ecole doctorale : SDM - SCIENCES DE LA MATIERE - Toulouse. Spécialité : Physico-Chimie Théorique. Unité de recherche :.
Cola Intergalactic / TD Snyder (PDF) globaldatabase.ecpat.org
The general mission objectives of the VIM are: (a) To investigate the interplanetary and interstellar media, and to characterize the interaction between the two ...
The ESO Diffuse Interstellar Bands Large Exploration Survey ...
This paper presents the observational overview of the ESO. Diffuse Interstellar Bands Large Exploration Survey (EDIBLES) and how we intend to use the obtained ...
Spectral studies of the interstellar dust and CMB mm emission
PICO has 21 bands (21 to 709 GHz). ? ESA Voyage 2050 has a L mission with precision spectrocopic capabilities in the mm range (early Universe, z>8).
The ESO Diffuse Interstellar Bands Large Exploration Survey ...
This paper presents the observational overview of the ESO. Diffuse Interstellar Bands Large Exploration Survey (EDIBLES) and how we intend to use the obtained ...