Japan Geoscience Union Meeting 2014

Presentation information

Oral

Symbol P (Space and Planetary Sciences) » P-PS Planetary Sciences

[P-PS26_30AM1] Next decade initiatives for lunar planetary explorations

Wed. Apr 30, 2014 9:00 AM - 10:45 AM 418 (4F)

Convener:*Hirohide Demura(The University of Aizu), Noriyuki Namiki(Planetary Exploration Research Center Chiba Institute of Technology), Naoki Kobayashi(Department of Planetary Science, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Keiji Ohtsuki(Graduate School of Science, Kobe University), Sei-ichiro WATANABE(Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University), Yoshizumi Miyoshi(Solar-Terrestrial Environement Laboratory, Nagoya University), Chair:Naoki Kobayashi(Department of Solar System Sciences, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Hirohide Demura(The University of Aizu)

10:15 AM - 10:30 AM

[PPS26-06] Exploration of Jovian Trojan asteroids by Solar Power Sail

Ryosuke NAKAMURA1, *Yasuhito SEKINE2, Shuji MATSUURA3, Hajime YANO3, Osamu MORI3, SOLAR SAIL, Working group 3 (1.AIST, 2.Universit of Tokyo, 3.JAXA)

Keywords:Jupiter, Trojan, asteroids, exploration, Solar Sail

Solar Power Sail is a novel concept with hybrid propulsion of large-area solar sail and ion engine driven by thin-film solar panel. It enables us to bring relatively large mission payloads to the outer solar system without nuclear technology. The Solar Power Sail spacecraft is currently planned in Japan to explore Jovian Trojan astereoids. There exist two competing hypotheses on their origin. The classic model suggests that Trojan asteroids are mainly survivors of building blocks of the Jupiter system, while NICE model claims that they must be intruders from outer regions after the planetary migration of gas planets settled. This mission will provide invaluable clues to the genesis of the planets, asteroids ana comets through remote sensing, in-situ sample analysis and comparison of the results with other small body missions, such as Dawn, Rosetta, Osiris-ReX and Hayabusa-2. Another target of this mission is novel astronomy; measurement of the infrared extragalactic background light without foreground contamination of the zodiacal light thanks to low-density environment at deep space, polarization measurement of the gamma-ray burst and accurate determination of its direction based on the interplanetary network technique. The Solar Power Sail mission will thus develop a new direction of space astronomy and planetary science providing us an interplanetary telescope site and will play an important roll to form a new interdisciplinary science field.