Annexe 1

 "During Shima's presentation, Prof. William A. Cassidy of the University of Pittsburgh, decided to submit a proposal to the National Science Foundation, which funds all Antarctic research by U. S. scientists, to search for meteorite concentrations within helicopter range of McMurdo Station, across the continent from the Yamato Mts. On returning home he reported the Shimas' results to Dr. Takesi Nagata, Director of Japan's National Institute of Polar Research, who was visiting the University of Pittsburgh at that time. Nagata sent a field party back to the Yamato Mts. icefields in December, 1973, to conduct the first search specifically aimed at collecting meteorites in Antarctica. The members recovered 12 more specimens that season. It was by no means so straightforward a task to field an American team. A lapse of up to 18 months generally is expected between a scientist's submission of a new proposal to the NSF and his or her arrival in Antarctica. However, as a radical departure from traditional Antarctic programs, Cassidy's proposal received mixed reviews and was declined. Many of the geologists, glaciologists, and other scientists who dominated Antarctic research saw meteorites as of minimal scientific value, and referees with personal knowledge of the frigid Antarctic wastes viewed the idea of focused searches for them as naive. Cassidy submitted a revised proposal in 1975 which also was declined, but he resubmitted it and it was accepted on short notice after he called the NSF with the news that a Japanese team had just returned with 663 specimens. In 1976, Cassidy led the first U.S. meteorite search in Antarctica. That year Nagata also sent a scientist to search for meteorites out of McMurdo Station and so joint searches were agreed upon with equal sharing of all specimens found. This arrangement continued for three years. With the exception of 1990 when the season's work was cancelled due to lack of logistical support, Cassidy led the U. S. teams every year until 1992 when he passed along the leadership role to his Co-investigator, Dr. Ralph Harvey."
Marvin U. B.
(A Historical Outline of Meteorite Discoveries in Australia and Antarctica, 1994)

 

 


Annexe 2

Plans for the future:
Antarctica Nomad project
Robotics Demonstrations for Search for Meteorites
  • objective : demonstrate rob. tech and search in a planetary environment of autonomous navigation, perception, communication, env. survival
  • success criterion : enable convincing demonstration of autonomous technologies and robotic confirmation of meteorites
  • secondary : advance state-of the art in robotic search for meteorites
  • commitment to NASA : meteorobots in support of ANSMET teams
  • this year : meteorite confirmation and autonomous ice traverse
  • confirm 20 meteorites (planted), 200 rock samples to classify,
  • traverse 50km in polar terrain, pattern search in 300m², 500 hrs of ops.

(Current Research Activities of ANSMET: 1. Recent Studies in the Walcott Neve Region; 2. Planned Future Activities)
Cost for the 98 Antarctica Expedition $260,000
98/99 Meteorite demonstration $740,000
Autonomous Rover Technologies $600,000
Dimitrios Apostolopoulos (Carnegie Mellon University, 1998)