![]() ![]() The Orison Skyway Shuttle Service has two main lines, Main Line and Inspiration Park Line a loop line that serves Inspiration Park, Inspiration Park Shuttle Service a discretionary line that links with Vision Center, Vision Center Line and a tour line, Discovery Tours. Transit Transit map of Orison and its different platforms Soon after, Providence Platform was converted into one of the most advanced shipyards ever in operation and the city of Orison developed around the existing latticework. In 2865, CEO Kelly Caplan purchased the gas giant Crusader when the UEE decided to sell the planets in the Stanton system. Providence industrial platform played an important role in the repair of capital ships. The first orbital platforms were built by the UEE Navy in 2855 and considered an engineering marvel at the time. Crusader locals often describe the gentle vibrations that accompany the periodic adjustments as "Orison’s free massage." History ![]() Precisely timed to prevent shearing and destabilization of the connected network of struts, each thruster is activated for a short burst allowing Orison to stay firmly in place. ![]() Orison maintains its precise orbital height through controlled firing of Seraph-class thrusters situated below each platform. It offers a breathtaking view of Crusader's commercial shipbuilding platforms. The shipyards themselves are famously beautiful and have made Orison a prime tourist destination in the Stanton system. It is built upon a military-constructed latticework of inhabitable floating platforms which Crusader Industries uses to manufacture their large-scale ships. Spoto, Minor Planet Center), on the Horizons web service by JPL ( ) and on astrometry provided by ESA/Gaia.Orison is a network of large interconnected platforms floating in the atmosphere of the planet Crusader. Roger Venable and Robert Dunford are occultation observers affiliated to International Occultation Timing Association ( IOTA). The campaign in Japan was led by Hiroyuki Watanabe from the Japan Occultation Information Network (JOIN).ĪCROSS heavily relies on the orbFit software for orbit improvement (F. Steve Chesley is at JPL / Solar System Dynamic group Bouquillon (Observatoire de Paris) for the ground-based follow-up of the Gaia satellite Data collected by DART IT were used to extract astrometry of Didymos using the high accuracy pipeline developed by S. Souami are also members of the DART IT (Investigation Team). Siakas (student, Aristotle University of Thessaloniki. Ferreira (post-doc, Aristotle University of Thessaloniki), A. Souami (ACROSS post-doc, Université Côte d’Azur, OCA, CNRS/Lab. Tsiganis (partner coordinator, Aristotle University of Thessaloniki), D. Tanga (project coordinator, Université Côte d’Azur, OCA, CNRS/Lab. Gaia mapping of asteroids in the Solar System Kleomenis Tsiganis of Aristotle University of Thessaloniki, AUTh, adds: “To make such campaigns possible, we needed to perform independent orbit improvement calculations from the currently available data, shrink the uncertainty of the occultation path to a few kilometres, and deploy observers accordingly to catch a momentary blinking out of the star that has to be measured in milliseconds.” Repeating occultations over several years will even permit measurements of the deviation of the system's trajectory around the Sun induced by DART’s impact – something that cannot be done by DART or Hera alone.ĪCROSS co-investigator Prof. ESA will then fly the Hera spacecraft to the Didymos system to perform a close-up survey of the post-impact asteroid. On the night of 26 September the DART spacecraft slammed into the smaller of the two asteroids shifting its orbit. ACROSS has a special focus on Didymos – actually a binary asteroid system, with its 780-m diameter main asteroid orbited by a smaller 160-m diameter moonlet called Dimorphos – the target of NASA’s Double Asteroid Redirect Test, DART. ![]()
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