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Data of the stratospheric balloon launched on 5/27/2007For HERO (High Energy Replicated Optics)
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Details of the balloon and launch operationsLaunch site:Fort Sumner Municipal Airport, New Mexico, US Launch team: Columbia Scientific Balloon Facility (CSBF) Balloon: Open balloon (zero pressure) Volume: Raven - 39.570.000 cu ft - 0.8 Mil. Serial number: - Flight identification number: 569N Campaign: - Payload weight: 3220 lbs Gondola weight: - Overall weight: 5500 lbs |
ImagesClick to enlarge. ![]() ![]() ![]() ![]() © Dr. Brian Ramsey & Adam Eakins |
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Description of the payload or experiment
HERO (High Energy Replicated Optics) Responsable institution: NASA Marshall Space Flight Center Principal Investigator: Dr. Brian Ramsey The instrument, is the first one aimed to obtain focused images of astronomical X-ray sources at hard X-ray energies (20–75 keV). The key component (the hard X-ray optics) are full-shell electroformed-nickel-replicated (ENR) mirrors coated with iridium to enhance high-energy reflectivity. As the critical grazing angle for reflection varies approximately inversely with energy, these mirrors employ smaller angles than their low-energy counterparts and consequently have smaller diameters and collecting areas per shell. The mirrors have a 6 meter focal length. To exploit the full potential of the HERO optics necessitates a balloon gondola that can provide commensurate pointing accuracy, stability, and pointing knowledge. The HERO gondola utilizes a coarse aspect system for slewing based on a differential global positioning system (GPS) and a fine inertial-mode pointing system that uses a novel day/night aspect camera system to update onboard gyroscopes. The total payload dimensions are 25 feet long, 6.5 ft wide and 16 ft high. | ||||||||||||||||
Performance in flight and data obtainedThe instrument performed very well. The scientific team managed to made during the flight 4 observations of galactic x-ray sources and one observation of an extragalactic source. |
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External references and bibliographical sources
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| If you detected mistakes in the information presented here, please tell me (Updated on 5-Oct-2007 - 05:37:55pm) | ||||||||||||||||
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