Academic literature on the topic 'Co-orbiting'

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Journal articles on the topic "Co-orbiting"

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Simpson, Jeffrey D., Sarah L. Martell, Gary Da Costa, et al. "The GALAH survey: co-orbiting stars and chemical tagging." Monthly Notices of the Royal Astronomical Society 482, no. 4 (2018): 5302–15. http://dx.doi.org/10.1093/mnras/sty3042.

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Watanabe, Yasuto, and Kazumi Ozaki. "Relative Abundances of CO2, CO, and CH4 in Atmospheres of Earth-like Lifeless Planets." Astrophysical Journal 961, no. 1 (2024): 1. http://dx.doi.org/10.3847/1538-4357/ad10a2.

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Abstract Carbon is an essential element for life on Earth, and the relative abundances of major carbon species (CO2, CO, and CH4) in the atmosphere exert fundamental controls on planetary climate and biogeochemistry. Here we employed a theoretical model of atmospheric chemistry to investigate diversity in the atmospheric abundances of CO2, CO, and CH4 on Earth-like lifeless planets orbiting Sun-like (F-, G-, and K-type) stars. We focused on the conditions for the formation of a CO-rich atmosphere, which would be favorable for the origin of life. Results demonstrated that elevated atmospheric C
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Yoder, C. F., S. P. Synnott, and H. Salo. "Orbits and masses of Saturn's co-orbiting satellites, Janus and Epimetheus." Astronomical Journal 98 (November 1989): 1875. http://dx.doi.org/10.1086/115265.

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Vokrouhlický, David, and David Nesvorný. "TRANSIT TIMING VARIATIONS FOR PLANETS CO-ORBITING IN THE HORSESHOE REGIME." Astrophysical Journal 791, no. 1 (2014): 6. http://dx.doi.org/10.1088/0004-637x/791/1/6.

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Ranjan, Sukrit, Edward W. Schwieterman, Michaela Leung, Chester E. Harman, and Renyu Hu. "The Importance of the Upper Atmosphere to CO/O2 Runaway on Habitable Planets Orbiting Low-mass Stars." Astrophysical Journal Letters 958, no. 1 (2023): L15. http://dx.doi.org/10.3847/2041-8213/ad037c.

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Abstract Efforts to spectrally characterize the atmospheric compositions of temperate terrestrial exoplanets orbiting M dwarf stars with JWST are now underway. Key molecular targets of such searches include O2 and CO, which are potential indicators of life. Recently, it was proposed that CO2 photolysis generates abundant (≳0.1 bar) abiotic O2 and CO in the atmospheres of habitable M dwarf planets with CO2-rich atmospheres, constituting a strong false positive for O2 as a biosignature and further complicating efforts to use CO as a diagnostic of surface biology. Importantly, this implied that T
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MacDonald, Cameron G., Jon-Paul Mastrogiacomo, Joshua L. Laughner, Jacob K. Hedelius, Ray Nassar, and Debra Wunch. "Estimating enhancement ratios of nitrogen dioxide, carbon monoxide and carbon dioxide using satellite observations." Atmospheric Chemistry and Physics 23, no. 6 (2023): 3493–516. http://dx.doi.org/10.5194/acp-23-3493-2023.

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Abstract. Using co-located space-based measurements of carbon dioxide (CO2) from the Orbiting Carbon Observatory-2 and Orbiting Carbon Observatory-3 (OCO-2/3) and carbon monoxide (CO) and nitrogen dioxide (NO2) from the TROPOspheric Monitoring Instrument (TROPOMI), we calculate total column enhancements for observations influenced by anthropogenic emissions from urban regions relative to clean background values. We apply this method to observations taken over or downwind of 27 large (population of >1 million) urban areas from around the world. Enhancement ratios between species are calculat
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Guthrie, Ben, Minkwan Kim, Hodei Urrutxua, and Jonathon Hare. "Image-based attitude determination of co-orbiting satellites using deep learning technologies." Aerospace Science and Technology 120 (January 2022): 107232. http://dx.doi.org/10.1016/j.ast.2021.107232.

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Christou, Apostolos A., and Paul Wiegert. "A population of Main Belt Asteroids co-orbiting with Ceres and Vesta." Icarus 217, no. 1 (2012): 27–42. http://dx.doi.org/10.1016/j.icarus.2011.10.016.

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Pokorný, Petr, Ariel N. Deutsch, and Marc J. Kuchner. "Mercury's Circumsolar Dust Ring as an Imprint of a Recent Impact." Planetary Science Journal 4, no. 2 (2023): 33. http://dx.doi.org/10.3847/psj/acb52e.

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Abstract A circumsolar dust ring has been recently discovered close to the orbit of Mercury. There are currently no hypotheses for the origin of this ring in the literature, so we explore four different origin scenarios here: the dust originated from (1) the sporadic meteoroid complex that comprises the major portion of the Zodiacal Cloud, (2) recent asteroidal/cometary activity, (3) hypothetical dust-generating bodies locked in mean-motion resonances beyond Mercury, and (4) bodies co-orbiting with Mercury. We find that only scenario (4) reproduces the observed structure and location of Mercur
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Su, Haoxiang, Zhenghong Dong, Lihao Liu, and Lurui Xia. "Numerical Solution for the Single-Impulse Flyby Co-Orbital Spacecraft Problem." Aerospace 9, no. 7 (2022): 374. http://dx.doi.org/10.3390/aerospace9070374.

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The traversal inspection of satellites in satellite constellations or geosynchronous orbits has been a focus of research. A large number of variable orbit requirements in the “single-to-single” mode severely affects the efficiency of inspections. To address this problem, this study investigated the problem of a single-impulse flyby co-orbiting two spacecraft and proposed a derivative-free numerical solution method that used the geometric relationship between the two intersections of the target and transfer orbits of the flyby problem in order to transform them into a nonlinear equation in a si
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Books on the topic "Co-orbiting"

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Co-Orbiting Platform Elements ('COPE') Workshop (1987 ESTEC). COPE: Co-orbiting platform elements : proceedings of an ESA Workshop held at ESTEC on 7-8 April 1987. European Space Agency, 1987.

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Co-Orbiting Platform Elements ('COPE') Workshop (1987 ESTEC). COPE: Co-orbiting platform elements : proceedings of an ESA Workshop held at ESTEC on 7-8 April 1987. European Space Agency, 1987.

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United States. National Aeronautics and Space Administration., ed. A critical review of charged particle astronomy at Saturn, the evidence for co-orbiting material in the inner satellite system: NASA-Ames grant no. 2-528, final technical report. National Aeronautics and Space Administration, 1991.

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Book chapters on the topic "Co-orbiting"

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Russell, C. T. "Magnetospheric and solar wind studies with co-orbiting spacecraft." In Solar System Plasmas in Space and Time. American Geophysical Union, 1994. http://dx.doi.org/10.1029/gm084p0085.

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Conference papers on the topic "Co-orbiting"

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Huang, Adam, William W. Hansen, Siegfried W. Janson, and Henry Helvajian. "Microengineered cold gas thruster system for a co-orbiting satellite assistant (COSA)." In Micromachining and Microfabrication, edited by Henry Helvajian, Siegfried W. Janson, and Franz Laermer. SPIE, 2001. http://dx.doi.org/10.1117/12.443032.

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Barresi, Giangrande, Claudio Soddu, Giuseppe Rondinelli, Lucio Caporicci, and A. Loria. "Autonomous navigation of small co-orbiting satellites using C/A GPS code." In Orlando '91, Orlando, FL, edited by Brian J. Horais. SPIE, 1991. http://dx.doi.org/10.1117/12.45889.

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Sharma, Pramod K., Edward A. Romana, A. Peter M. Glassford, and Joyce M. Steakley. "Infrared detection of near co-orbiting particles in the SIRTF field of view." In SPIE's International Symposium on Optical Science, Engineering, and Instrumentation, edited by Philip T. C. Chen, William E. McClintock, and Gary J. Rottman. SPIE, 1998. http://dx.doi.org/10.1117/12.328482.

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Abshire, James B., Pamela S. Millar, and Xiaoli Sun. "Semiconductor Laser-Based Ranging Instrument for Earth Gravity Measurements." In Semiconductor Lasers: Advanced Devices and Applications. Optica Publishing Group, 1995. http://dx.doi.org/10.1364/slada.1995.tub.5.

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A laser ranging instrument is being developed to measure the spatial variations in the Earth's gravity field. It will range in space to a cube corner on a passive co-orbiting sub-satellite with a velocity accuracy of 20 to 50 um/sec by using AlGaAs lasers intensity modulated at 2 GHz.
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Crisp, David, Charles E. Miller, and Philip L. DeCola. "The NASA orbiting carbon observatory: measuring the column-averaged atmospheric CO 2 mole franction abundance from Space." In Remote Sensing, edited by Roland Meynart, Steven P. Neeck, and Haruhisa Shimoda. SPIE, 2006. http://dx.doi.org/10.1117/12.689570.

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Xiao, Yunjie, Qing Shen, and Jin Xing. "A co-orbiting multi-satellite edge computing offload method for LEO constellation networks considering mission request energy consumption." In International Conference on Cyber Security, Artificial Intelligence, and Digital Economy (CSAIDE 2023), edited by Pavel Loskot and Shaozhang Niu. SPIE, 2023. http://dx.doi.org/10.1117/12.2681582.

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Colavita, M. M., M. Shao, M. D. Rayman, and K. L. Short. "OSI: Orbiting Stellar Interferometer for Astrometry and Imaging." In Space Optics for Astrophysics and Earth and Planetary Remote Sensing. Optica Publishing Group, 1991. http://dx.doi.org/10.1364/soa.1991.tuc3.

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OSI, Orbiting Stellar Interferometer, is a concept for a space interferometer mission with both astrometric and imaging goals: 10 μarc sec astrometric accuracy for 16th mag objects in 100 sec of integration time and for 20th mag objects in 1 h, and 5 mas resolution aperture synthesis imaging. The instrument consists of 6 siderostats arranged as 3 co-linear interferometers on a single structure; two interferometers are used for attitude control, and the third for science observations. Delay lines are used for path- length equalization, allowing a large field of view. Available baselines range f
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Boggess, Albert. "History and scientific objectives of the Hubble Space Telescope mission." In OSA Annual Meeting. Optica Publishing Group, 1989. http://dx.doi.org/10.1364/oam.1989.thd1.

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The goal of orbiting an astronomical telescope with very high quality optics was established near the beginning of NASA's history. Its most forceful and persuasive early advocate was Lyman Spitzer, who played a major role in setting both the scientific and technical objectives and in obtaining the support required to carryout the project. Feasibility and engineering studies were begun in the 1960s, culminating in 1977 in contracts for construction of the telescope and its supporting spacecraft by Perkin-Elmer Corp, and Lockheed Missiles & Space Co., respectively. The demanding engineering
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Hee, Jee Loong, R. Santhosh, Kathy Simmons, Graham Johnson, David Hann, and Michael Walsh. "Oil Film Thickness Measurements on Surfaces Close to an Aero-Engine Ball Bearing Using Optical Techniques." In ASME Turbo Expo 2017: Turbomachinery Technical Conference and Exposition. American Society of Mechanical Engineers, 2017. http://dx.doi.org/10.1115/gt2017-63813.

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In a civil aero-engine transmission system a number of bearings are used for shaft location and load support. A bespoke experimental test facility in the University of Nottingham’s Gas Turbine and Transmissions Research Centre (G2TRC) was created to investigate oil shedding from a location bearing. An engine representative ball bearing was installed in the rig and under-race lubrication was supplied via under-race feed to three locations under the inner race and cage. The oil was supplied in an engine representative manner but the delivery system was modified to provide circumferentially even
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Falcoz, Alexandre, Sophie Narbonne, Keyvan Kanani, et al. "Guidance, Navigation & Control on-board architecture for Mars Sample Return Rendezvous & Capture." In ESA 12th International Conference on Guidance Navigation and Control and 9th International Conference on Astrodynamics Tools and Techniques. ESA, 2023. http://dx.doi.org/10.5270/esa-gnc-icatt-2023-108.

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Mars Sample Return (MSR) is a key NASA/ESA collaboration to bring the first samples of Mars material back to Earth for scientific in-depth analysis. Once collected by NASA’s Perseverance rover and injected into Mars’s orbit by the NASA’s Mars Ascent Vehicle (Sampler Retrieval Lander mission), the Orbiting Sample (OS) will be detected, captured and brought back to Earth safely by ESA’s Earth Return Orbiter (ERO) in the early to mid-2030s. This paper focuses on the Guidance, Navigation and Control (GNC) architecture engineered by Airbus Defence and Space to address the uncooperative rendezvous &
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