Gotowa bibliografia na temat „Planetary bodies”
Utwórz poprawne odniesienie w stylach APA, MLA, Chicago, Harvard i wielu innych
Spis treści
Zobacz listy aktualnych artykułów, książek, rozpraw, streszczeń i innych źródeł naukowych na temat „Planetary bodies”.
Przycisk „Dodaj do bibliografii” jest dostępny obok każdej pracy w bibliografii. Użyj go – a my automatycznie utworzymy odniesienie bibliograficzne do wybranej pracy w stylu cytowania, którego potrzebujesz: APA, MLA, Harvard, Chicago, Vancouver itp.
Możesz również pobrać pełny tekst publikacji naukowej w formacie „.pdf” i przeczytać adnotację do pracy online, jeśli odpowiednie parametry są dostępne w metadanych.
Artykuły w czasopismach na temat "Planetary bodies"
Hu, H., i B. Wu. "PLANETARY3D: A PHOTOGRAMMETRIC TOOL FOR 3D TOPOGRAPHIC MAPPING OF PLANETARY BODIES". ISPRS Annals of Photogrammetry, Remote Sensing and Spatial Information Sciences IV-2/W5 (29.05.2019): 519–26. http://dx.doi.org/10.5194/isprs-annals-iv-2-w5-519-2019.
Pełny tekst źródłaKadish, Jon, J. R. Barber, P. D. Washabaugh i D. J. Scheeres. "Stresses in accreted planetary bodies". International Journal of Solids and Structures 45, nr 2 (styczeń 2008): 540–50. http://dx.doi.org/10.1016/j.ijsolstr.2007.08.008.
Pełny tekst źródłaConnolly, William E. "Bodies, Microbes and the Planetary". Theory & Event 21, nr 4 (październik 2018): 962–67. http://dx.doi.org/10.1353/tae.2018.0058.
Pełny tekst źródłaCockell, Charles S., i Gerda Horneck. "Planetary parks—formulating a wilderness policy for planetary bodies". Space Policy 22, nr 4 (listopad 2006): 256–61. http://dx.doi.org/10.1016/j.spacepol.2006.08.006.
Pełny tekst źródłaKotliarov, I. D. "Classification of celestial bodies within planetary systems". Moscow University Physics Bulletin 63, nr 6 (grudzień 2008): 416–19. http://dx.doi.org/10.3103/s0027134908060118.
Pełny tekst źródłaMelosh, H. J. "Ejection of rock fragments from planetary bodies". Geology 13, nr 2 (1985): 144. http://dx.doi.org/10.1130/0091-7613(1985)13<144:eorffp>2.0.co;2.
Pełny tekst źródłaLin, Yucong, Melissa Bunte, Srikanth Saripalli, James Bell i Ronald Greeley. "Autonomous volcanic plume detection on planetary bodies". Acta Astronautica 97 (kwiecień 2014): 151–63. http://dx.doi.org/10.1016/j.actaastro.2013.11.029.
Pełny tekst źródłaBinzel, Richard P. "Small bodies looming large in planetary science". Nature Astronomy 3, nr 4 (kwiecień 2019): 282–83. http://dx.doi.org/10.1038/s41550-019-0747-6.
Pełny tekst źródłaSkripka, V. L., i L. H. Minyazeva. "Planetary rock-breaking bodies and horizontal drilling". Proceedings of higher educational establishments. Geology and Exploration, nr 5 (5.02.2023): 86–93. http://dx.doi.org/10.32454/0016-7762-2022-64-5-86-93.
Pełny tekst źródłaVisser, R. G., C. W. Ormel, C. Dominik i S. Ida. "Spinning up planetary bodies by pebble accretion". Icarus 335 (styczeń 2020): 113380. http://dx.doi.org/10.1016/j.icarus.2019.07.014.
Pełny tekst źródłaRozprawy doktorskie na temat "Planetary bodies"
Romeo, Michael Joseph. "Routing Among Planetary Bodies". Kent State University / OhioLINK, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=kent1528470515838277.
Pełny tekst źródłaChabot, Nancy Lynne. "Geochemical studies of the cores of terrestrial planetary bodies". Diss., The University of Arizona, 1999. http://hdl.handle.net/10150/289052.
Pełny tekst źródłaHarri, Ari-Matti. "In situ obreviations of the atmospheres of terrestrial planetary bodies /". Helsinki : Finn. Meteorological Inst, 2005. http://www.gbv.de/dms/goettingen/509702546.pdf.
Pełny tekst źródłaHilbert, Bryan (Bryan Nathaniel) 1977. "Stellar occultation lightcurve modeling for elliptical occulting bodies". Thesis, Massachusetts Institute of Technology, 2001. http://hdl.handle.net/1721.1/54444.
Pełny tekst źródłaIncludes bibliographical references (leaf 41).
We present a new method of calculating model lightcurves for stellar occultations by the Jovian planets. We model the occulting planet as a three-dimensional body of non-zero ellipticity, and define two ellipses of intersection with the body which dictate the appearance of the lightcurve. These include the visible-limb plane ellipse, which is the observed figure of the body as seen in the sky, and the line-of-sight ellipse, which contains the line of sight to the occulted star, and is the plane in which the starlight is refracted. The observed stellar flux during the occultation is primarily dictated by the ellipticity and subsequent radius of curvature of the instantaneous ellipse in the line-of-sight plane. This new method is applied to several test cases, as well as to the Jovian occultation of HIP9369 on 10 October 1999. Lightcurves generated by this model are compared to identical situations using the method published in Hubbard et al. (1997), showing that the Hubbard model works well for low-latitude occultations, but fails at higher latitudes. In the case of the high-latitude Jovian occultation, the best-fit lightcurve, produced from this new method, yielded a half-light equatorial radius of 71,343±1.2 km with a scale height of 19.25±0.5km, and an isothermal temperature of 139K. The same data, fit using a lightcurve generated by the method described in Hubbard et al. (1997), resulted in a half-light equatorial radius of 71,819km with a scale height of 17.9km with errors comparable to the previous fit, resulting in an isothermal temperature of 129K. Lightcurves are numerically generated for an ellipsoidal planet and, for comparison, an approximation to the ellipsoidal case consisting of a sphere with radius equal to the radius of curvature of the ellipsoid at the half-light point. We find that in the case of an occultation where the line-of-sight ellipticity does not vary, that the radius of curvature approximation matches the ellipsoidal planet lightcurve to within 0.007%. For an oblique occultation however, the line-of-sight ellipticity varies, and the approximation, using only a single radius of curvature sphere, is only good to about 1%. As a result, we find that using a model such as that presented in Baum and Code (1953) to fit the lightcurve of an ellipsoidal planet can return values for half-light radius (after accounting for the distance between the center of curvature and the center of the body) which may match the local distance to the center of the ellipsoid to a fraction of a percent, while returning values of scale height which may be in error by several percent. Test cases are also then put through numerical inversions, to obtain temperature versus pressure profiles. Test cases with spherical planets return temperature profiles that match those used to create the lightcurves, while test cases with ellipsoidal planets return temperature profiles which can differ from the input temperatures by tens of degrees, assuming a constant local gravity over the course of the occultation.
by Bryan Hilbert.
S.M.
Theis, Karen Julia. "Iron isotope fractionation of planetary bodies during early solar system formation processes". Thesis, University of Manchester, 2008. http://www.manchester.ac.uk/escholar/uk-ac-man-scw:163898.
Pełny tekst źródłaKanata, Sayaka. "Research on Localization and Guidance for Space Rovers on Small Planetary Bodies". 京都大学 (Kyoto University), 2010. http://hdl.handle.net/2433/123338.
Pełny tekst źródłaRuprecht, Jessica Dawn. "Astronomical studies of solar system bodies 2060 Chiron and 1 Ceres". Thesis, Massachusetts Institute of Technology, 2013. http://hdl.handle.net/1721.1/82301.
Pełny tekst źródłaCataloged from PDF version of thesis.
Includes bibliographical references (p. 43-45).
In this thesis two separate projects are investigated, a stellar occultation by 2060 Chiron and rotationally resolved spectra of 1 Ceres. On 29 November 2011 UT, 2060 Chiron occulted a 14-mag star; data were successfully obtained at the 3-m IRTF on Mauna Kea and 2-m Faulkes North Telescope at Haleakala. The IRTF lightcurve shows a solid-body detection of Chiron's nucleus with a chord lasting 16.04 seconds, corresponding to a chord length of 158±14 km. Symmetric, dual extinction features in the Faulkes light curve indicate the presence of optically thick material roughly 300 km from the body midpoint. The duration of the features indicates a ~ 3 km feature separated by 10-14 km from a second - 7 km feature. The symmetry, optical thickness, and narrow size of these features allows for the intriguing possibility of a near-circular arc or shell of material. Rotationally resolved spectra of Ceres in the 0.43-0.85 micron range were observed using the DeVeny spectrograph on the Perkins 72-inch telescope at Lowell Observatory. Spectral differences as a function of phase were investigated. It is concluded that Ceres' surface is uniform at the 1% level at visible wavelengths. Additionally, the 0.6 and 0.67 pm features reported by Vilas and McFadden [1992] and Fornasier et al. [1999] are not seen at any phase at the 1% level.
by Jessica Dawn Ruprecht.
S.M.
Bryson, James Francis Joseph. "The origin of ancient magnetic activity on small planetary bodies : a nanopaleomagnetic study". Thesis, University of Cambridge, 2015. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.708801.
Pełny tekst źródłaBettella, Alberto. "Generation and propagation of vibrations on satellite structures and planetary bodies after hypervelocity impacts". Doctoral thesis, Università degli studi di Padova, 2008. http://hdl.handle.net/11577/3425965.
Pełny tekst źródłaAlibay, Farah. "Evaluation of multi-vehicle architectures for the exploration of planetary bodies in the Solar System". Thesis, Massachusetts Institute of Technology, 2014. http://hdl.handle.net/1721.1/87476.
Pełny tekst źródłaCataloged from PDF version of thesis.
Includes bibliographical references (pages 193-210).
Planetary exploration missions are becoming increasingly complex and expensive due to ever more ambitious scientific and technical goals. On the other hand, budgets in planetary science have suffered from dramatic cuts over the past decade and projections estimate a flat budget of approximately $1.2B/year for the upcoming years. This has led to a desire for a reduction in the risk and complexity, as well as an increase in the robustness and reliability, of planetary exploration vehicles. One of the methods proposed to deal with this issue is the use of distributed, multi-vehicle architectures as a replacement for the traditional large, monolithic systems used in flagship missions. However, mission concept formulation engineers do not possess the tools to include multi-vehicle architectures in their early trade space exploration process. This is mostly due to the fact that these types of architectures cannot be readily evaluated against monolithic systems through the use of traditional mass-based metrics. Furthermore, in multi-vehicle system, architectural decisions about one vehicle, such as instrument or capability selection, quickly propagate through the entire system and impose requirements on the other vehicles. This can be difficult to model without going through detailed point designs. The objective of this thesis is to explore the potential benefits of both spatially and temporally distributed multi-vehicle systems, where the vehicles are heterogeneous, as compared to monolithic systems. Specifically, a set of metrics mapping the effects of using multi-vehicle systems on science benefit, complexity, mass, cost, coverage, productivity and risk are developed. Furthermore, a software tool to simulate the performance of teams of planetary surface vehicles in their operational environment has been built and its use demonstrated. Finally, the framework put forward in this thesis is used to perform several case studies, including a case study on the exploration of the Jovian moon Europa and another on the ascent and return components of a Mars Sample Return mission. From these, distributed systems are shown to provide increased science return and robustness as well as lower development and manufacturing costs as compared to their monolithic equivalents.
by Farah Alibay.
Ph. D.
Książki na temat "Planetary bodies"
Mann, Ingrid, Akiko Nakamura i Tadashi Mukai, red. Small Bodies in Planetary Systems. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76935-4.
Pełny tekst źródłaNakamura, A. M., T. Mukai i Ingrid Mann. Small bodies in planetary systems. Berlin: Springer, 2009.
Znajdź pełny tekst źródłaHanslmeier, Arnold, Stephan Kempe i Joseph Seckbach, red. Life on Earth and other Planetary Bodies. Dordrecht: Springer Netherlands, 2012. http://dx.doi.org/10.1007/978-94-007-4966-5.
Pełny tekst źródła1929-, Teisseyre R., Leliwa-Kopystyński J. 1937-, Lang B i Bakun-Czubarow N, red. Evolution of the Earth and other planetary bodies. Amsterdam: Elsevier, 1992.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration., red. Solar wind effects on atmospheres of the weakly magnetized bodies--Mars, Titan, and the moon: Final technical report. [Washington, DC: National Aeronautics and Space Administration, 1996.
Znajdź pełny tekst źródłaLuhmann, Janet G. Solar wind effects on atmospheres of the weakly magnetized bodies--Mars, Titan, and the moon: Final technical report. [Washington, DC: National Aeronautics and Space Administration, 1996.
Znajdź pełny tekst źródłaDigitalis, Raven. Planetary spells & rituals: Practicing dark & light magick aligned with the cosmic bodies. Woodbury, Minn: Llewellyn Publications, 2010.
Znajdź pełny tekst źródłaDigitalis, Raven. Planetary spells & rituals: Practicing dark & light magick aligned with the cosmic bodies. Woodbury, Minn: Llewellyn Publications, 2010.
Znajdź pełny tekst źródłaNational Research Council (U.S.). Task Group on Sample Return from Small Solar System Bodies. Evaluating the biological potential in samples returned from planetary satellites and small solar system bodies: Framework for decision making. Washington, D.C: National Academy Press, 1998.
Znajdź pełny tekst źródłaMEVTV, Workshop on the Evolution of Magma Bodies on Mars (1990 San Diego Calif ). MEVTV Workshop on the Evolution of Magma Bodies on Mars: Held at San Diego, California, January 15-17, 1990. Houston, Tex: The Institute, 1990.
Znajdź pełny tekst źródłaCzęści książek na temat "Planetary bodies"
Hare, Trent Michael. "Mapping planetary bodies". W The Routledge Handbook of Geospatial Technologies and Society, 562–76. London: Routledge, 2023. http://dx.doi.org/10.4324/9780367855765-46.
Pełny tekst źródłaSchmedemann, Nico, Matteo Massironi, Roland Wagner i Katrin Stephan. "Small Bodies and Dwarf Planets". W Planetary Geology, 311–43. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-65179-8_13.
Pełny tekst źródłaJiwani, Yasmin. "Contagious Bodies". W Planetary Health Humanities and Pandemics, 179–98. New York: Routledge, 2024. http://dx.doi.org/10.4324/9781003367581-12.
Pełny tekst źródłaSaur, Joachim, Fritz M. Neubauer i Karl-Heinz Glassmeier. "Induced Magnetic Fields in Solar System Bodies". W Planetary Magnetism, 391–421. New York, NY: Springer New York, 2009. http://dx.doi.org/10.1007/978-1-4419-5901-0_12.
Pełny tekst źródłaMittlefehldt, David W., Timothy J. McCoy, Cyrena A. Goodrich i Alfred Kracher. "Chapter 4. NON-CHONDRITIC METEORITES FROM ASTEROIDAL BODIES". W Planetary Materials, redaktor James J. Papike, 523–718. Berlin, Boston: De Gruyter, 1998. http://dx.doi.org/10.1515/9781501508806-019.
Pełny tekst źródłaBaur, Oliver. "Gravity Field of Planetary Bodies". W Encyclopedia of Geodesy, 1–6. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-02370-0_46-1.
Pełny tekst źródłaDwivedi, Om Prakash. "Ecoprogramming the Vulnerable Bodies". W Eco-Anxiety and Planetary Hope, 111–18. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-08431-7_11.
Pełny tekst źródłaChristou, A. A. "Future Planetary Missions". W The Dynamics of Small Bodies in the Solar System, 587–93. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-015-9221-5_56.
Pełny tekst źródłaJewitt, D. "Six Hot Topics in Planetary Astronomy". W Small Bodies in Planetary Systems, 1–37. Berlin, Heidelberg: Springer Berlin Heidelberg, 2008. http://dx.doi.org/10.1007/978-3-540-76935-4_9.
Pełny tekst źródłaHussmann, H., F. Sohl i J. Oberst. "4.2.2 Basic data of planetary bodies". W Solar System, 208–29. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-88055-4_15.
Pełny tekst źródłaStreszczenia konferencji na temat "Planetary bodies"
Remo, John L. "Classifying Solid Planetary Bodies". W NEW TRENDS IN ASTRODYNAMICS AND APPLICATIONS III. AIP, 2007. http://dx.doi.org/10.1063/1.2710063.
Pełny tekst źródłaSchulte, Mitch. "Remote sensing of planetary bodies". W Autonomous Systems: Sensors, Processing, and Security for Ground, Air, Sea, and Space Vehicles and Infrastructure 2024, redaktorzy Michael C. Dudzik, Theresa J. Axenson i Stephen M. Jameson. SPIE, 2024. http://dx.doi.org/10.1117/12.3023813.
Pełny tekst źródłaWhite, Robert A. "Generating Artificial Gravity on Planetary Bodies". W 55th AIAA Aerospace Sciences Meeting. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2017. http://dx.doi.org/10.2514/6.2017-1447.
Pełny tekst źródłaDollfus, Audouin. "Telescopic polarimetry of planetary bodies: an overview". W San Diego '92, redaktor Walter G. Egan. SPIE, 1992. http://dx.doi.org/10.1117/12.138829.
Pełny tekst źródłaMARTINO, MARIO DI, ALBINO CARBOGNANI i ALBERTO CELLINO. "DETECTION OF TRANSIENT PHENOMENA ON PLANETARY BODIES". W The 32nd Session of International Seminars and International Collaboration. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701787_0053.
Pełny tekst źródłaFoster, Cyrus, i Matthew Daniels. "Mission Opportunities for Human Exploration of Nearby Planetary Bodies". W AIAA SPACE 2010 Conference & Exposition. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2010. http://dx.doi.org/10.2514/6.2010-8609.
Pełny tekst źródłaGold, Thomas. "Reasons for expecting subsurface life on many planetary bodies". W Optical Science, Engineering and Instrumentation '97, redaktor Richard B. Hoover. SPIE, 1997. http://dx.doi.org/10.1117/12.278775.
Pełny tekst źródłaPicardi, Giovanni, i Roberto Seu. "Radar Sounding of Planetary Bodies: An Instrument Design Approach". W 20th European Microwave Conference, 1990. IEEE, 1990. http://dx.doi.org/10.1109/euma.1990.336266.
Pełny tekst źródłaYucong Lin, Melissa Bunte, Srikanth Saripalli i Ronald Greeley. "Autonomous detection of volcanic plumes on outer planetary bodies". W 2012 IEEE International Conference on Robotics and Automation (ICRA). IEEE, 2012. http://dx.doi.org/10.1109/icra.2012.6224796.
Pełny tekst źródłaPrimeau, Gilles. "Magnetoaerodynamic (MAD) propulsion for exploration of atmosphere-bearing planetary bodies". W 34th AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1998. http://dx.doi.org/10.2514/6.1998-3408.
Pełny tekst źródłaRaporty organizacyjne na temat "Planetary bodies"
Shin, Tony. The Search for Water on Planetary Bodies using Neutron Science. Office of Scientific and Technical Information (OSTI), marzec 2022. http://dx.doi.org/10.2172/1853890.
Pełny tekst źródłaGender justice and planetary health. Global Health 50/50, 2024. http://dx.doi.org/10.56649/tauj1442.
Pełny tekst źródła