Relevant bibliographies by topics / Planets

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Planets'

Author: Grafiati
Published: 4 June 2021
Last updated: 25 July 2025

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Journal articles on the topic "Planets"

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Kokaia, Giorgi, Melvyn B. Davies, and Alexander J. Mustill. "Effects of capturing a wide-orbit planet on planetary systems: system stability and habitable zone bombardment rates." Monthly Notices of the Royal Astronomical Society 511, no. 2 (2021): 1685–93. http://dx.doi.org/10.1093/mnras/stab3659.

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ABSTRACT A large fraction of stars are formed in dense clusters. In the cluster, close encounters between stars at distances less than 100 au are common. It has been shown that during close encounters planets can transfer between stars. Such captured planets will be on different orbits compared to planets formed in the system, often on very wide, eccentric, and inclined orbits. We examine how these captured planets affect Kuiper belt-like planetesimal belts in their new systems by examining the effects on habitable planets in systems containing an outer gas giant. We show that these captured p
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Barr, Amy C., Vera Dobos, and László L. Kiss. "Interior structures and tidal heating in the TRAPPIST-1 planets." Astronomy & Astrophysics 613 (May 2018): A37. http://dx.doi.org/10.1051/0004-6361/201731992.

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Context. With seven planets, the TRAPPIST-1 system has among the largest number of exoplanets discovered in a single system so far. The system is of astrobiological interest, because three of its planets orbit in the habitable zone of the ultracool M dwarf. Aims. We aim to determine interior structures for each planet and estimate the temperatures of their rock mantles due to a balance between tidal heating and convective heat transport to assess their habitability. We also aim to determine the precision in mass and radius necessary to determine the planets’ compositions. Methods. Assuming the
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Jackson, Brian, Rory Barne, and Richard Greenberg. "Planetary Transits and Tidal Evolution." Proceedings of the International Astronomical Union 4, S253 (2008): 217–29. http://dx.doi.org/10.1017/s1743921308026434.

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AbstractTransiting planets are generally close enough to their host stars that tides may govern their orbital and thermal evolution. We present calculations of the tidal evolution of recently discovered transiting planets and discuss their implications. The tidal heating that accompanies this orbital evolution can be so great that it controls the planet's physical properties and may explain the large radii observed in several cases, including, for example, TrES-4. Also, since a planet's transit probability depends on its orbit, it evolves due to tides. Current values depend sensitively on the
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Franchini, Alessia, Rebecca G. Martin, and Stephen H. Lubow. "Multiplanet disc interactions in binary systems." Monthly Notices of the Royal Astronomical Society 491, no. 4 (2019): 5351–60. http://dx.doi.org/10.1093/mnras/stz3175.

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ABSTRACT We investigate the evolution of a multiplanet–disc system orbiting one component of a binary star system. The planet–disc system is initially coplanar but misaligned to the binary orbital plane. The planets are assumed to be giants that open gaps in the disc. We first study the role of the disc in shaping the mutual evolution of the two planets using a secular model for low initial tilt. In general, we find that the planets and the disc do not remain coplanar, in agreement with previous work on the single planet case. Instead, the planets and the disc undergo tilt oscillations. A high
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Schaefer, Laura K., and Vivien Parmentier. "The Air Over There: Exploring Exoplanet Atmospheres." Elements 17, no. 4 (2021): 257–63. http://dx.doi.org/10.2138/gselements.17.4.257.

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The atmospheric composition for a rocky exoplanet will depend strongly on the planet’s bulk composition and orbital position. Nontraditional gases may be present in the atmospheres of exceptionally hot planets. Atmospheres of more clement planets will depend on the abundance of volatiles acquired during planet formation and atmospheric removal processes, including escape, condensation, and reaction with the surface. To date, observations of exoplanet atmospheres have focused on giant planets, but future space-and ground-based observatories will revolutionize the precision and spectral resoluti
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Garrido-Deutelmoser, Juan, Cristobal Petrovich, Leonardo Krapp, Kaitlin M. Kratter, and Ruobing Dong. "Substructures in Protoplanetary Disks Imprinted by Compact Planetary Systems." Astrophysical Journal 932, no. 1 (2022): 41. http://dx.doi.org/10.3847/1538-4357/ac6bfd.

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Abstract The substructures observed in protoplanetary disks may be the signposts of embedded planets carving gaps or creating vortices. The inferred masses of these planets often fall in the Jovian regime despite their low abundance compared to lower-mass planets, partly because previous works often assume that a single substructure (a gap or vortex) is caused by a single planet. In this work, we study the possible imprints of compact systems composed of Neptune-like planets (∼10–30 M ⊕) and show that long-standing vortices are a prevalent outcome when their interplanetary separation (Δa) fall
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Howell, Steve B. "On the Value of High Precision Radial Velocity Observations and Astrometric Orbits for Binary Stars Hosting Exoplanets." Research Notes of the AAS 8, no. 9 (2024): 244. http://dx.doi.org/10.3847/2515-5172/ad7e23.

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Abstract Observations have concluded that exoplanet hosting binary stars appear to have wider mean separations than a definitive sample of “field binaries” as well as an apparent deficit of very close pairs. Many exoplanets orbit near their host stars equatorial plane, especially for close-in, small planets. Precision radial velocities of exoplanets in close binary stars are sparse but badly needed in order to provide statistical samples revealing the host stars spin axis and determinations of the masses and orbital planes of their planets. Astrometric orbits of the stars can provide precise b
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Kozhanov, T. S., and Nizyarov N. "Mathematical Theory of Motion of Revolving Axes on the Surface of Planets." International Astronomical Union Colloquium 178 (2000): 619–22. http://dx.doi.org/10.1017/s0252921100061790.

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Let a planet perform translational and rotational motions in the field of solar attraction. Let’s assume that the observer on the surface of the planet, knows (even approximately) an orbit and variations of orientation. It is necessary to clarify the motion of the instanteous rotation axis on the planet’s surface from the observer’s point of view on the planet’s surface.1. The coordinate system, to describe the translational and rotational motions of planets around the Sun we shall take into account the properties of orbits of solar system planets, namely: 1)All planets move in the same direct
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Maldonado, R. F., E. Villaver, A. J. Mustill, and M. Chávez. "Disentangling the parameter space: the role of planet multiplicity in triggering dynamical instabilities on planetary systems around white dwarfs." Monthly Notices of the Royal Astronomical Society 512, no. 1 (2022): 104–15. http://dx.doi.org/10.1093/mnras/stac481.

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ABSTRACT Planets orbiting intermediate- and low-mass stars are in jeopardy as their stellar hosts evolve to white dwarfs (WDs) because the dynamics of the planetary system changes due to the increase of the planet:star mass ratio after stellar mass-loss. In order to understand how the planet multiplicity affects the dynamical stability of post-main sequence (MS) systems, we perform thousands of N-body simulations involving planetary multiplicity as the variable and with a controlled physical and orbital parameter space:equal-mass planets; the same orbital spacing between adjacent planet’s pair
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Li, Gongjie. "Tilting Planets during Planet Scattering." Astrophysical Journal Letters 915, no. 1 (2021): L2. http://dx.doi.org/10.3847/2041-8213/ac0620.

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Dissertations / Theses on the topic "Planets"

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Brickman, Jacklyn E. "Experiments in Biological Planet Formation and Plants: Nourishing Bodies, Nourishing Planets." The Ohio State University, 2020. http://rave.ohiolink.edu/etdc/view?acc_num=osu1595340630648528.

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Trotta, Leonardo Di Schiavi. "Modelo dinâmico 3-D para a evolução do sistema Plutão-Caronte /." Rio Claro, 2017. http://hdl.handle.net/11449/150604.

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Orientador: Tadashi Yokoyama<br>Banca: Nelson Callegari Junior<br>Banca: Rodney da Silva Gomes<br>Resumo: O sistema Plutão-Caronte é um par quase binário em estado de duplo sincronismo. Hoje sabe-se que Plutão possui cinco satélites: Caronte, Styx, Nix, Kerberos e Hydra, onde os últimos quatro são muito menores que Caronte. A origem mais plausível para o sistema Plutão-Caronte é a de um impacto de grandes proporções entre corpos de tamanhos similares, onde o impactador (que viria a ser Caronte) permanece quase intacto após o evento. Caronte iniciaria o movimento orbital próximo de Plutão (ex:
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Joos, Franco. "Polarimetry of gas planets /." Zürich : ETH, 2007. http://e-collection.ethbib.ethz.ch/show?type=diss&nr=17051.

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Turner, Jake D., Robin M. Leiter, Lauren I. Biddle, et al. "Investigating the physical properties of transiting hot Jupiters with the 1.5-m Kuiper Telescope." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/626279.

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We present new photometric data of 11 hot Jupiter transiting exoplanets (CoRoT-12b, HATP-5b, HAT-P-12b, HAT-P-33b, HAT-P-37b, WASP-2b, WASP-24b, WASP-60b, WASP-80b, WASP-103b and XO-3b) in order to update their planetary parameters and to constrain information about their atmospheres. These observations of CoRoT-12b, HAT-P-37b and WASP-60b are the first follow-up data since their discovery. Additionally, the first near-UV transits of WASP-80b and WASP-103b are presented. We compare the results of our analysis with previous work to search for transit timing variations (TTVs) and a wavelength de
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Ortiz, Álvarez Mauricio [Verfasser], and Andreas [Akademischer Betreuer] Quirrenbach. "Planets around giant stars: Two close-in transiting planets and one S-type planet in an eccentric binary system / Mauricio Ortiz Álvarez ; Betreuer: Andreas Quirrenbach." Heidelberg : Universitätsbibliothek Heidelberg, 2017. http://d-nb.info/118073890X/34.

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Lines, Stefan Matthew. "The formation of circumbinary planets." Thesis, University of Bristol, 2016. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.702118.

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The discovery of nearly two thousand extrasolar planets over the last two decades is indicative that planets form everywhere. Exoplanet detections have been made of a plethora of planetary types and sizes across a wide range of orbital characteristics. One of the more exotic locations that planets have been discovered in is around stellar binaries. Their proximity to such a large time-dependent potential from the orbital motion of the stars can be problematic for their formation and long-term stability. Circumbinary planets, with orbits that fully encompass the binary, have been found to orbit
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Janes, Daniel Mark. "Tectonics of one-plate planets." Diss., The University of Arizona, 1990. http://hdl.handle.net/10150/185087.

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The Voyager 2 encounter with Neptune and its moons in August of 1989 completed the discovery phase of planetary exploration. In the 25 years since Mariner 4 returned the first images of another planet, geophysical models for such basic processes as mantle convection and loading which were developed for the Earth have been strained beyond their limits by features such as the Tharsis rise on Mars and the coronae of Miranda which cover as much as a quarter of their planetary circumference. In this work I develop a general planetary shell model in spherical coordinates that is capable of treating
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Fortney, Jonathan J. "The evolution of giant planets." Diss., The University of Arizona, 2004. http://hdl.handle.net/10150/290002.

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As a whole this dissertation aims to understand giant planets as an entire class of astronomical objects. Initially we investigate the mechanics and evolutionary effects of phase separation in the deep interiors of giant planets. We present the first models of Saturn and Jupiter to couple their evolution to both a radiative-atmosphere grid and to high-pressure phase diagrams of hydrogen with helium and other admixtures. We find that previously calculated hydrogen-helium phase diagrams in which Saturn's interior reaches a region of predicted helium immiscibility do not allow enough energy relea
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Zaranek, Sarah Ellen. "Roles of convection in the evolution of planetary interiors and terrestrial lithospheres /." View online version; access limited to Brown University users, 2005. http://wwwlib.umi.com/dissertations/fullcit/3174708.

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Steffen, Jason. "Detecting new planets in transiting systems /." Thesis, Connect to this title online; UW restricted, 2006. http://hdl.handle.net/1773/9686.

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Books on the topic "Planets"

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Peters, Elisa. The planets =: Los planetas. PowerKids Press, 2013.

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Inc, World Book, ed. Neptune and the distant dwarf planets. 2nd ed. World Book, 2007.

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Oxlade, Chris. Planets. Wayland, 2012.

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Sorensen, Lynda. Planets. Rourke Corp., 1993.

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Stone, Lynn M. Planets. Rourke Pub., 2009.

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Jo, Rudy Lisa, ed. Planets! HarperCollins, 2005.

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Kerrod, Robin. Planets. Edited by Forsey Chris and Ross Veronica. Belitha, 2001.

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Tory, Gordon-Harris, ed. Planets. Scholastic, 2012.

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National Geographic Society (U.S.), ed. Planets. National Geographic, 2016.

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Guillain, Charlotte. Planets. Heinemann Library, 2010.

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Book chapters on the topic "Planets"

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Economou, Eleftherios N. "Planets." In From Quarks to the Universe. Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-20654-7_13.

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Hubbard, John H., and Beverly H. West. "Planets." In MacMath 9.2. Springer New York, 1993. http://dx.doi.org/10.1007/978-1-4613-8378-9_17.

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Hubbard, John H., and Beverly H. West. "Planets." In MacMath 9.0. Springer New York, 1992. http://dx.doi.org/10.1007/978-1-4684-0390-9_17.

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Hubbard, John H., and Beverly H. West. "Planets." In MacMath 9.2. Springer Berlin Heidelberg, 1993. http://dx.doi.org/10.1007/978-3-662-25368-7_17.

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Economou, Eleftherios N. "Planets." In A Short Journey from Quarks to the Universe. Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-20089-2_11.

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Canavan, Gerry. "Planets." In The Routledge Companion to Politics and Literature in English. Routledge, 2023. http://dx.doi.org/10.4324/9781003038009-44.

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Kunth, Daniel, and Elena Terlevich. "Planets." In StarWords. Springer International Publishing, 2024. http://dx.doi.org/10.1007/978-3-031-49024-8_9.

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Harwood-Smith, Jennifer. "Planets." In The Routledge Companion to Imaginary Worlds. Routledge, 2017. http://dx.doi.org/10.4324/9781315637525-21.

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Ossendrijver, Mathieu. "Planets." In Babylonian Mathematical Astronomy: Procedure Texts. Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-3782-6_3.

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Hanslmeier, Arnold. "Water on Planets and Dwarf Planets." In Water in the Universe. Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-90-481-9984-6_3.

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Conference papers on the topic "Planets"

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Shao, Michael. "Search for terrestrial planets with SIM Planet Quest." In SPIE Astronomical Telescopes + Instrumentation, edited by John D. Monnier, Markus Schöller, and William C. Danchi. SPIE, 2006. http://dx.doi.org/10.1117/12.671898.

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Seager, Sara, E. B. Ford, and E. L. Turner. "Characterizing Earth-like planets with terrestrial planet finder." In Astronomical Telescopes and Instrumentation, edited by Alan M. Dressler. SPIE, 2002. http://dx.doi.org/10.1117/12.456559.

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Miyazaki, Aya, and Kiyoshi Tomimatsu. "Onomato planets." In the 3rd International Conference. ACM Press, 2009. http://dx.doi.org/10.1145/1517664.1517726.

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Dryomova, G. N., V. V. Dryomov, and A. V. Tutukov. "Interstellar planets." In Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой «Астрономия и исследование космического пространства». Ural University Press, 2021. http://dx.doi.org/10.15826/b978-5-7996-3229-8.26.

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The lecture is devoted to the study of the role of gravitational scattering in the evolution of planetary systems. This mechanism explains the origin of the Oort cloud and free asteroids, comets, and planets (ACPs) from the parent star.
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Marcy, Geoff W., and R. Paul Butler. "First three planets." In Photonics West '96, edited by Stuart A. Kingsley and Guillermo A. Lemarchand. SPIE, 1996. http://dx.doi.org/10.1117/12.243440.

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Schmidt, Rainer, Andrew Lindley, Ross King, Andrew Jackson, Carl Wilson, and Fabian Steeg. "The Planets IF." In the 1st International Digital Preservation Interoperability Framework Symposium. ACM Press, 2010. http://dx.doi.org/10.1145/2039263.2039273.

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Özgen, D. S., Y. Afacan, and E. Surer. "Save the Planets." In GoodTechs '20: 6th EAI International Conference on Smart Objects and Technologies for Social Good. ACM, 2020. http://dx.doi.org/10.1145/3411170.3411253.

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Mazeh, Tsevi. "The Transiting Planets." In STELLAR ASTROPHYSICS WITH THE WORLD'S LARGEST TELESCOPES: First International Workshop on Stellar Astrophysics with the World's Largest Telescopes. AIP, 2005. http://dx.doi.org/10.1063/1.1893330.

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Kramer, Michael. "Planets around Pulsars." In PLANETARY SYSTEMS BEYOND THE MAIN SEQUENCE: Proceedings of the International Conference. AIP, 2011. http://dx.doi.org/10.1063/1.3556180.

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Kochte, M. "Imaging Terrestrial Planets." In THE SEARCH FOR OTHER WORLDS: Fourteenth Astrophysics Conference. AIP, 2004. http://dx.doi.org/10.1063/1.1774528.

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Reports on the topic "Planets"

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Macintosh, B. Direct Imaging of Warm Extrasolar Planets. Office of Scientific and Technical Information (OSTI), 2005. http://dx.doi.org/10.2172/15016011.

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Smullen, Rachel. Binaries, Planets, and Pluto, Oh my! Office of Scientific and Technical Information (OSTI), 2021. http://dx.doi.org/10.2172/1783509.

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Hazi, A. Planets and Stars under the Magnifying Glass. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/907853.

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Hills, J. G., M. P. Goda, and J. C. Solem. Close Encounters of Asteroids and Comets to Planets. Office of Scientific and Technical Information (OSTI), 1999. http://dx.doi.org/10.2172/759193.

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Smullen, Rachel, and Soumi De. Black Holes, Crashing Galaxies, and Strange New Planets. Office of Scientific and Technical Information (OSTI), 2021. http://dx.doi.org/10.2172/1787271.

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Johnson, Zoe. Space Drifters. Montana State University, 2025. https://doi.org/10.15788/1751923342.

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“Space Drifters” is a poem that describes two beings wandering the galaxy together, possibly atfer a catastrophic event destroyed their planet. Space is lonely, but these entities hold on to each other, spiraling together like the double helix of DNA. Rather than succumbing to the darkness, the beings find beauty in their drifting. The imagery attempts to capture the glory of the universe—stars, planets, swirling masses of color. Ultimately, the universe is not uncaring. It guides the couple, illuminating the path to new beginnings. Together, the space
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Celliers, P., J. Eggert, G. Collins, et al. Creating the Core Conditions of Extra-solar and Solar Giant Planets. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/902290.

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Ullom, J., M. Cunningham, B. Macintosh, T. Miyazaki, and S. Labov. ''High-Speed, Photon-Counting Camera for the Detection of Extrasolar Planets''. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/15003349.

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Dutta, Sumit. Identifying Minor Planets in UCAC Data and Deriving Accurate O-C. Defense Technical Information Center, 2006. http://dx.doi.org/10.21236/ada455924.

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Duckss, Weitter. Why do Hydrogen and Helium Migrate from Some Planets and Smaller Objects? Intellectual Archive, 2019. http://dx.doi.org/10.32370/iaj.2055.

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