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Journal articles on the topic 'Space flight to Saturn'

Author: Grafiati

Published: 4 June 2021

Last updated: 31 July 2024

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1

Himelblau, H., D. Kern, and G. Davis. "Summary of Cassini Acoustic Criteria Development Using Titan IV Flight Data." Journal of the IEST 36, no. 5 (September 1, 1993): 19–27. http://dx.doi.org/10.17764/jiet.2.36.5.c408vvk263q216u5.

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The Cassini spacecraft is being developed by the Jet Propulsion Laboratory (JPL) for the National Aeronautics and Space Administration (NASA) to orbit and explore the planet Saturn, its rings, and satellites. Cassini will be launched on a Titan IV and boosted out of Earth orbit by a Centaur. This paper discusses the development of Cassini acoustic criteria using Titan IV flight data. Factors affecting the development of Cassini acoustic criteria using corrected Titan IV flight data1 include the statistical methods used to account for spatial and flight-to-flight variations, the use of maximax spectra, data corrections for acoustic pressure increases near the payload fairing surfaces, and corrections for payload fill factor effects. Separate acoustic criteria were developed for the two launch sites.

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2

Solórzano, Carlos Renato Huaura, Antonio Fernando Bertachini de Almeida Prado, and Alexander Alexandrovich Sukhanov. "Analysis of Electric Propulsion System for Exploration of Saturn." Mathematical Problems in Engineering 2009 (2009): 1–14. http://dx.doi.org/10.1155/2009/756037.

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Exploration of the outer planets has experienced new interest with the launch of the Cassini and the New Horizons Missions. At the present time, new technologies are under study for the better use of electric propulsion system in deep space missions. In the present paper, the method of the transporting trajectory is used to study this problem. This approximated method for the flight optimization with power-limited low thrust is based on the linearization of the motion of a spacecraft near a keplerian orbit that is close to the transfer trajectory. With the goal of maximizing the mass to be delivered in Saturn, several transfers were studied using nuclear, radioisotopic and solar electric propulsion systems.

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3

Weber, Jessica M., Theresa C. Marlin, Medha Prakash, Bronwyn L. Teece, Katherine Dzurilla, and Laura M. Barge. "A Review on Hypothesized Metabolic Pathways on Europa and Enceladus: Space-Flight Detection Considerations." Life 13, no. 8 (August 11, 2023): 1726. http://dx.doi.org/10.3390/life13081726.

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Enceladus and Europa, icy moons of Saturn and Jupiter, respectively, are believed to be habitable with liquid water oceans and therefore are of interest for future life detection missions and mission concepts. With the limited data from missions to these moons, many studies have sought to better constrain these conditions. With these constraints, researchers have, based on modeling and experimental studies, hypothesized a number of possible metabolisms that could exist on Europa and Enceladus if these worlds host life. The most often hypothesized metabolisms are methanogenesis for Enceladus and methane oxidation/sulfate reduction on Europa. Here, we outline, review, and compare the best estimated conditions of each moon’s ocean. We then discuss the hypothetical metabolisms that have been suggested to be present on these moons, based on laboratory studies and Earth analogs. We also detail different detection methods that could be used to detect these hypothetical metabolic reactions and make recommendations for future research and considerations for future missions.

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4

Cartlidge, Edwin. "Space scientists return to Saturn." Physics World 17, no. 6 (June 2004): 10. http://dx.doi.org/10.1088/2058-7058/17/6/20.

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5

Anonymous. "Space flight." Eos, Transactions American Geophysical Union 75, no. 48 (1994): 562. http://dx.doi.org/10.1029/eo075i048p00562-04.

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6

Jones, Willie D. "Space Flight." IEEE Spectrum 60, no. 11 (November 2023): 14–15. http://dx.doi.org/10.1109/mspec.2023.10309283.

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7

Burne, Sofía, César Bertucci, Nick Sergis, Laura F. Morales, Nicholas Achilleos, Beatriz Sánchez-Cano, Yaireska Collado-Vega, Sergio Dasso, Niklas J. T. Edberg, and Bill S. Kurth. "Space Weather in the Saturn–Titan System." Astrophysical Journal 948, no. 1 (May 1, 2023): 37. http://dx.doi.org/10.3847/1538-4357/acc738.

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Abstract New evidence based on Cassini magnetic field and plasma data has revealed that the discovery of Titan outside Saturn’s magnetosphere during the T96 flyby on 2013 December 1 was the result of the impact of two consecutive interplanetary coronal mass ejections (ICMEs) that left the Sun in 2013 early November and interacted with the moon and the planet. We study the dynamic evolution of Saturn's magnetopause and bow shock, which evidences a magnetospheric compression from late November 28 to December 4 (at least), under prevailing solar wind dynamic pressures of 0.16–0.3 nPa. During this interval, transient disturbances associated with the two ICMEs are observed, allowing for the identification of their magnetic structures. By analyzing the magnetic field direction, and the pressure balance in Titan’s induced magnetosphere, we show that Cassini finds Saturn’s moon embedded in the second ICME after being swept by its interplanetary shock and amid a shower of solar energetic particles that may have caused dramatic changes in the moon’s lower ionosphere. Analyzing a list of Saturn's bow shock crossings during 2004–2016, we find that the magnetospheric compression needed for Titan to be in the supersonic solar wind can be generally associated with the presence of an ICME or a corotating interaction region. This leads to the conclusion that Titan would rarely face the pristine solar wind, but would rather interact with transient solar structures under extreme space weather conditions.

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8

Gordon, Robert S. C. "Rings of Saturn: Fellini Rosi." Journal of Italian Cinema & Media Studies 10, no. 3 (June 1, 2022): 449–74. http://dx.doi.org/10.1386/jicms_00139_1.

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This article offers a comparative reading of Gianfranco Rosi’s Sacro GRA (‘Holy GRA’) (2013) and Federico Fellini’s Roma (1972). It sets Sacro GRA within Rosi’s career, his ambiguous identity as an ‘Italian’ filmmaker and the film’s relation to the history of cinema in/on Rome and psycho-geographical road movies. It moves on to analyse Rosi’s treatment of place and urban space, comparing key motifs and patterns in Sacro GRA with the short episode of Fellini’s Roma, also set on the GRA, Rome’s urban outer ring road. This dual reading is articulated around four axes of comparison in the construction and evocation of the ring-road space: street furniture, metacinematic frames and recordings, noises and silences, machines and monsters. Through these and other incidental constellations, the article argues that the two films display parallel, at times symmetrical, fascinations with the urban as simultaneously a space of utopia and dystopia, nature and the man-made, past and future.

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9

ROBERTSON, DONALD F. "Human space flight." Nature 338, no. 6210 (March 1989): 10. http://dx.doi.org/10.1038/338010a0.

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10

Woolford, Barbara J. "Manned Space Flight." Proceedings of the Human Factors Society Annual Meeting 30, no. 4 (September 1986): 354–57. http://dx.doi.org/10.1177/154193128603000410.

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An overview of manned space flight is given. This describes the key goals and achievements of the space programs of the United States and of the Soviet Union. The importance of the “Man” in manned space flight is emphasized. Human factors are shown to have played an ever increasing role in the design of manned space craft.

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11

Goddard, Alison. "Space: Mission to Saturn ready to blast off." Physics World 10, no. 10 (October 1997): 7. http://dx.doi.org/10.1088/2058-7058/10/10/7.

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12

Marzari, F., P. Tricarico, and H. Scholl. "Saturn Trojans: Stability Regions in the Phase Space." Astrophysical Journal 579, no. 2 (November 10, 2002): 905–13. http://dx.doi.org/10.1086/342873.

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13

赵, 士洋. "Space Flight Science Based on the Expansion of Space Flight Engineering." Interdisciplinary Science Letters 05, no. 01 (2021): 1–5. http://dx.doi.org/10.12677/isl.2021.51001.

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14

Smith, S. M., B. L. Rice, H. Dlouhy, and S. R. Zwart. "Assessment of Nutritional Intake During Space Flight and Space Flight Analogs." Procedia Food Science 2 (2013): 27–34. http://dx.doi.org/10.1016/j.profoo.2013.04.006.

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15

Ohshima, Hiroshi. "Human Space Flight and Space Medicine." TRENDS IN THE SCIENCES 10, no. 9 (2005): 33–39. http://dx.doi.org/10.5363/tits.10.9_33.

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16

Sanderson, Katharine. "Commercial space flight: Scientists in space." Nature 476, no. 7361 (August 2011): 477–78. http://dx.doi.org/10.1038/nj7361-477a.

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17

Fischer, Georg, Donald A. Gurnett, William S. Kurth, Ferzan Akalin, Philippe Zarka, Ulyana A. Dyudina, William M. Farrell, and Michael L. Kaiser. "Atmospheric Electricity at Saturn." Space Science Reviews 137, no. 1-4 (May 23, 2008): 271–85. http://dx.doi.org/10.1007/s11214-008-9370-z.

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18

Hubbard, W. B., C. C. Porco, D. M. Hunten, G. H. Rieke, M. J. Rieke, D. W. McCarthy, V. Haemmerle, et al. "The Occultation of 28 Sgr by Saturn: Saturn Pole Position and Astrometry." Icarus 103, no. 2 (June 1993): 215–34. http://dx.doi.org/10.1006/icar.1993.1067.

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19

Weigt, D. M., W. R. Dunn, C. M. Jackman, R. Kraft, G. Branduardi-Raymont, J. D. Nichols, A. D. Wibisono, M. F. Vogt, and G. R. Gladstone. "Searching for Saturn’s X-rays during a rare Jupiter Magnetotail crossing using Chandra." Monthly Notices of the Royal Astronomical Society 506, no. 1 (June 14, 2021): 298–305. http://dx.doi.org/10.1093/mnras/stab1680.

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ABSTRACT Every 19 yr, Saturn passes through Jupiter’s ‘flapping’ magnetotail. Here, we report Chandra X-ray observations of Saturn planned to coincide with this rare planetary alignment and to analyse Saturn’s magnetospheric response when transitioning to this unique parameter space. We analyse three Director’s Discretionary Time (DDT) observations from the High Resolution Camera (HRC-I) on-board Chandra, taken on 2020 November 19, 21, and 23 with the aim to find auroral and/or disc emissions. We infer the conditions in the kronian system by looking at coincident soft X-ray solar flux data from the Geostationary Operational Environmental Satellite (GOES) and Hubble Space Telescope (HST) observations of Saturn’s ultraviolet (UV) auroral emissions. The large Saturn–Sun–Earth angle during this time would mean that most flares from the Earth-facing side of the Sun would not have impacted Saturn. We find no significant detection of Saturn’s disc or auroral emissions in any of our observations. We calculate the 3σ upper band energy flux of Saturn during this time to be 0.9–3.04 × 10−14 erg cm−2 s−1 which agrees with fluxes found from previous modelled spectra of the disc emissions. We conclude by discussing the implications of this non-detection and how it is imperative that the next fleet of X-ray telescope (such as Athena and the Lynx mission concept) continue to observe Saturn with their improved spatial and spectral resolution and very enhanced sensitivity to help us finally solve the mysteries behind Saturn’s apparently elusive X-ray aurora.

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20

Smith, Scott, and Sara Zwart. "Magnesium and Space Flight." Nutrients 7, no. 12 (December 8, 2015): 10209–22. http://dx.doi.org/10.3390/nu7125528.

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21

Dinges, David F. "Sleep in Space Flight." American Journal of Respiratory and Critical Care Medicine 164, no. 3 (August 2001): 337–38. http://dx.doi.org/10.1164/ajrccm.164.3.2105072a.

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22

Bowler, S. "Human space-flight review." Astronomy & Geophysics 46, no. 1 (February 1, 2005): 1.7—b—1.7. http://dx.doi.org/10.1093/astrog/46.1.1.7-b.

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23

Maryniak, Gregg. "Seeking sustainable space flight." Physics World 16, no. 12 (December 2003): 17–18. http://dx.doi.org/10.1088/2058-7058/16/12/28.

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24

Smith, Scott M., Peter N. Uchakin, and Brian W. Tobin. "Space flight nutrition research." Nutrition 18, no. 10 (October 2002): 926–29. http://dx.doi.org/10.1016/s0899-9007(02)00904-8.

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25

Varma, Madhu, Tomoi Sato, Lihua Zhang, and Michael M. Meguid. "Space flight related anorexia." Lancet 356, no. 9230 (August 2000): 681. http://dx.doi.org/10.1016/s0140-6736(05)73828-9.

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26

Kemp, M. H. D. "Solar-powered space flight." Aeronautical Journal 109, no. 1102 (December 2005): 619–30. http://dx.doi.org/10.1017/s0001924000000956.

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Abstract The aim of this paper is analyse the practicality or otherwise of solar-powered propulsion (after launch using conventional chemical rocketry) for a space vehicle’s late pre-orbital trajectory phase, for orbital transfer and for post-orbital flight. We introduce a ‘concept’ vehicle that in principle permits the use of solar-powered propulsion in each of these stages. Some of the technical challenges that such a vehicle might face are analysed, including the problem of how to keep a large ultra-low mass optical concentrator arrangement sufficiently accurately positioned in different parts of such a trajectory.

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27

Lin, Xu. "Space flight visual simulation." Acta Astronautica 12, no. 3 (March 1985): 177–85. http://dx.doi.org/10.1016/0094-5765(85)90059-1.

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28

de la Fuente Marcos, C., and R. de la Fuente Marcos. "Centaur 2013 VZ₇₀: Debris from Saturn’s irregular moon population?" Astronomy & Astrophysics 657 (January 2022): A59. http://dx.doi.org/10.1051/0004-6361/202142166.

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Context. Saturn has an excess of irregular moons. This is thought to be the result of past collisional events. Debris produced during such episodes in the neighborhood of a host planet can evolve into co-orbitals trapped in quasi-satellite and/or horseshoe resonant states. A recently announced centaur, 2013 VZ70, follows an orbit that could be compatible with those of prograde Saturn’s co-orbitals. Aims. We perform an exploration of the short-term dynamical evolution of 2013 VZ70 to confirm or reject a co-orbital relationship with Saturn. A possible connection with Saturn’s irregular moon population is also investigated. Methods. We studied the evolution of 2013 VZ70 backward and forward in time using N-body simulations, factoring uncertainties into the calculations. We computed the distribution of mutual nodal distances between this centaur and a sample of moons. Results. We confirm that 2013 VZ70 is currently trapped in a horseshoe resonant state with respect to Saturn but that it is a transient co-orbital. We also find that 2013 VZ70 may become a quasi-satellite of Saturn in the future and that it may experience brief periods of capture as a temporary irregular moon. This centaur might also pass relatively close to known irregular moons of Saturn. Conclusions. Although an origin in trans-Neptunian space is possible, the hostile resonant environment characteristic of Saturn’s neighborhood favors a scenario of in situ formation via impact, fragmentation, or tidal disruption as 2013 VZ70 can experience encounters with Saturn at very low relative velocity. An analysis of its orbit within the context of those of the moons of Saturn suggests that 2013 VZ70 could be related to the Inuit group, particularly Siarnaq, the largest and fastest rotating member of the group. Also, the mutual nodal distances of 2013 VZ70 and the moons Fornjot and Thrymr are below the first percentile of the distribution.

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29

Hirst, Ann E., and E. Keithlloyd. "Cassini, His Ovals and a Space Probe to Saturn." Mathematical Gazette 81, no. 492 (November 1997): 409. http://dx.doi.org/10.2307/3619618.

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30

Huang, Yukun, Miao Li, Junfeng Li, and Shengping Gong. "On the instability of Saturn’s hypothetical retrograde co-orbitals." Monthly Notices of the Royal Astronomical Society 488, no. 2 (July 24, 2019): 2543–48. http://dx.doi.org/10.1093/mnras/stz1840.

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ABSTRACT We find an interesting fact that fictitious retrograde co-orbitals of Saturn, or small bodies inside the retrograde 1:1 resonance with Saturn, are highly unstable in our numerical simulations. It is shown that, in the presence of Jupiter, the retrograde co-orbitals will get ejected from Saturn’s co-orbital space within a time-scale of 10 Myr. This scenario reminds us of the instability of Saturn Trojans caused by both the great inequality and the secular resonances. Therefore, we carry out in-depth inspections of both mechanisms and prove that the retrograde resonance overlap, raised by great inequality, cannot serve as an explanation for the instability of the retrograde co-orbitals, due to the weakness of the retrograde 2:5 resonance with Jupiter at low eccentricity. However, we discover that both ν5 and ν6 secular resonances contribute to the slow growth of the eccentricity and are therefore possibly the primary causes of the instability inside Saturn’s retrograde co-orbital space.

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31

Pascu, D., and R. E. Schmidt. "Photographic positional observations of Saturn." Astronomical Journal 99 (June 1990): 1974. http://dx.doi.org/10.1086/115480.

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32

Noll, K. S., T. R. Geballe, and R. F. Knacke. "Arsine in Saturn and Jupiter." Astrophysical Journal 338 (March 1989): L71. http://dx.doi.org/10.1086/185404.

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33

Bezard, B., P. Drossart, E. Lellouch, G. Tarrago, and J. P. Maillard. "Detection of arsine in Saturn." Astrophysical Journal 346 (November 1989): 509. http://dx.doi.org/10.1086/168032.

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34

Ward, William R., and Douglas P. Hamilton. "Tilting Saturn. I. Analytic Model." Astronomical Journal 128, no. 5 (November 2004): 2501–9. http://dx.doi.org/10.1086/424533.

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35

Hamilton, Douglas P., and William R. Ward. "Tilting Saturn. II. Numerical Model." Astronomical Journal 128, no. 5 (November 2004): 2510–17. http://dx.doi.org/10.1086/424534.

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36

Srama, R., and E. Grün. "The COSMIC DUST ANALYZER for the CASSINI Mission to Saturn." International Astronomical Union Colloquium 150 (1996): 227–31. http://dx.doi.org/10.1017/s0252921100501596.

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AbstractIn October 1997 a unique mission to the Saturnian system will be launched by NASA, the CASSINI mission. One goal of this mission is to study the Saturnian dust environment, and for this task, the COSMIC DUST ANALYZER (CDA) has been developed and is currently being tested. Impact ionization is used to determine the speed (1 - 100 km/s) and the mass (1•10–15 – 1•10–9 g) of impinging particles. Furthermore, the electric charge (1•10–15 – 1•10–12 C) of the particles can be measured via the induction principle, and an integrated time-of-flight mass spectrometer will analyze the chemical composition of individual dust particles. In order to achieve sufficient sensitivity for dust fluxes as low as 10 particles/(month-m2), the sensor has a large sensitive area of 0.1 m2. This paper will describe the function of the experiment.

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37

Pajevic, Paola, Jordan Spatz, Jenna Garr, Chris Adamson, and Lowell Misener. "Osteocyte biology and space flight." Current Biotechnology 2, no. 3 (September 1, 2013): 179–83. http://dx.doi.org/10.2174/22115501113029990017.

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38

Harris, Bernard A., Roger D. Billica, Sheryl L. Bishop, Tom Blackwell, Charles S. Layne, Deborah L. Harm, Gwenn R. Sandoz, and Edward C. Rosenow. "Physical Examination During Space Flight." Mayo Clinic Proceedings 72, no. 4 (April 1997): 301–8. http://dx.doi.org/10.4065/72.4.301.

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39

Pajevic, Paola Divieti, Jordan M. Spatz, Jenna Garr, Chris Adamson, and Lowell Misener. "Osteocyte biology and space flight." Current Biotechnology 999, no. 999 (August 1, 2013): 31–36. http://dx.doi.org/10.2174/22103031113039990017.

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40

Bova, Ben. "Space Flight: Manned Versus Unmanned." Science 233, no. 4764 (August 8, 1986): 610. http://dx.doi.org/10.1126/science.233.4764.610.b.

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41

Arnold, James R. "Space Flight: Manned Versus Unmanned." Science 233, no. 4764 (August 8, 1986): 610. http://dx.doi.org/10.1126/science.233.4764.610.a.

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42

Laub, J. H. "Space Flight: Manned Versus Unmanned." Science 233, no. 4764 (August 8, 1986): 610. http://dx.doi.org/10.1126/science.233.4764.610.c.

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43

Bacal, Kira, Roger Billica, and Sheryl Bishop. "Neurovestibular symptoms following space flight." Journal of Vestibular Research 13, no. 2-3 (October 1, 2003): 93–102. http://dx.doi.org/10.3233/ves-2003-132-304.

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Neurovestibular symptoms experienced by astronauts in the post-flight period were examined using data from medical debriefs contained in the NASA Longitudinal Study of Astronaut Health database. Ten symptoms were identified (clumsiness, difficulty concentrating, persisting sensation aftereffects, nausea, vomiting, vertigo while walking, vertigo while standing, difficulty walking a straight line, blurred vision, and dry heaves), of which eight were crossed with twelve demographic parameters (mission duration, astronaut gender, age, one-g piloting experience, previous space flight experience, g-suit inflation, g-suit deflation, in-flight space motion sickness, in-flight exercise, post-flight exercise, mission role, fluid loading). Three symptoms were experienced by a majority of subjects, and another two by more than a quarter of the subjects. Intensity of the symptoms was mild, suggesting that they are unlikely to pose a risk to the crew during landing and the post-flight period. Seven of the symptoms and eight of the parameters under study were found to be significantly associated with each other.

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44

Watt, Douglas, and Luc Lefebvre. "Vestibular suppression during space flight." Journal of Vestibular Research 13, no. 4-6 (December 28, 2003): 363–76. http://dx.doi.org/10.3233/ves-2003-134-619.

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Normal movements performed while voluntarily fixing the head to the torso can lead to motion sickness in susceptible individuals. The underlying mechanism may involve excessive suppression of vestibular responses. A similar motor strategy is often adopted in the early days of a space flight and might contribute to the development of space motion sickness. In a recent experiment, we monitored the eye, head and upper torso rotations of four Life and Microgravity Spacelab crew members. For the purposes of this study, all data were excluded except for periods during which the subject was performing pure yaw-axis head movements. All subjects showed a significant increase in gaze slip on the first day of their mission, suggesting that increased vestibular suppression was occurring. Furthermore, this amount of increased suppression would have been more than adequate to produce motion sickness in susceptible individuals on the ground. The results support the theory of two, independent mechanisms for space motion sickness.

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45

Sonnenfeld, G. "Immune Responses in Space Flight." International Journal of Sports Medicine 19, S 3 (July 1998): S195—S204. http://dx.doi.org/10.1055/s-2007-971992.

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46

Pierson, Duane L., Monjula Chidambaram, Joe Don Heath, Laura Mallary, Saroj K. Mishra, Baldev Sharma, and George M. Weinstock. "Epidemiology ofStaphylococcus aureusduring space flight." FEMS Immunology & Medical Microbiology 16, no. 3-4 (December 1996): 273–81. http://dx.doi.org/10.1111/j.1574-695x.1996.tb00146.x.

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47

Lee, Andrew G., William J. Tarver, Thomas H. Mader, Charles Robert Gibson, Stephen F. Hart, and Christian A. Otto. "Neuro-Ophthalmology of Space Flight." Journal of Neuro-Ophthalmology 36, no. 1 (March 2016): 85–91. http://dx.doi.org/10.1097/wno.0000000000000334.

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48

Phillips, K. "TACKLING SPACE FLIGHT BONE LOSS." Journal of Experimental Biology 211, no. 7 (April 1, 2008): i. http://dx.doi.org/10.1242/jeb.018127.

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49

Berdahl, John, David Fleischman, R. Rand Allingham, and Mike Fautsch. "Disc Swelling and Space Flight." Ophthalmology 119, no. 6 (June 2012): 1290. http://dx.doi.org/10.1016/j.ophtha.2012.02.024.

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50

Kim, Dae Hee, and Cameron F. Parsa. "Space Flight and Disc Edema." Ophthalmology 119, no. 11 (November 2012): 2420–21. http://dx.doi.org/10.1016/j.ophtha.2012.07.016.

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