Rujukan Bulan_(satelit)

Nota

  1. ↑ The maximum value is given based on scaling of the brightness from the value of −12.74 given for an equator to Moon-centre distance of 378 000 km in the NASA factsheet reference to the minimum Earth–Moon distance given there, after the latter is corrected for the Earth's equatorial radius of 6 378 km, giving 350 600 km. The minimum value (for a distant new Moon) is based on a similar scaling using the maximum Earth–Moon distance of 407 000 km (given in the factsheet) and by calculating the brightness of the earthshine onto such a new Moon. The brightness of the earthshine is [ Earth albedo × (Earth radius / Radius of Moon's orbit)2 ] relative to the direct solar illumination that occurs for a full Moon. (Earth albedo = 0.367; Earth radius = (polar radius × equatorial radius)½ = 6 367 km.)
  2. ↑ The range of angular size values given are based on simple scaling of the following values given in the fact sheet reference: at an Earth-equator to Moon-centre distance of 378 000 km, the angular size is 1896 arcseconds. The same fact sheet gives extreme Earth–Moon distances of 407 000 km and 357 000 km. For the maximum angular size, the minimum distance has to be corrected for the Earth's equatorial radius of 6 378 km, giving 350 600 km.

Petikan

  1. 1 2 3 4 5 6 7 8 9 10 11 12 Wieczorek, M.; dll. (2006). "The constitution and structure of the lunar interior". Reviews in Mineralogy and Geochemistry. 60 (1): 221–364. doi:10.2138/rmg.2006.60.3. 
  2. 1 2 Lang, Kenneth R. (2011); The Cambridge Guide to the Solar System, 2nd ed., Cambridge University Press
  3. 1 2 3 4 5 Williams, Dr. David R. (2 February 2006). "Moon Fact Sheet". NASA (National Space Science Data Center). 
  4. ↑ Matthews, Grant (2008). "Celestial body irradiance determination from an underfilled satellite radiometer: application to albedo and thermal emission measurements of the Moon using CERES". Applied Optics. 47 (27): 4981–93. Bibcode:2008ApOpt..47.4981M. doi:10.1364/AO.47.004981. PMID 18806861. 
  5. ↑ A.R. Vasavada, D.A. Paige, and S.E. Wood (1999). "Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits". Icarus. 141 (2): 179. Bibcode:1999Icar..141..179V. doi:10.1006/icar.1999.6175.  Parameter |yesr= tidak diketahui diabaikan (bantuan)Selenggaraan CS1: Pelbagai nama: senarai pengarang (link)
  6. ↑ http://lasp.colorado.edu/life/GEOL5835/Moon_presentation_19Sept.pdf
  7. ↑ Taylor, Stuart Ross (1975). Lunar science: A post-Apollo view. New York, Pergamon Press, Inc. m/s. 64. 
  8. ↑ "NASA Research Team Reveals Moon Has Earth-Like Core". NASA. 01.06.11.  Check date values in: |date= (bantuan)
  9. ↑ Nemchin, A.; Timms, N.; Pidgeon, R.; Geisler, T.; Reddy, S.; Meyer, C. (2009). "Timing of crystallization of the lunar magma ocean constrained by the oldest zircon". Nature Geoscience. 2 (2): 133–136. Bibcode:2009NatGe...2..133N. doi:10.1038/ngeo417. 
  10. ↑ Shearer, C.; dll. (2006). "Thermal and magmatic evolution of the Moon". Reviews in Mineralogy and Geochemistry. 60 (1): 365–518. doi:10.2138/rmg.2006.60.4. 
  11. ↑ Lucey, P.; Korotev, Randy L.; dll. (2006). "Understanding the lunar surface and space-Moon interactions". Reviews in Mineralogy and Geochemistry. 60 (1): 83–219. doi:10.2138/rmg.2006.60.2. 
  12. ↑ Schubert, J. (2004). "Interior composition, structure, and dynamics of the Galilean satellites.". dalam F. Bagenal; dll. Jupiter: The Planet, Satellites, and Magnetosphere. Cambridge University Press. m/s. 281–306. ISBN 978-0-521-81808-7. Selenggaraan CS1: Penggunaan eksplisit et al. (link) Selenggaraan CS1: display-para pengarang (link)
  13. ↑ Williams, J.G. (2006). "Lunar laser ranging science: Gravitational physics and lunar interior and geodesy". Advances in Space Research. 37 (1): 6771. arXiv:gr-qc/0412049 . Bibcode:2006AdSpR..37...67W. doi:10.1016/j.asr.2005.05.013.  Parameter |coauthors= tidak diketahui diabaikan (guna |author=) (bantuan)
  14. ↑ "Landscapes from the ancient and eroded lunar far side". esa. Dicapai 15 February 2010. 
  15. ↑ Spudis, Paul D.; Cook, A.; Robinson, M.; Bussey, B.; Fessler, B.; Cook; Robinson; Bussey; Fessler (01/1998). "Topography of the South Polar Region from Clementine Stereo Imaging". Workshop on New Views of the Moon: Integrated Remotely Sensed, Geophysical, and Sample Datasets: 69. Bibcode:1998nvmi.conf...69S.  Check date values in: |date= (bantuan)Selenggaraan CS1: Pelbagai nama: senarai pengarang (link)
  16. 1 2 3
  17. ↑ Pieters, C.M.; Tompkins, S.; Head, J.W.; Hess, P.C. (1997). "Mineralogy of the Mafic Anomaly in the South Pole‐Aitken Basin: Implications for excavation of the lunar mantle". Geophysical Research Letters. 24 (15): 1903–1906. Bibcode:1997GeoRL..24.1903P. doi:10.1029/97GL01718. 
  18. ↑ Taylor, G.J. (17 July 1998). "The Biggest Hole in the Solar System". Planetary Science Research Discoveries, Hawai'i Institute of Geophysics and Planetology. Dicapai 12 April 2007. 
  19. ↑ Schultz, P. H. (03/1997). "Forming the south-pole Aitken basin – The extreme games". Conference Paper, 28th Annual Lunar and Planetary Science Conference. 28: 1259. Bibcode:1997LPI....28.1259S.  Check date values in: |date= (bantuan)
  20. ↑ Phillips, Tony (12 March 2007). "Stereo Eclipse". Science@NASA. Dicapai 17 March 2010. 
  21. ↑ Espenak, F. (2000). "Solar Eclipses for Beginners". MrEclipse. Dicapai 17 March 2010. 
  22. ↑
  23. ↑

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