Tham khảo Lõi_hành_tinh

  1. ↑ Solomon, S.C. (2007). “Hot News on Mercury's core”. Science. 316 (5825): 702–3. doi:10.1126/science.1142328. PMID 17478710.
  2. ↑ Williams, Jean-Pierre; Nimmo, Francis (2004). “Thermal evolution of the Martian core: Implications for an early dynamo”. Geology. 32 (2): 97–100. Bibcode:2004Geo....32...97W. doi:10.1130/g19975.1.
  3. ↑ Pollack, James B.; Grossman, Allen S.; Moore, Ronald; Graboske, Harold C. Jr. (1977). “A Calculation of Saturn's Gravitational Contraction History”. Icarus. Academic Press, Inc. 30: 111–128. Bibcode:1977Icar...30..111P. doi:10.1016/0019-1035(77)90126-9.
  4. ↑ Fortney, Jonathan J.; Hubbard, William B. (2003). “Phase separation in giant planets: inhomogeneous evolution of Saturn”. Icarus. Academic Press. 164: 228–243. arXiv:astro-ph/0305031. Bibcode:2003Icar..164..228F. doi:10.1016/s0019-1035(03)00130-1.
  5. ↑ Stevenson, D. J. (1982). “Formation of the Giant Planets”. Planet. Space Sci. Pergamon Press Ltd. 30 (8): 755–764. Bibcode:1982P&SS...30..755S. doi:10.1016/0032-0633(82)90108-8.
  6. ↑ Sato, Bun'ei; al., et (tháng 11 năm 2005). “The N2K Consortium. II. A Transiting Hot Saturn around HD 149026 with a Large Dense Core”. The Astrophysical Journal. The American Astronomical Society. 633: 465–473. arXiv:astro-ph/0507009. Bibcode:2005ApJ...633..465S. doi:10.1086/449306.
  7. 1 2 NASA (2012). “MESSENGER Provides New Look at Mercury's Surprising Core and Landscape Curiosities”. News Releases. The Woodlands, Texas: NASA: 1–2.