2641:
507:
liquid layer around an inner solid core. As the orbital radius of a rocky planet increases, the size of the core relative to the total radius of the planet decreases. This is believed to be because differentiation of the core is directly related to a body's initial heat, so
Mercury's core is relatively large and active. Venus and Mars, as well as the moon, do not have magnetic fields. This could be due to a lack of a convecting liquid layer interacting with a solid inner core, as Venus’ core is not layered. Although Mars does have a liquid and solid layer, they do not appear to be interacting in the same way that Earth's liquid and solid components interact to produce a dynamo.
34:
167:. The moment of inertia for a differentiated planet is less than 0.4, because the density of the planet is concentrated in the center. Mercury has a moment of inertia of 0.346, which is evidence for a core. Conservation of energy calculations as well as magnetic field measurements can also constrain composition, and surface geology of the planets can characterize differentiation of the body since its accretion. Mercury, Venus, and Mars’ cores are about 75%, 50%, and 40% of their radius respectively.
2653:
2713:
42:
766:. Metallic hydrogen is present within the core (in lower abundances than Jupiter). Saturn has a rock and or ice core 10–30 times the mass of the Earth, and this core is likely soluble in the gas envelope above, and therefore it is primordial in composition. Since the core still exists, the envelope must have originally accreted onto previously existing planetary cores. Thermal contraction/evolution models support the presence of
516:
major area of contention because it is difficult to produce in laboratory settings, due to the high pressures needed. Jupiter and Saturn appear to release a lot more energy than they should be radiating just from the sun, which is attributed to heat released by the hydrogen and helium layer. Uranus does not appear to have a significant heat source, but
Neptune has a heat source that is attributed to a “hot” formation.
2701:
2665:
2689:
538:
early in the Solar System's history. Mercury has a solid silicate crust and mantle overlying a solid metallic outer core layer, followed by a deeper liquid core layer, and then a possible solid inner core making a third layer. The composition of the iron-rich core remains uncertain, but it likely contains nickel, silicon and perhaps sulfur and carbon, plus trace amounts of other elements.
2677:
122:, Wiechert in 1898 postulated that the Earth had a similar bulk composition to iron meteorites, but the iron had settled to the interior of the Earth, and later represented this by integrating the bulk density of the Earth with the missing iron and nickel as a core. The first detection of Earth's core occurred in 1906 by Richard Dixon Oldham upon discovery of the
782:
will provide more insight to planetary core formation. It was previously understood that collisions in the solar system fully merged, but recent work on planetary bodies argues that remnants of collisions have their outer layers stripped, leaving behind a body that would eventually become a planetary
369:
thus make up the remaining mass deficit of Earth's core; though the abundances of each are still a matter of controversy revolving largely around the pressure and oxidation state of Earth's core during its formation. No geochemical evidence exists to include any radioactive elements in Earth's core.
719:
than the mantle (agreeing with the differentiation history of the planet, as well as the impact hypothesis), and with a liquid core potassium-40 would have had opportunity to partition into the core providing an additional source of heat. The model further concludes that the core of mars is entirely
506:
All of the rocky inner planets, as well as the moon, have an iron-dominant core. Venus and Mars have an additional major element in the core. Venus’ core is believed to be iron-nickel, similarly to Earth. Mars, on the other hand, is believed to have an iron-sulfur core and is separated into an outer
537:
Mercury has an observed magnetic field, which is believed to be generated within its metallic core. Mercury's core occupies 85% of the planet's radius, making it the largest core relative to the size of the planet in the Solar System; this indicates that much of
Mercury's surface may have been lost
162:
that flew by
Mercury and Venus to observe their surface characteristics. The cores of other planets cannot be measured using seismometers on their surface, so instead they have to be inferred based on calculations from these fly-by observation. Mass and size can provide a first-order calculation of
445:
of the inner core (which can occur as a result of temperature). Examples of compositional buoyancy include precipitation of iron alloys onto the inner core and liquid immiscibility both, which could influence convection both positively and negatively depending on ambient temperatures and pressures
799:
As the field of exoplanets grows as new techniques allow for the discovery of both diverse exoplanets, the cores of exoplanets are being modeled. These depend on initial compositions of the exoplanets, which is inferred using the absorption spectra of individual exoplanets in combination with the
686:
could have provided an important source of heat contributing to the early Earth's dynamo, though to a lesser extent than on sulfur rich Mars. The core contains half the Earth's vanadium and chromium, and may contain considerable niobium and tantalum. The core is depleted in germanium and gallium.
515:
Current understanding of the outer planets in the solar system, the ice and gas giants, theorizes small cores of rock surrounded by a layer of ice, and in
Jupiter and Saturn models suggest a large region of liquid metallic hydrogen and helium. The properties of these metallic hydrogen layers is a
710:
Core merging between proto-Mars and another differentiated planetoid could have been as fast as 1000 years or as slow as 300,000 years (depending on the viscosity of both cores and mantles). Impact-heating of the
Martian core would have resulted in stratification of the core and kill the Martian
320:
at very low concentration. This leaves Earth's core with a 5–10% weight deficit for the outer core, and a 4–5% weight deficit for the inner core; which is attributed to lighter elements that should be cosmically abundant and are iron-soluble; H, O, C, S, P, and Si. Earth's core contains half the
746:
Jupiter has a rock and/or ice core 10–30 times the mass of the Earth, and this core is likely soluble in the gas envelope above, and so primordial in composition. Since the core still exists, the outer envelope must have originally accreted onto a previously existing planetary core. Thermal
246:
material. The observed Hf/W ratios in iron meteorites constrain metal segregation to under 5 million years, the Earth's mantle Hf/W ratio places Earth's core as having segregated within 25 million years. Several factors control segregation of a metal core including the crystallization of
827:. The first such planet discovered was 18 times the density of water, and five times the size of Earth. Thus the planet cannot be gaseous, and must be composed of heavier elements that are also cosmically abundant like carbon and oxygen; making it likely crystalline like a diamond.
480:
Small planetary cores may experience catastrophic energy release associated with phase changes within their cores. Ramsey (1950) found that the total energy released by such a phase change would be on the order of 10 joules; equivalent to the total energy release due to
393:(Hf/W) isotopic ratios, when compared with a chondritic reference frame, show a marked enrichment in the silicate earth indicating depletion in Earth's core. Iron meteorites, believed to be resultant from very early core fractionation processes, are also depleted.
93:
Planetary cores are challenging to study because they are impossible to reach by drill and there are almost no samples that are definitively from the core. Thus, they are studied via indirect techniques such as seismology, mineral physics, and planetary dynamics.
677:
meteorites. Sulfur, carbon, and phosphorus only account for ~2.5% of the light element component/mass deficit. No geochemical evidence exists for including any radioactive elements in the core. However, experimental evidence has found that potassium is strongly
467:
of crystallization. All planetary bodies have a primordial heat value, or the amount of energy from accretion. Cooling from this initial temperature is called secular cooling, and in the Earth the secular cooling of the core transfers heat into an insulating
454:
A planetary core acts as a heat source for the outer layers of a planet. In the Earth, the heat flux over the core mantle boundary is 12 terawatts. This value is calculated from a variety of factors: secular cooling, differentiation of light elements,
436:
for further details. A dynamo requires a source of thermal and/or compositional buoyancy as a driving force. Thermal buoyancy from a cooling core alone cannot drive the necessary convection as indicated by modelling, thus compositional buoyancy (from
1338:
Bussey, Ben; Gillis, Jeffrey J.; Peterson, Chris; Hawke, B. Ray; Tompkins, Stephanie; McCallum, I. Stewart; Shearer, Charles K.; Neal, Clive R.; Righter, Kevin (2006-01-01). "The
Constitution and Structure of the Lunar Interior".
360:
may be present up to 0.2 weight %. Hydrogen and carbon, however, are highly volatile and thus would have been lost during early accretion and therefore can only account for 0.1 to 0.2 weight % respectively.
117:
calculated the average density of the Earth to be 5.48 times the density of water (later refined to 5.53), which led to the accepted belief that the Earth was much denser in its interior. Following the discovery of
720:
liquid, as the latent heat of crystallization would have driven a longer-lasting (greater than one billion years) dynamo. If the core of Mars is liquid, the lower bound for sulfur would be five weight %.
650:
is still debated; however, if it does have a core it would have formed synchronously with the Earth's own core at 45 million years post-start of the Solar System based on hafnium-tungsten evidence and the
432:
is a proposed mechanism to explain how celestial bodies like the Earth generate magnetic fields. The presence or lack of a magnetic field can help constrain the dynamics of a planetary core. Refer to
673:
generated within its metallic core. The Earth has a 5–10% mass deficit for the entire core and a density deficit from 4–5% for the inner core. The Fe/Ni value of the core is well constrained by
2271:
Nittler, Larry R.; Chabot, Nancy L.; Grove, Timothy L.; Peplowski, Patrick N. (2018). "The
Chemical Composition of Mercury". In Solomon, Sean C.; Nittler, Larry R.; Anderson, Brian J. (eds.).
2375:
Munker, Carsten; Pfander, Jorg A; Weyer, Stefan; Buchl, Anette; Kleine, Thorsten; Mezger, Klaus (July 2003). "Evolution of
Planetary Cores and the Earth-Moon System from Nb/Ta Systematics".
2485:
Lord, Peter; Tilley, Scott; Oh, David Y.; Goebel, Dan; Polanskey, Carol; Snyder, Steve; Carr, Greg; Collins, Steven M.; Lantoine, Gregory (March 2017). "Psyche: Journey to a metal world".
812:
results when a gas giant has its outer atmosphere stripped away by its parent star, likely due to the planet's inward migration. All that remains from the encounter is the original core.
703:
Mars possibly hosted a core-generated magnetic field in the past. The dynamo ceased within 0.5 billion years of the planet's formation. Hf/W isotopes derived from the martian meteorite
2526:
1555:
Margot, Jean-Luc; Peale, Stanton J.; Solomon, Sean C.; Hauck, Steven A.; Ghigo, Frank D.; Jurgens, Raymond F.; Yseboodt, Marie; Giorgini, Jon D.; Padovan, Sebastiano (December 2012).
493:. Such phase changes would only occur at specific mass to volume ratios, and an example of such a phase change would be the rapid formation or dissolution of a solid core component.
126:
shadow zone; the liquid outer core. By 1936 seismologists had determined the size of the overall core as well as the boundary between the fluid outer core and the solid inner core.
707:, indicate rapid accretion and core differentiation of Mars; i.e. under 10 million years. Potassium-40 could have been a major source of heat powering the early Martian dynamo.
833:
is a 5.7 millisecond pulsar found to have a companion with a mass similar to
Jupiter but a density of 23 g/cm, suggesting that the companion is an ultralow mass carbon
1295:
Nakamura, Yosio; Latham, Gary; Lammlein, David; Ewing, Maurice; Duennebier, Frederick; Dorman, James (July 1974). "Deep lunar interior inferred from recent seismic data".
356:
is strongly siderophilic and only moderately volatile and depleted in the silicate earth; thus may account for 1.9 weight % of Earth's core. By similar arguments,
195:
Jupiter and Saturn most likely formed around previously existing rocky and/or icy bodies, rendering these previous primordial planets into gas-giant cores. This is the
283:
and the early Earth formed the modern Earth and Moon. During this impact the majority of the iron from Theia and the Earth became incorporated into the Earth's core.
374:
to be strongly siderophilic at the temperatures associated with core formation, thus there is potential for potassium in planetary cores of planets, and therefore
146:. The Moon's core has a radius of 300 km. The Moon's iron core has a liquid outer layer that makes up 60% of the volume of the core, with a solid inner core.
2014:
Murthy, V. Rama; van Westrenen, Wim; Fei, Yingwei (2003). "Experimental evidence that potassium is a substantial radioactive heat source in planetary cores".
79:. Gas giant cores are proportionally much smaller than those of terrestrial planets, though they can be considerably larger than the Earth's nevertheless;
75:
also have cores, though the composition of these are still a matter of debate and range in possible composition from traditional stony/iron, to ice or to
291:
Core merging between the proto-Mars and another differentiated planetoid could have been as fast as 1000 years or as slow as 300,000 years (depending on
163:
the components that make up the interior of a planetary body. The structure of rocky planets is constrained by the average density of a planet and its
979:
Pollack, James B.; Grossman, Allen S.; Moore, Ronald; Graboske, Harold C. Jr. (1977). "A Calculation of Saturn's Gravitational Contraction History".
267:
Impacts between planet-sized bodies in the early Solar System are important aspects in the formation and growth of planets and planetary cores.
2534:
845:
Exoplanets with moderate densities (more dense than Jovian planets, but less dense than terrestrial planets) suggests that such planets like
316:, the unknown component, the composition of the inner and outer core, can be determined: 85% Fe, 5% Ni, 0.9% Cr, 0.25% Co, and all other
416:
of an early planetesimal, although a recent hypothesis suggests that they are impact-generated mixtures of core and mantle materials.
1111:
Sato, Bun'ei; al., et (November 2005). "The N2K Consortium. II. A Transiting Hot Saturn around HD 149026 with a Large Dense Core".
704:
401:(Nb/Ta) isotopic ratios, when compared with a chondritic reference frame, show mild depletion in bulk silicate Earth and the moon.
850:
446:
associated with the host-body. Other celestial bodies that exhibit magnetic fields are Mercury, Jupiter, Ganymede, and Saturn.
210:
is broadly defined as the development from one thing to many things; homogeneous body to several heterogeneous components. The
2609:
2080:
Hauck, S. A.; Van Orman, J. A. (2011). "Core petrology: Implications for the dynamics and evolution of planetary interiors".
711:
dynamo for a duration between 150 and 200 million years. Modelling done by Williams, et al. 2004 suggests that in order for
1014:
Fortney, Jonathan J.; Hubbard, William B. (2003). "Phase separation in giant planets: inhomogeneous evolution of Saturn".
743:, indicating some metallic substance is present. Its magnetic field is the strongest in the Solar System after the Sun's.
923:
Williams, Jean-Pierre; Nimmo, Francis (2004). "Thermal evolution of the Martian core: Implications for an early dynamo".
242:
reservoirs develop positive Hf/W anomalies, and metal reservoirs acquire negative anomalies relative to undifferentiated
1772:
Wood, Bernard J.; Walter, Michael J.; Jonathan, Wade (June 2006). "Accretion of the Earth and segregation of its core".
1456:, National Aeronautics and Space Administration, Jet Propulsion Laboratory, California Institute of Technology, 1987,
2502:
2359:
2306:
2140:
1675:
2548:
Bailes, M.; et al. (September 2011). "Transformation of a Star into a Planet in a Millisecond Pulsar Binary".
2640:
2738:
1531:
647:
135:
76:
1920:
1203:
Nachrichten der Königlichen Gesellschaft der Wissenschaften zu Göttingen, Mathematische-physikalische Klasse
57:. Cores may be entirely liquid, or a mixture of solid and liquid layers as is the case in the Earth. In the
472:
mantle. As the inner core grows, the latent heat of crystallization adds to the heat flux into the mantle.
853:
are composed of primarily water. Internal pressures of such water-worlds would result in exotic phases of
280:
550:' core varies significantly depending on the model used to calculate it, thus constraints are required.
2733:
2631:
1479:
Solomon, Sean C. (June 1979). "Formation, history and energetics of cores in the terrestrial planets".
2426:
Williams, Quentin; Agnor, Craig B.; Asphaug, Erik (January 2006). "Hit-and-run planetary collisions".
2275:. Cambridge Planetary Science Book Series. Cambridge, UK: Cambridge University Press. pp. 30–51.
238:. Thus if metal segregation (between the Earth's core and mantle) occurred in under 45 million years,
688:
433:
207:
1900:
1281:
664:
20:
2256:
NASA (2012). "MESSENGER Provides New Look at Mercury's Surprising Core and Landscape Curiosities".
196:
181:
164:
27:
524:
The following summarizes known information about the planetary cores of given non-stellar bodies.
259:
process and may drive the production and extraction of iron metal from an original silicate melt.
652:
276:
192:(10 – 10 years) and these develop into planetary bodies over an additional 10–100 million years.
139:
1198:
2106:
Edward R. D. Scott, "Impact Origins for Pallasites," Lunar and Planetary Science XXXVIII, 2007.
1844:
Halliday; N., Alex (February 2000). "Terrestrial accretion rates and the origin of the Moon".
1887:
1268:
1857:
1823:
1089:
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2339:
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2209:
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2023:
1935:
1853:
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1705:
1605:
1568:
1488:
1403:
1348:
1304:
1130:
1085:
1033:
988:
932:
679:
413:
188:
around 10 km in diameter. From here gravity takes over to produce Moon to Mars-sized
8:
2705:
1260:
235:
2571:
2439:
2388:
2343:
2290:
2213:
2172:
2093:
2027:
1939:
1921:"Consequences of giant impacts in early Mars: Core merging and Martian Dynamo evolution"
1785:
1709:
1609:
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1407:
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1037:
992:
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2408:
2312:
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1951:
1805:
1737:
1631:
1435:
1372:
1241:
1146:
1120:
1049:
1023:
948:
898:
824:
227:
155:
1865:
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1237:
1045:
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2459:
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2400:
2355:
2351:
2316:
2302:
2235:
2227:
2136:
2039:
1797:
1729:
1721:
1671:
1635:
1617:
1557:"Mercury's moment of inertia from spin and gravity data: MERCURY'S MOMENT OF INERTIA"
1537:
1527:
1504:
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1457:
1439:
1427:
1419:
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1364:
1320:
1245:
1150:
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1000:
902:
890:
767:
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of 9 million years, and is approximated as an extinct system after 45 million years.
2512:
1955:
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740:
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2490:
2471:
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2392:
2347:
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2128:
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1943:
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1809:
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1713:
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1621:
1613:
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1411:
1390:
Weber, R. C.; Lin, P.-Y.; Garnero, E. J.; Williams, Q.; Lognonne, P. (2011-01-21).
1356:
1312:
1233:
1177:
1138:
1093:
1041:
996:
940:
882:
809:
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to have had a functional dynamo, the Martian core was initially hotter by 150
695:
of Earth's history. Inner core crystallization timing is still largely unresolved.
438:
317:
313:
189:
66:
2613:
2412:
763:
1667:
728:
442:
309:
114:
108:
33:
2717:
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830:
784:
670:
456:
158:
were initially characterized by analyzing data from spacecraft, such as NASA's
119:
2494:
2298:
2222:
2197:
2181:
2156:
2727:
2455:
2231:
1725:
1596:
Solomon, Sean C. (August 1976). "Some aspects of core formation in Mercury".
1541:
1508:
1423:
1368:
1324:
820:
779:
490:
486:
429:
308:
Using the chondritic reference model and combining known compositions of the
2579:
2396:
1626:
1461:
1415:
1316:
886:
655:. Such a core may have hosted a geomagnetic dynamo early on in its history.
2681:
2587:
2463:
2404:
2239:
2043:
1801:
1733:
1431:
1222:"The Constitution of the Interior of the Earth, as Revealed by Earthquakes"
1182:
1165:
894:
683:
375:
215:
185:
58:
1360:
1947:
1581:
1556:
1125:
1028:
834:
815:
464:
252:
211:
2447:
2035:
1793:
682:
when dealing with temperatures associated with core-accretion, and thus
674:
482:
357:
248:
159:
143:
87:
72:
2712:
41:
2009:
2007:
2005:
1994:
McDonough, W. F. (2003). "Compositional Model for the Earth's Core".
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944:
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409:
371:
338:
292:
256:
243:
219:
84:
1391:
1221:
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1142:
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within the core in large abundances (but still less than Jupiter).
731:
has an observed magnetic field generated within its metallic core.
469:
398:
390:
334:
326:
322:
239:
231:
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2002:
1914:
1912:
1910:
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1757:
1755:
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846:
394:
386:
362:
342:
330:
223:
180:
Planetary systems form from flattened disks of dust and gas that
80:
2519:
1879:
1998:. Maryland: University of Maryland Geology Department: 547–568.
759:
716:
692:
366:
353:
123:
54:
1907:
1748:
1696:
Stevenson, David J. (2001-07-12). "Mars' core and magnetism".
279:
states that an impact between a theoretical Mars-sized planet
138:
was characterized in 1974 using seismic data collected by the
854:
547:
978:
823:, previously stars, are formed alongside the formation of a
2270:
2075:
2073:
2071:
2069:
2067:
2065:
2063:
2061:
1294:
1076:
Stevenson, D. J. (1982). "Formation of the Giant Planets".
787:, titled “Journey to a Metal World,” is aiming to studying
751:
within the core in large abundances (greater than Saturn).
712:
62:
2676:
303:
2533:. National Geographic Society. 2011-08-25. Archived from
1454:
Mariner 10 mission highlights : Venus mosaic P-14461
1337:
1170:
Philosophical Transactions of the Royal Society of London
918:
916:
914:
912:
2058:
1201:[About the mass distribution inside the Earth].
2602:
2374:
1919:
Monteaux, Julien; Arkani-Hamed, Jafar (November 2013).
1839:
1837:
1554:
1389:
1007:
2013:
1259:
Transdyne Corporation (2009). J. Marvin Hemdon (ed.).
974:
972:
970:
968:
966:
964:
962:
909:
816:
Planets derived from stellar cores and diamond planets
2629:
1662:(2 ed.). Cambridge: Cambridge University Press.
1258:
1252:
747:
contraction/evolution models support the presence of
441:) is required. On Earth the buoyancy is derived from
2425:
1918:
1834:
1816:
873:
Solomon, S.C. (2007). "Hot News on Mercury's core".
348:
2541:
2368:
2198:"Physicists doubt bold report of metallic hydrogen"
1872:
1521:
1261:"Richard D. Oldham's Discovery of the Earth's Core"
959:
2484:
1989:
1987:
1985:
1771:
2161:Monthly Notices of the Royal Astronomical Society
1983:
1981:
1979:
1977:
1975:
1973:
1971:
1969:
1967:
1965:
791:that could possibly be a remnant planetary core.
739:Jupiter has an observed magnetic field generated
90:may have a core 100 times the mass of the Earth.
2725:
1104:
1071:
1069:
1067:
1065:
1063:
1199:"Uber die Massenverteilung im Inneren der Erde"
1166:"Experiments to determine the density of Earth"
857:forming on the surface and within their cores.
381:
2527:""Diamond" Planet Found; May be Stripped Star"
2079:
1962:
1013:
370:Despite this, experimental evidence has found
2157:"On the Instability of Small Planetary Cores"
1655:
1157:
1060:
922:
496:
149:
2612:. MessageToEagle. 2012-04-09. Archived from
2251:
2249:
2195:
2123:Nimmo, F. (2015), "Energetics of the Core",
1481:Physics of the Earth and Planetary Interiors
1190:
475:
251:. Crystallization of perovskite in an early
45:The internal structure of the outer planets.
37:The internal structure of the inner planets.
2323:
2148:
1226:Quarterly Journal of the Geological Society
510:
262:
1843:
1656:Pater, Imke de; Lissauer, Jack J. (2015).
1213:
866:
773:
527:
83:'s is 10–30 times heavier than Earth, and
26:For core body of planetary formation, see
2561:
2280:
2246:
2221:
2180:
1993:
1695:
1625:
1580:
1181:
1163:
1124:
1075:
1027:
762:has an observed magnetic field generated
184:rapidly (within thousands of years) into
2088:. American Geophysical Union: DI41B–03.
1928:Journal of Geophysical Research: Planets
1880:"A new Model for the Origin of the Moon"
1561:Journal of Geophysical Research: Planets
1196:
40:
32:
1595:
1478:
1110:
872:
404:
304:Determining primary composition – Earth
61:, core sizes range from about 20% (the
2726:
2547:
2329:
2154:
1341:Reviews in Mineralogy and Geochemistry
1219:
837:, likely the core of an ancient star.
501:
53:consists of the innermost layers of a
2122:
2118:
2116:
2114:
2112:
1691:
1689:
1687:
1651:
1649:
1647:
1645:
1474:
1472:
1470:
1392:"Seismic Detection of the Lunar Core"
2255:
803:
270:
2196:Castelvecchi, Davide (2017-01-26).
1996:Geochemistry of the Mantle and Core
1846:Earth and Planetary Science Letters
1084:(8). Pergamon Press Ltd.: 755–764.
987:(1). Academic Press, Inc: 111–128.
449:
13:
2260:. The Woodlands, Texas: NASA: 1–2.
2133:10.1016/b978-0-444-53802-4.00139-1
2109:
1684:
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1467:
840:
665:Structure of the Earth § Core
489:. Such an event could explain the
202:
21:Structure of the Earth § Core
14:
2750:
2273:Mercury: The View after MESSENGER
1238:10.1144/GSL.JGS.1906.062.01-04.21
1220:Oldham, R. D. (1 February 1906).
519:
349:Weight deficit components – Earth
2711:
2699:
2687:
2675:
2663:
2651:
2639:
2330:Fegley, B. Jr. (2003). "Venus".
800:emission spectra of their star.
2478:
2419:
2264:
2189:
2100:
1589:
1548:
1515:
1446:
1383:
1331:
1288:
562:Equilibrium Condensation Model
329:, and may contain considerable
102:
65:) to 85% of a planet's radius (
2487:2017 IEEE Aerospace Conference
2352:10.1016/b0-08-043751-6/01150-6
1934:(3). AGU Publications: 84–87.
337:. Earth's core is depleted in
136:internal structure of the Moon
129:
16:Innermost layer(s) of a planet
1:
1866:10.1016/s0012-821x(99)00317-9
1046:10.1016/s0019-1035(03)00130-1
860:
794:
2127:, Elsevier, pp. 27–55,
1668:10.1017/cbo9781316165270.023
1618:10.1016/0019-1035(76)90124-X
1522:Hubbard, William B. (1992).
1501:10.1016/0031-9201(79)90081-5
1297:Geophysical Research Letters
1098:10.1016/0032-0633(82)90108-8
1001:10.1016/0019-1035(77)90126-9
382:Isotopic composition – Earth
298:
175:
170:
97:
7:
2155:Ramsey, W.H. (April 1950).
723:
689:Core mantle differentiation
419:
412:are thought to form at the
199:model of planet formation.
10:
2755:
2082:AGU Fall Meeting Abstracts
778:Missions to bodies in the
734:
669:The Earth has an observed
662:
532:
497:Trends in the Solar System
150:Cores of the rocky planets
106:
25:
19:For the Earth's core, see
18:
2495:10.1109/aero.2017.7943771
2299:10.1017/9781316650684.003
2223:10.1038/nature.2017.21379
1113:The Astrophysical Journal
754:
698:
648:existence of a lunar core
476:Stability and instability
424:
208:Planetary differentiation
2332:Treatise on Geochemistry
1263:. Transdyne Corporation.
764:within its metallic core
658:
541:
511:Outer gas and ice giants
263:Core merging and impacts
197:planetary core accretion
28:Accretion (astrophysics)
2580:10.1126/science.1208890
2489:. IEEE. pp. 1–11.
2397:10.1126/science.1084662
2182:10.1093/mnras/110.4.325
1882:. SETI Institute. 2012.
1858:2000E&PSL.176...17H
1416:10.1126/science.1199375
1317:10.1029/gl001i003p00137
1090:1982P&SS...30..755S
887:10.1126/science.1142328
774:Remnant planetary cores
653:giant impact hypothesis
641:
528:Within the Solar System
286:
277:giant impact hypothesis
77:fluid metallic hydrogen
2739:Structure of the Earth
2125:Treatise on Geophysics
1895:Cite journal requires
1276:Cite journal requires
1183:10.1098/rstl.1798.0022
1164:Cavendish, H. (1798).
693:first 30 million years
434:Earth's magnetic field
218:isotopic system has a
46:
38:
2338:. Elsevier: 487–507.
1852:(1). Science: 17–30.
1361:10.2138/rmg.2006.60.3
1197:Wiechert, E. (1897).
44:
36:
2537:on October 16, 2011.
1948:10.1002/2013je004587
1582:10.1029/2012JE004161
691:occurred within the
414:core-mantle boundary
405:Pallasite meteorites
2572:2011Sci...333.1717B
2556:(6050): 1717–1720.
2531:National Geographic
2448:10.1038/nature04311
2440:2006Natur.439..155A
2389:2003Sci...301...84M
2344:2003TrGeo...1..487F
2291:2018mvam.book...30N
2214:2017Natur.542...17C
2173:1950MNRAS.110..325R
2094:2011AGUFMDI41B..03H
2036:10.1038/nature01560
2028:2003Natur.423..163M
1940:2014JGRE..119..480M
1794:10.1038/nature04763
1786:2006Natur.441..825W
1710:2001Natur.412..214S
1610:1976Icar...28..509S
1573:2012JGRE..117.0L09M
1526:. Krieger Pub. Co.
1524:Planetary interiors
1493:1979PEPI...19..168S
1408:2011Sci...331..309W
1353:2006RvMG...60..221W
1309:1974GeoRL...1..137N
1135:2005ApJ...633..465S
1038:2003Icar..164..228F
993:1977Icar...30..111P
937:2004Geo....32...97W
546:The composition of
502:Inner rocky planets
236:siderophile element
1659:Planetary Sciences
825:millisecond pulsar
228:lithophile element
47:
39:
2734:Planetary geology
2610:"Hot Ice Planets"
2434:(7073): 155–160.
2022:(6936): 163–167.
2016:Letters to Nature
1824:"differentiation"
1780:(7095): 825–833.
1704:(6843): 214–219.
1402:(6015): 309–312.
1078:Planet. Space Sci
804:Chthonian planets
768:metallic hydrogen
749:metallic hydrogen
639:
638:
559:Chondritic Model
461:radioactive decay
318:refractory metals
271:Earth–Moon system
190:planetary embryos
165:moment of inertia
154:The cores of the
2746:
2716:
2715:
2704:
2703:
2702:
2692:
2691:
2690:
2680:
2679:
2668:
2667:
2666:
2656:
2655:
2654:
2644:
2643:
2635:
2625:
2624:
2622:
2621:
2606:
2600:
2599:
2565:
2545:
2539:
2538:
2523:
2517:
2516:
2482:
2476:
2475:
2423:
2417:
2416:
2372:
2366:
2365:
2327:
2321:
2320:
2284:
2268:
2262:
2261:
2253:
2244:
2243:
2225:
2193:
2187:
2186:
2184:
2152:
2146:
2145:
2120:
2107:
2104:
2098:
2097:
2077:
2056:
2055:
2011:
2000:
1999:
1991:
1960:
1959:
1925:
1916:
1905:
1904:
1898:
1893:
1891:
1883:
1876:
1870:
1869:
1841:
1832:
1831:
1820:
1814:
1813:
1769:
1746:
1745:
1718:10.1038/35084155
1693:
1682:
1681:
1653:
1640:
1639:
1629:
1627:2060/19750022908
1593:
1587:
1586:
1584:
1552:
1546:
1545:
1519:
1513:
1512:
1476:
1465:
1464:
1450:
1444:
1443:
1387:
1381:
1380:
1335:
1329:
1328:
1292:
1286:
1285:
1279:
1274:
1272:
1264:
1256:
1250:
1249:
1232:(1–4): 456–475.
1217:
1211:
1210:
1194:
1188:
1187:
1185:
1161:
1155:
1154:
1128:
1126:astro-ph/0507009
1108:
1102:
1101:
1073:
1058:
1057:
1031:
1029:astro-ph/0305031
1011:
1005:
1004:
976:
957:
956:
945:10.1130/g19975.1
920:
907:
906:
870:
810:chthonian planet
565:Pyrolitic Model
553:
552:
450:Core heat source
439:changes of phase
295:of both cores).
2754:
2753:
2749:
2748:
2747:
2745:
2744:
2743:
2724:
2723:
2722:
2710:
2700:
2698:
2688:
2686:
2674:
2664:
2662:
2652:
2650:
2638:
2630:
2628:
2619:
2617:
2608:
2607:
2603:
2546:
2542:
2525:
2524:
2520:
2505:
2483:
2479:
2424:
2420:
2383:(5629): 84–87.
2373:
2369:
2362:
2328:
2324:
2309:
2269:
2265:
2254:
2247:
2194:
2190:
2153:
2149:
2143:
2121:
2110:
2105:
2101:
2078:
2059:
2012:
2003:
1992:
1963:
1923:
1917:
1908:
1896:
1894:
1885:
1884:
1878:
1877:
1873:
1842:
1835:
1828:Merriam Webster
1822:
1821:
1817:
1770:
1749:
1694:
1685:
1678:
1654:
1643:
1594:
1590:
1553:
1549:
1534:
1520:
1516:
1477:
1468:
1452:
1451:
1447:
1388:
1384:
1336:
1332:
1293:
1289:
1277:
1275:
1266:
1265:
1257:
1253:
1218:
1214:
1195:
1191:
1162:
1158:
1109:
1105:
1074:
1061:
1012:
1008:
977:
960:
921:
910:
881:(5825): 702–3.
871:
867:
863:
843:
841:Hot ice planets
818:
806:
797:
776:
757:
741:within its core
737:
726:
701:
667:
661:
644:
544:
535:
530:
522:
513:
504:
499:
478:
457:Coriolis forces
452:
443:crystallization
427:
422:
407:
384:
351:
306:
301:
289:
273:
265:
205:
203:Differentiation
178:
173:
152:
140:Apollo missions
132:
120:iron meteorites
115:Henry Cavendish
111:
105:
100:
31:
24:
17:
12:
11:
5:
2752:
2742:
2741:
2736:
2721:
2720:
2708:
2696:
2684:
2672:
2660:
2648:
2627:
2626:
2601:
2540:
2518:
2503:
2477:
2418:
2367:
2360:
2322:
2307:
2263:
2245:
2188:
2167:(4): 325–338.
2147:
2141:
2108:
2099:
2057:
2001:
1961:
1906:
1897:|journal=
1871:
1833:
1815:
1747:
1683:
1676:
1641:
1604:(4): 509–521.
1588:
1547:
1532:
1514:
1487:(2): 168–182.
1466:
1445:
1382:
1347:(1): 221–364.
1330:
1303:(3): 137–140.
1287:
1278:|journal=
1251:
1212:
1189:
1156:
1143:10.1086/449306
1119:(1): 465–473.
1103:
1059:
1022:(1): 228–243.
1006:
958:
908:
864:
862:
859:
842:
839:
831:PSR J1719-1438
821:Carbon planets
817:
814:
805:
802:
796:
793:
785:Psyche mission
775:
772:
756:
753:
736:
733:
725:
722:
700:
697:
671:magnetic field
663:Main article:
660:
657:
643:
640:
637:
636:
633:
630:
627:
623:
622:
619:
616:
613:
609:
608:
605:
602:
599:
595:
594:
591:
588:
585:
581:
580:
577:
574:
571:
567:
566:
563:
560:
557:
543:
540:
534:
531:
529:
526:
521:
520:Observed types
518:
512:
509:
503:
500:
498:
495:
477:
474:
451:
448:
426:
423:
421:
418:
406:
403:
383:
380:
350:
347:
305:
302:
300:
297:
288:
285:
272:
269:
264:
261:
204:
201:
177:
174:
172:
169:
151:
148:
131:
128:
107:Main article:
104:
101:
99:
96:
51:planetary core
15:
9:
6:
4:
3:
2:
2751:
2740:
2737:
2735:
2732:
2731:
2729:
2719:
2714:
2709:
2707:
2697:
2695:
2685:
2683:
2678:
2673:
2671:
2661:
2659:
2649:
2647:
2642:
2637:
2636:
2633:
2616:on 2016-03-04
2615:
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2597:
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2577:
2573:
2569:
2564:
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2551:
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2532:
2528:
2522:
2514:
2510:
2506:
2504:9781509016136
2500:
2496:
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2398:
2394:
2390:
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2378:
2371:
2363:
2361:9780080437514
2357:
2353:
2349:
2345:
2341:
2337:
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2326:
2318:
2314:
2310:
2308:9781316650684
2304:
2300:
2296:
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2283:
2278:
2274:
2267:
2259:
2258:News Releases
2252:
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2203:
2199:
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2142:9780444538031
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1270:
1262:
1255:
1247:
1243:
1239:
1235:
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1227:
1223:
1216:
1209:(3): 221–243.
1208:
1205:(in German).
1204:
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1021:
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1002:
998:
994:
990:
986:
982:
975:
973:
971:
969:
967:
965:
963:
954:
950:
946:
942:
938:
934:
931:(2): 97–100.
930:
926:
919:
917:
915:
913:
904:
900:
896:
892:
888:
884:
880:
876:
869:
865:
858:
856:
852:
848:
838:
836:
832:
828:
826:
822:
813:
811:
801:
792:
790:
786:
781:
780:asteroid belt
771:
769:
765:
761:
752:
750:
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742:
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730:
721:
718:
714:
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564:
561:
558:
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551:
549:
539:
525:
517:
508:
494:
492:
491:asteroid belt
488:
487:geologic time
484:
473:
471:
466:
462:
458:
447:
444:
440:
435:
431:
430:Dynamo theory
417:
415:
411:
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186:planetesimals
183:
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161:
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156:rocky planets
147:
145:
141:
137:
127:
125:
121:
116:
110:
95:
91:
89:
86:
82:
78:
74:
70:
68:
64:
60:
56:
52:
43:
35:
29:
22:
2706:Solar System
2618:. Retrieved
2614:the original
2604:
2553:
2549:
2543:
2535:the original
2530:
2521:
2486:
2480:
2431:
2427:
2421:
2380:
2376:
2370:
2335:
2331:
2325:
2272:
2266:
2257:
2208:(7639): 17.
2205:
2201:
2191:
2164:
2160:
2150:
2124:
2102:
2085:
2081:
2019:
2015:
1995:
1931:
1927:
1888:cite journal
1874:
1849:
1845:
1827:
1818:
1777:
1773:
1701:
1697:
1658:
1601:
1597:
1591:
1567:(E12): n/a.
1564:
1560:
1550:
1523:
1517:
1484:
1480:
1453:
1448:
1399:
1395:
1385:
1344:
1340:
1333:
1300:
1296:
1290:
1269:cite journal
1254:
1229:
1225:
1215:
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1202:
1192:
1173:
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1159:
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1112:
1106:
1081:
1077:
1019:
1015:
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984:
980:
928:
924:
878:
874:
868:
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829:
819:
807:
798:
777:
758:
745:
738:
727:
709:
702:
684:potassium-40
668:
645:
545:
536:
523:
514:
505:
479:
453:
428:
408:
385:
376:potassium-40
352:
307:
290:
274:
266:
216:tungsten-182
206:
194:
179:
153:
133:
112:
109:Earth's core
103:Earth's core
92:
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59:Solar System
50:
48:
2694:Outer space
1176:: 469–479.
835:white dwarf
680:siderophile
483:earthquakes
465:latent heat
253:magma ocean
212:hafnium-182
130:Moon's core
2728:Categories
2620:2014-04-13
2282:1712.02187
1533:089464565X
861:References
795:Extrasolar
783:core. The
675:chondritic
410:Pallasites
358:phosphorus
249:perovskite
160:Mariner 10
144:moonquakes
88:HD149026 b
73:Gas giants
2670:Astronomy
2658:Chemistry
2596:206535504
2563:1108.5201
2456:1476-4687
2317:119021137
2232:0028-0836
1726:1476-4687
1636:120492617
1542:123053051
1509:0031-9201
1440:206530647
1424:0036-8075
1377:130734866
1369:1529-6466
1325:0094-8276
1246:129025380
1151:119026159
903:129291662
378:as well.
372:potassium
339:germanium
299:Chemistry
293:viscosity
257:oxidation
244:chondrite
220:half-life
176:Accretion
171:Formation
113:In 1797,
98:Discovery
85:exoplanet
2588:21868629
2513:45190228
2464:16407944
2405:12843390
2240:28150796
2044:12736683
1956:41492849
1802:16778882
1734:11449282
1462:18035258
1432:21212323
1054:54961173
953:40968487
895:17478710
729:Ganymede
724:Ganymede
632:Unknown
607:Unknown
604:Unknown
556:Element
485:through
470:silicate
420:Dynamics
399:tantalum
391:tungsten
335:tantalum
327:chromium
323:vanadium
321:Earth's
240:silicate
232:tungsten
2718:Science
2646:Physics
2632:Portals
2568:Bibcode
2550:Science
2472:4406814
2436:Bibcode
2385:Bibcode
2377:Science
2340:Bibcode
2287:Bibcode
2210:Bibcode
2169:Bibcode
2090:Bibcode
2052:4430068
2024:Bibcode
1936:Bibcode
1854:Bibcode
1830:. 2014.
1810:8942975
1782:Bibcode
1742:4391025
1706:Bibcode
1606:Bibcode
1569:Bibcode
1489:Bibcode
1404:Bibcode
1396:Science
1349:Bibcode
1305:Bibcode
1131:Bibcode
1086:Bibcode
1034:Bibcode
989:Bibcode
933:Bibcode
925:Geology
875:Science
847:GJ1214b
735:Jupiter
626:Oxygen
612:Sulfur
598:Cobalt
584:Nickel
533:Mercury
395:Niobium
387:Hafnium
363:Silicon
343:gallium
331:niobium
224:Hafnium
182:accrete
81:Jupiter
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981:Icarus
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760:Saturn
755:Saturn
705:Zagami
601:0.26%
579:78.7%
576:94.4%
573:88.6%
463:, and
425:Dynamo
367:oxygen
354:Sulfur
314:mantle
255:is an
124:P-wave
55:planet
2682:Stars
2592:S2CID
2558:arXiv
2509:S2CID
2468:S2CID
2409:S2CID
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2048:S2CID
1952:S2CID
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1147:S2CID
1121:arXiv
1050:S2CID
1024:arXiv
949:S2CID
899:S2CID
855:water
851:GJ436
659:Earth
635:9.8%
621:4.9%
615:5.1%
593:6.6%
590:5.6%
587:5.5%
570:Iron
548:Venus
542:Venus
310:crust
281:Theia
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