On the previous page the comparison between the Earth and Pluto (2,274 km) was addressed by the planets both having large companion moons. It is believed the Charon (1,212 km) itself was created by a larger body striking Pluto, similar to the formation of our own moon (fig. 1). The theory of Earth having a second moon could also be drawn from the recent discovery of two additional moons around Pluto. What this tell us is that a planetary collision, followed by an accretion of debris into a single moon does not totally discount the possibility of the planet having additional moons. Although these two moons around Pluto are most likely captured bodies from the Kuiper Belt - perhaps Earth itself captured either a rogue moon of one from an orbit the crossed Earth's orbit several hundred million years ago. We have seen earlier how Pluto's orbit takes it inside that of Neptune's, and additional, where did the Mars size object that struck the Earth four billion years ago come from. If it can happen once, then it could easily be considered possible to happen twice. |
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I have selected Uranus's moon Miranda (470 km)
as a captured moon because of its size, mass and uncompleted composition due to failed
accretion (which is covered in another page). |
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Looking at the graph below, one can see the density of Miranda, the Moon and the Earth. It is interesting to see that Miranda is quite less then the Moon in density. If will took both moons and orbited them around a planet with the mass, density and bulk size of Earth, a moon like Miranda would be quickly pulled apart and fall progressively into a decaying orbit. This would mean that there could simply be no 500 hundred million year, periodic impacts from this debris to explain the extinction cycles. |
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If we look at Mars (3,397.2 km) , we can see that the small moon Phobos (13.4x9.2 km), now orbiting the planet at only 6,050 km -
will eventually crash into the planets surface within 70 million years. Phobos's currently
decaying orbit is well within the distance we find between that of the Earth and our Moon.
In fact, it would be awfully close. Allowing a 1.3 density of our second moon, it would
off had to been outside the current orbit of our moon (even allowing for the moons closer
orbit back then). |
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| A Fiery Encounter | A Fateful Rendezvous | A Celestial Visitor | Of Gravitational Tides | Circles Of Unrest |
| Impact Extinction's | A Final Requiem | Acknowledgements | Back To Main Page |
| Karina Hall's - Macquarie University Eureka Schools Prize (website Entry) For Earth, Environmental & Planetary Sciences 2006 | |