Changes in Earth's Orbit Linked to Extinctions 311
Josh Fink writes "A group of Dutch Scientists have recently released a study stating that they have found that changes in Earth's orbit around the sun are linked to mammal extinctions. From the article: '"Extinctions in rodent species occur in pulses which are spaced by intervals controlled by astronomical variations and their effects on climate change..." The cycles are associated with lower temperatures, changes in precipitation, habitats, vegetation and food availability which are the main factors influencing the extinction peaks, the study published in the journal Nature said.' So on top of worrying about global warming, it seems we should also worry about the physics that govern the orbit of Earth around the sun. Too bad we don't have a way of keeping the Earth in the same orbit/on the same axis of rotation."
Model orbital changes on your own compy (Score:5, Interesting)
The EdGCM [columbia.edu] project has wrapped a NASA GCM in a graphical interface. You can double-click to install, and if you'd like to turn the sun down a few percent or change the orbit, there are checkboxes and sliders. Press play, wait a while (hours to a day or so depending on your computer), and you can look at the results...
Disclaimer: I'm the developer.
Re:BTW (Score:4, Interesting)
Not saying this necessarily applies; just pointing out that just because a process may be gradual does not mean that its consequences can't be sudden.
Re:BTW (Score:3, Interesting)
Re:BTW (Score:3, Interesting)
Re:BTW (Score:4, Interesting)
Re:Move Along (Score:2, Interesting)
Modifying the orbit of Earth is feasible! (Score:4, Interesting)
Yes, we have! And it's very interesting indeed!
http://www.space.com/scienceastronomy/planetearth
A link to the paper: Korycansky, D. G.; Laughlin, Gregory; Adams, Fred C. Astronomical engineering: a strategy for modifying planetary orbits. Astrophys.Space Sci. 275 (2001) 349-366
http://arxiv.org/abs/astro-ph/0102126 [arxiv.org]
Abstract:
"The Sun's gradual brightening will seriously compromise the Earth's biosphere within ~ 1E9 years. If Earth's orbit migrates outward, however, the biosphere could remain intact over the entire main-sequence lifetime of the Sun. In this paper, we explore the feasibility of engineering such a migration over a long time period. The basic mechanism uses gravitational assists to (in effect) transfer orbital energy from Jupiter to the Earth, and thereby enlarges the orbital radius of Earth. This transfer is accomplished by a suitable intermediate body, either a Kuiper Belt object or a main belt asteroid. The object first encounters Earth during an inward pass on its initial highly elliptical orbit of large (~ 300 AU) semimajor axis. The encounter transfers energy from the object to the Earth in standard gravity-assist fashion by passing close to the leading limb of the planet. The resulting outbound trajectory of the object must cross the orbit of Jupiter; with proper timing, the outbound object encounters Jupiter and picks up the energy it lost to Earth. With small corrections to the trajectory, or additional planetary encounters (e.g., with Saturn), the object can repeat this process over many encounters. To maintain its present flux of solar energy, the Earth must experience roughly one encounter every 6000 years (for an object mass of 1E22 g). We develop the details of this scheme and discuss its ramifications."
Global warming vs. global wobbling (Score:3, Interesting)
http://cdiac.ornl.gov/trends/temp/vostok/graphics
shows that for last 450,000 years Earth was mostly in the Ice Age, interrupted
by 10,000 year long warm periods spaced 100,000 years apart. We are about 15,000
years into the last warm period on record.
Because of strong periodicity, the current best explanation of this cycle is
by astronomical phenomena (Earth orbit/axis wobble).
This does not contradict global warming---it just shows that the climate
is a very delicate balance between strong opposing phenomena; the point being
that we should be real careful how we influence it.