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[sci.astro] Solar System (Astronomy Frequently Asked Questions) (5/9)
Section - E.17.2 What can we do about avoiding impacts?

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Previous Document: E.17.1 What would be the effects of an asteroid impact on the Earth?
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A number of papers on the risks, potential damages from impacts, and
ways to mitigate the danger is at
<URL:http://www.llnl.gov/planetary/>.

Our ability to prevent impacts depends upon several things, the size
of the object, its orbit, and the amount of time until impact.
Generally speaking, the more time the better.  It is perhaps
counter-intuitive, but we could mount the best defense against objects
in orbits similar to that of Earth.  Such an object would pass close
to Earth several times, giving us many chances to discover it,
calculate an extremely accurate orbit, and launch one or more missions
to it.  We might have decades or even centuries to plan.  Conversely,
a comet on an impact course might be discovered only a month or so
away from impact, giving us little or no time to act.

The optimum approach to avoiding an impact is to discover an object
well before impact and gently nudge it.  If discovered long enough
before impact, only small nudges are sufficient to change the object's
orbit so that it will no longer strike Earth.  There are a number of
strategies to nudge an asteroid including landing a rocket engine on
the asteroid or vaporizing a small portion of it with a laser or
stand-off nuclear blast or reflected, concentrated sunlight.

Popular depictions of laser beams or nuclear weapons being used to
blast asteroids into pieces are usually unrealistic; moreover, if
actually used, such "solutions" would probably make the situation
worse.  First, it is unlikely that the firepower exists to blow apart,
say, a 5 km asteroid.  Second, even if we could blow apart an
asteroid, most of the pieces would stay on essentially the same orbit,
i.e., on target to hit the Earth.  A rain of 1000 100-m--sized objects
could still cause considerable damage.

User Contributions:

1
Keith Phemister
Sep 13, 2024 @ 11:23 pm
Copied from above: If the Universe were infinitely old, infinite in extent, and filled
with stars, then every direction you looked would eventually end on
the surface of a star, and the whole sky would be as bright as the
surface of the Sun.
Why would anyone assume this? Certainly, we have directions where we look that are dark because something that does not emit light (is not a star) is between us and the light. A close example is in our own solar system. When we look at the Sun (a star) during a solar eclipse the Moon blocks the light. When we look at the inner planets of our solar system (Mercury and Venus) as they pass between us and the Sun, do we not get the same effect, i.e. in the direction of the planet we see no light from the Sun? Those planets simply look like dark spots on the Sun.
Olbers' paradox seems to assume that only stars exist in the universe, but what about the planets? Aren't there more planets than stars, thus more obstructions to light than sources of light?
What may be more interesting is why can we see certain stars seemingly continuously. Are there no planets or other obstructions between them and us? Or is the twinkle in stars just caused by the movement of obstructions across the path of light between the stars and us? I was always told the twinkle defines a star while the steady light reflected by our planets defines a planet. Is that because the planets of our solar system don't have the obstructions between Earth and them to cause a twinkle effect?
9-14-2024 KP

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