astro-ph/0509595 [abs, pdf] :
Title: A Gravitational Tractor for Towing Asteroids
Authors: Edward T. Lu, Stanley G. Love
Categories: astro-ph
Comments: 4 pages, 1 figure - to be published in Nature
We present a concept for a spacecraft that can controllably alter the trajectory of an Earth threatening asteroid using gravity as a towline. The spacecraft hovers near the asteroid with thrusters angled outward so the exhaust does not impinge on the surface. This deflection method is insensitive to the structure, surface properties, and rotation state of the asteroid.
http://arxiv.org/abs/astro-ph/0509595
This was proposed about a year ago by one of the astronauts -- can't remember which one. It does look as though it might actually work.
Sadly, I get blocked from viewing the file - anyone care to repost, or to point me somewhere else?
Thanks!
Bob shaw
Bob, here the PDF version I downloaded from ArXiv...
The proposed method is simple but seems a little bit inefficient to me... in the example they give, it needs a 10 ton spaceship hoovering 50m above a 200m asteroid for 20 years using a nuclear ion drive!
This is a relatively heavy spacecraft and wide deviation angle of thrust reduce it's efficiency... I have impression that a smaller probe anchored to surface and using in-situ material (heating it or escavating and accelerating material) would be more efficient, even if a little bit more complicated to make...
Is there any real Earth's survival against asteroides/meteors proposal that is to implemented at the present time? I haven't heard any of this from NASA, JAXA, ESA. It is time to prepare and later would to late and will cost us a much higher price than a longer term investment.
I think it is of first priority for the preservation of Earth's life. Let us experiment with a safe asteroide different than ones of Apophis 2004 MN4 to see the results so that we can feel more confident for next similar mission.
About tugging or pushing, the first is simpler and elegant but slower since the spacecraft cannot push harder than the gravitational atraction force. The second is more complex but it has greater throughput and more dangerous of losing the trajectory control. These terms are elaborated according to the intuition and not by the math calculations.
I think that every nations must contribute resources and money to concrete this project since it is a Earth's survival project.
Rodolfo
A lot of intermixing of English and Metric units in that report. Didn't that get us
in trouble once already?
If we are going to try and move an asteroid around, let's make sure we get it right.
At least there is a project for deflection of an asteroide from ESA:
September 26
Two Asteroid Targets Chosen for Deflection Test
The European Space Agency (ESA) has selected two asteroids as potential targets for a mission aimed at deflecting a nearby space rock.
After a comprehensive review, the space agency selected the near-Earth objects 2002 AT4 and 1989 ML as primary targets for its upcoming Don Quijote mission. The mission will send two spacecraft, dubbed Hidalgo and Sancho, to an asteroid in hopes of slightly deflecting the space rock’s path.
The Don Quijote mission will visit only one of the two asteroid targets – a final decision will be made in 2007 – and calls for the Hidalgo craft to slam into the space rock at a high speed while Sancho records the event, ESA officials said. The Sancho probe is slated to arrive at the asteroid earlier than Hidalgo to observe the object before and after the impact, they added.
Don Quijote’s mission is designed to demonstrate the feasibility of changing an asteroid’s orbit – however slightly – using conventional spacecraft technology. Two teams are expected to flesh out plans for the mission’s spacecraft pair, with a final design selection to made in 2007 along with the target space rock, ESA officials said.
-- SPACE.com Staff.
More information, http://www.esa.int/gsp/completed/neo/donquijote.html
Rodolfo
'Gravity tractor' to deflect Earth-bound asteroids
NewScientist.com News Service Nov. 9, 2005
NASA scientists have come up with a surprisingly simple yet effective
way to deflect an Earth-bound asteroid: park a large spacecraft
close by and let gravity do the work, creating an invisible towline
to tug the rock off its deadly course.
The strategy crucially relies on our ability to detect an
asteroid threat about 20 years in advance. For...
http://www.kurzweilai.net/email/newsRedirect.html?newsID=5014&m=7610
DEFLECTING INCOMING ASTEROIDS (Science Show: 12/11/2005)
There is a long tradition in film and literature of an asteroid being
diverted at the last moment from its collision course with Earth by the
miracles of space technology. Back in the real world, a study by Britian's
Engineering and Physical Sciences Research Council will look at some
realistic ways to avoid catastrophic collisions. Dr Ed Lew from the Johnson
Space Centre says that, with a couple of decades notice gravity could be
used to deflect an incoming asteroid.
http://www.abc.net.au/rn/science/ss/stories/s1502451.htm
Don't dismiss the value of breaking up a large impactor.
Each year, the Earth is hit by tons and tons of asteroid and cometary material, enough that, if it were to hit all at once, it would cause an impact big enough to wipe out most life on the planet. But it hits in very tiny fragments that burn up before they reach the ground.
If you could blast a relatively small asteroid, like Itokawa, into billions of grains of sand, its impact would not be noticed. Of course, you couldn't reduce the whole thing to such small particles, larger pieces would remain and would make it through to impact -- but they would be a *lot* smaller than the original impactor, and each would have a lot less effect on the ecosystem.
The whole point is to increase the asteroid's surface area. The more of the mass that's subject to ablation, the more of the mass that will simply burn up in the upper atmosphere and filter slowly down to the surface over the following months. And since we already receive thousands of tons of such material every year, that's not really a threat. The remaining several thousand pieces large enough to make it to the ground might cause a lot of local destruction, but (if they were all kept small enough) would be no worse in overall effect than if a few hundred square km were heavily carpet-bombed.
All in all, I'd rather have a few thousand 100-meter craters and the ensuing, potentially manageable destruction casued by them, than have a single 200-km cratering event whose blast effects would wipe out most life on Earth...
-the other Doug
Astrophysics, abstract
astro-ph/0102126
From: Donald Korycansky [view email]
Date: Wed, 7 Feb 2001 22:40:53 GMT (84kb)
Astronomical engineering: a strategy for modifying planetary orbits
Authors: D. G. Korycansky, Gregory Laughlin, Fred C. Adams
Comments: 21 pgs, 7 figs. Paper to appear in Astrophysics and Space Science
Journal-ref: Astrophys.Space Sci. 275 (2001) 349-366
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.
http://arxiv.org/abs/astro-ph/0102126
Powered by Invision Power Board (http://www.invisionboard.com)
© Invision Power Services (http://www.invisionpower.com)