<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">IJAA</journal-id><journal-title-group><journal-title>International Journal of Astronomy and Astrophysics</journal-title></journal-title-group><issn pub-type="epub">2161-4717</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ijaa.2013.34060</article-id><article-id pub-id-type="publisher-id">IJAA-41086</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Cosmic Engineering: Moving Asteroids
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>arcin</surname><given-names>Misiak</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>UAM, Poznan, Poland</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>gmuse2@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>09</day><month>10</month><year>2013</year></pub-date><volume>03</volume><issue>04</issue><fpage>517</fpage><lpage>519</lpage><history><date date-type="received"><day>June</day>	<month>8,</month>	<year>2013</year></date><date date-type="rev-recd"><day>July</day>	<month>8,</month>	<year>2013</year>	</date><date date-type="accepted"><day>July</day>	<month>16,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   This paper presents methods of orbit transfer for small planetoids from the main belt to the future colonies on Mars using current technologies. The results show that by using nuclear weapon or even kinetic energy weapon (for retrograde bodies) asteroids with masses up to about 100 tons can be moved. Both options assume that asteroid will survive explosion. 
 
</p></abstract><kwd-group><kwd>Astrodynamics; Celestial Mechanics; Orbital Motion; Optimal Control</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In recent years there is a growing interest in the planetoids, concerning extraction of precious materials from them, like iron, nickel, water or platinum [<xref ref-type="bibr" rid="scirp.41086-ref1">1</xref>]. The common view is to send a spaceship, extract minerals and bring them back to Earth. This is an expensive, timeand effort-consuming approach. Instead we propose moving asteroids from its original place in the main belt to the planet Mars (or could be also Moon) where future human colonies will be held. The idea of modifying orbits of celestial objects was considered in literature before for example in quite fictional proposal to higher Earth orbit because of Sun’s future brightening [<xref ref-type="bibr" rid="scirp.41086-ref2">2</xref>].</p><p>The methods we employ are similar to those considered in the case of a deflection of an asteroid on the collision curse with the Earth [3-5].</p><p>In Chapter 2 we consider nuclear explosion in front of an asteroid, in Chapter 3 kinetic energy weapon, Chapter 4 considers the effect of light pressure on the asteroids and finally in Chapter 5 we present a short summary.</p></sec><sec id="s2"><title>2. Nuclear Explosion</title><p>Let’s consider sending a spacecraft equipped with nuclear weapon to an asteroids. Assuming nuclear explosion just in front of an asteroid (<xref ref-type="fig" rid="fig1">Figure 1</xref>) huge energy will be released in high energy gamma rays and very energetic particles. This energy will slow down the asteroid.</p><p>We treat the interaction between the products of nuclear explosion and an asteroid as an inelastic collision. Supposing proportionality of momentum and energy like</p><p>for radiation<img src="20-4500178\5e9f5075-d996-4778-8949-5ad76993f3a7.jpg" />, from the conservation of momentum follows:</p><p><img src="20-4500178\e3db6af8-3c2c-4fd1-aad5-dfed2e27edc3.jpg" /></p><disp-formula id="scirp.41086-formula68356"><label>, (1)</label><graphic position="anchor" xlink:href="20-4500178\5338629e-9804-44ef-8f0a-69c126478326.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="20-4500178\c0cd94e6-793e-4b51-9e41-44dd338e3c75.jpg" />—velocity of an asteroid before explosion,<img src="20-4500178\db4b4e92-b583-4831-bdd6-aeea19461d46.jpg" />—velocity of an asteroid after the explosion,<img src="20-4500178\67b33570-f242-4d6a-bff7-a53764c9bc04.jpg" />— mass of an asteroid.</p><p>Hydrogen bomb can release <img src="20-4500178\d46ae375-4986-47e0-a47c-958a61632b45.jpg" /> of energytypical asteroids velocity in the main belt is <img src="20-4500178\6136d6cb-54bc-4889-a386-946f59ec74c3.jpg" /></p><p>and the final velocity we want to achieve is according to Hohmann transfer [6,7] between asteroid-Mars system:</p><p><img src="20-4500178\becdb8b9-fd16-42ee-adf9-5ae42d6ffb9e.jpg" /></p><p>Introducing these numbers to the Equation (1) we can compute the mass of the asteroids which can be moved in this way:</p><p><img src="20-4500178\48b00e43-ccf1-46fb-ba69-8f0392ab21c5.jpg" /></p><p>If we suppose that an asteroids is built from pure nickel, and current price 18 $/kg the asteroids will be worth more than 1 million dollars.</p><p>The similar procedure can also be applied for the Kuiper belt objects.</p></sec><sec id="s3"><title>3. Kinetic Energy Weapon</title><p>As a second possibility to move an asteroid we consider shooting an asteroid by 5 tons weapon from the Earth orbit. This approach can be useful if we can find an asteroid which orbit the Sun in the opposite direction as the Earth does (retrograde motion) <xref ref-type="fig" rid="fig2">Figure 2</xref>.</p><p>In that case we can take advantage from the Earth motion around the Sun (about<img src="20-4500178\4a629416-0e76-4ace-af56-af1e788781a5.jpg" />). For an inelastic col-</p><p>lision the conservation of momentum leads to:</p><p><img src="20-4500178\64707326-ec96-4d6c-a4b2-b608156ddae5.jpg" /></p><disp-formula id="scirp.41086-formula68357"><label>, (2)</label><graphic position="anchor" xlink:href="20-4500178\e0a95b05-f5e5-4b75-b331-d4b9de71860a.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="20-4500178\a7d3dc67-9c54-42da-9f38-611d7e46750f.jpg" />—mass of an asteroid, where<img src="20-4500178\a182d2dd-307f-45e6-8130-740a2f2d8323.jpg" />—mass of a weapon,<img src="20-4500178\f23b0b66-be89-4b82-aaf7-04cba5741fce.jpg" />—velocity of an asteroid before the collision,<img src="20-4500178\3b7e331e-9ea7-4998-afce-6cf34f601ec3.jpg" />—velocity of an asteroid after the collision,<img src="20-4500178\c28c5b5a-4f7b-4178-9561-b7d353903b8c.jpg" />—velocity of the weapon.</p><p>The velocity of the weapon shot from the Earth in the moment of collision is:</p><p><img src="20-4500178\bf44e95f-c432-4b82-b76c-cb1afc209ae6.jpg" /></p><p>Substituting this and<img src="20-4500178\295ab415-30f2-4432-9d30-5a3535cf4e87.jpg" />, <img src="20-4500178\ee8e4b02-f439-4d77-b5b6-9f64580ff5c9.jpg" />to the Equation (2) we get:</p><p><img src="20-4500178\8e656b39-e8e3-4964-97d6-634eb5738f57.jpg" /></p><p>We can also consider an elastic collision, which is probably more difficult to construct (something like air bags used by NASA in Mars missions). In this case from the conservation of momentum and energy follows:</p><p><img src="20-4500178\bf48ae8d-2de2-4939-9b45-7568a6425234.jpg" /></p><p>which after substitution yields to:</p><p><img src="20-4500178\277469c8-7be9-492d-bf34-b411a7965c00.jpg" /></p><p>The solution of the above equation gives for the mass of the asteroids possible to transfer in this way:</p><p><img src="20-4500178\54172ae3-d22e-4934-aadb-6db0430624d7.jpg" /></p><p>This value is more than twice the mass possible to move through inelastic collision.</p></sec><sec id="s4"><title>4. Solar Sail</title><p>As a third possibility for moving asteroid to a desired position let’s consider attaching a huge solar sail. The average force in Newton’s acting on a sail from light pressure at a distance about 2AU is:</p><p><img src="20-4500178\ca5285fb-8ab7-4867-9c52-91f69bd3ba92.jpg" />where<img src="20-4500178\e4021d7e-3449-4610-bac6-b206fb6a12fc.jpg" />—area of the sail in square meter.</p><p>Considering sail with area <img src="20-4500178\3636c1d0-1711-416c-b7cb-5b1c8b9243aa.jpg" /> we get the force about<img src="20-4500178\8de76e75-a8c8-4f89-b47b-d4ab716481d5.jpg" />. Depending on the orientation of the sail we can move asteroid spiralling inward or outward from the Sun [<xref ref-type="bibr" rid="scirp.41086-ref8">8</xref>]. In the case of moving asteroid from the main belt to Mars we need inward spiralling and orientation of the sail shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>. In this case the force has two components: radial <img src="20-4500178\53d85b01-886f-4ddf-bebb-bb663df05630.jpg" /> and tangential <img src="20-4500178\d720a335-1a76-483a-aa7f-af436acb89bd.jpg" />, where <img src="20-4500178\ae098a24-c2bc-4766-b631-8cce19ec7d1b.jpg" /> is the angle between sun light and the line perpendicular to the sail.</p><p>Substituting <img src="20-4500178\7bf01264-c037-4331-b60e-f180f2554699.jpg" /> the mass of the asteroids possible to move in about a year is:</p><p><img src="20-4500178\ca81ad8c-59b9-4bf8-b4a7-96e6056ff837.jpg" /></p><p>Another option using the pressure of the light which can be considered is to attach small nuclear reactor equipped with a laser to an asteroid. In this scenario the energy generated by nuclear reactions is used to power the laser. The beam of light from the laser is sent in the direction of the velocity of the asteroid. As a result asteroid will spiral from the main belt inward the Sun and can reach the Mars orbit. If the reactor has the mass M and the power 100 MW the mass of the asteroid which can be transferred from the main belt to the Mars in a year is about:</p><p>Assuming mass of the reactor with fuel<img src="20-4500178\4d7ea336-49c1-4867-906e-27e5d6f00fda.jpg" />, mass of the asteroid is also<img src="20-4500178\4490cf4b-6910-4ff9-9469-69f394175b8a.jpg" />.</p></sec><sec id="s5"><title>5. Summary</title><p>From the options considered, the most universal is a nuclear blast in front of the asteroid. The biggest possible mass to move from the main belt to Mars we got in elastic collision between missiles ejected from the Earth and an asteroid is 131,000 kg. However this possibility requires finding an asteroid which orbits the Sun in the opposite direction. Both options assume that asteroid will survive explosion (collision). 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