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Today there are numerous studies on asteroid mining. They elaborate on selecting the right objects, prospecting missions, potential asteroid redirection, and the mining process itself. For economic reasons, most studies focus on mining…

Earth and Planetary Astrophysics · Physics 2018-12-27 Thomas I. Maindl , Roman Miksch , Birgit Loibnegger

Advances in robotics and additive manufacturing have become game-changing for the prospects of space industry. It has become feasible to bootstrap a self-sustaining, self-expanding industry at reasonably low cost. Simple modeling was…

Popular Physics · Physics 2016-12-13 Philip T. Metzger , Anthony Muscatello , Robert P. Mueller , James Mantovani

To deflect impact-trajectory of massive km^3 and spinning asteroid by a few terrestrial radius one need a large momentum exchange. The dragging of huge spinning bodies in space by external engine seems difficult or impossible. Our solution…

Astrophysics · Physics 2008-03-11 D. Fargion

Satellites around large asteroids are preferentially found among those with the most rapid rotation and elongated shape. The taxonomic statistics are similarly skewed; in total, 13 asteroids larger than 100 km are known to have satellites,…

Earth and Planetary Astrophysics · Physics 2025-05-07 Kevin J. Walsh , Ronald-Louis Ballouz , Harrison F. Agrusa , Josef Hanus , Martin Jutzi , Patrick Michel

A method for asteroid deflection that makes use of a spacecraft moving back and forth on a segment of an appropriate Keplerian orbit about the asteroid is described and evaluated. It is shown that, on average, the spacecraft describing such…

Space Physics · Physics 2017-04-05 Yohannes Ketema

This paper proposes a distributed on-orbit spacecraft assembly algorithm, where future spacecraft can assemble modules with different functions on orbit to form a spacecraft structure with specific functions. This form of spacecraft…

Robotics · Computer Science 2024-11-27 Tianle Liu , Zhixiang Wang , Yongwei Zhang , Ziwei Wang , Zihao Liu , Yizhai Zhang , Panfeng Huang

A model for the asteroid resurfacing by regolith convection is built to estimate its timescale. In the model, regolith convection is driven by the impact-induced global seismic shaking. The model consists of three steps: (i) intermittent…

Earth and Planetary Astrophysics · Physics 2016-04-06 Tomoya M. Yamada , Kousuke Ando , Tomokatsu Morota , Hiroaki Katsuragi

Through multiple, small unmanned probes we can more efficiently capture an asteroid and return it to lunar orbit. The Asteroid Return and Exploration System (ARES) aims to make use of previously tested technology with the application of a…

Space Physics · Physics 2014-10-08 Charles Domercant , Aiden Gonzalez

Asteroid mining can become an enabling technology to establish a sustainable manned colony on Mars, which requires metallic materials more often than they are readily available in shipments from Earth. This paper describes a feasibility…

Instrumentation and Methods for Astrophysics · Physics 2026-04-22 Serena Suriano , Shamil Biktimirov , Dmitry Pritykin , Anton Ivanov

The Asteroid Redirect Mission (ARM) proposes to retrieve a near-Earth asteroid and position it in a lunar distant retrograde orbit (DRO) for later study, crewed exploration, and ultimately resource exploitation. During the Caltech Space…

Earth and Planetary Astrophysics · Physics 2015-05-15 Javier Roa , Casey J. Handmer

As the space industry matures, large space stations will be built. This paper organizes and documents constraints on the size of these space stations. Human frailty, station design, and construction impose these constraints. Human…

Popular Physics · Physics 2024-08-02 David W. Jensen

Designing for rotational stability can dramatically affect the geometry of a space station. If improperly designed, the rotating station could end up catastrophically tumbling end-over-end. Active stabilization can address this problem;…

Popular Physics · Physics 2024-08-02 David W. Jensen

Asteroids are leftover pieces from the era of planet formation that help us understand conditions in the early Solar System. Unlike larger planetary bodies that were subject to global thermal modification during and subsequent to their…

Earth and Planetary Astrophysics · Physics 2009-06-25 Kevin J. Walsh , Patrick Michel , Derek C. Richardson

Radiolocation methods of probing minor celestial bodies (asteroids) by the nanosecond pulses can be used for monitoring of near-Earth space with the purpose of identification of hazardous cosmic objects able to impact the Earth. Development…

Earth and Planetary Astrophysics · Physics 2015-05-20 V. D. Zakharchenko , I. G. Kovalenko , O. V. Pak

Solar system small bodies come in a wide variety of shapes and sizes, which are achieved following very individual evolutional paths through billions of years. This paper focuses on the reshaping process of rubble-pile asteroids driven by…

Earth and Planetary Astrophysics · Physics 2017-08-03 Yang Yu , Derek C. Richardson , Patrick Michel

Time-resolved photometry of asteroids can be used for shape and spin reconstruction. If the number of measurements per asteroid is not sufficient to create a model, the whole data set can be used to reconstruct the distribution of shape…

Earth and Planetary Astrophysics · Physics 2020-05-14 Mikko Kaasalainen , Josef Durech

Asteroids and meteorites provide key evidence on the formation of planetesimals in the Solar System. Asteroids are traditionally thought to form in a bottom-up process by coagulation within a population of initially km-scale planetesimals.…

Earth and Planetary Astrophysics · Physics 2016-08-31 Anders Johansen , Emmanuel Jacquet , Jeffrey N. Cuzzi , Alessandro Morbidelli , Matthieu Gounelle

Using a fully autonomous spacecraft - Bering - we propose to detect and study sub-km asteroids from an orbit within the asteroid Main Belt. The main purpose of the proposed Bering mission is to detect a statistically significant sample of…

As evidenced by recent survey results, majority of asteroids are slow rotators (P>12 h), but lack spin and shape models due to selection bias. This bias is skewing our overall understanding of the spins, shapes, and sizes of asteroids, as…

Earth and Planetary Astrophysics · Physics 2023-11-08 A. Marciniak , J. Ďurech , A. Choukroun , J. Hanuš , W. Ogłoza , R. Szakáts , L. Molnár , A. Pál , F. Monteiro , E. Frappa , W. Beisker , H. Pavlov , J. Moore , R. Adomavičienė , R. Aikawa , S. Andersson , P. Antonini , Y. Argentin , A. Asai , P. Assoignon , J. Barton , P. Baruffetti , K. L. Bath , R. Behrend , L. Benedyktowicz , L. Bernasconi , G. Biguet , M. Billiani , D. Błażewicz , R. Boninsegna , M. Borkowski , J. Bosch , S. Brazill , M. Bronikowska , A. Bruno , M. Butkiewicz - Bąk , J. Caron , G. Casalnuovo , J. J. Castellani , P. Ceravolo , M. Conjat , P. Delincak , J. Delpau , C. Demeautis , A. Demirkol , M. Dróżdż , R. Duffard , C. Durandet , D. Eisfeldt , M. Evangelista , S. Fauvaud , M. Fauvaud , M. Ferrais , M. Filipek , P. Fini , K. Fukui , B. Gährken , S. Geier , T. George , B. Goffin , J. Golonka , T. Goto , J. Grice , K. Guhl , K. Halíř , W. Hanna , M. Harman , A. Hashimoto , W. Hasubick , D. Higgins , M. Higuchi , T. Hirose , R. Hirsch , O. Hofschulz , T. Horaguchi , J. Horbowicz , M. Ida , B. Ignácz , M. Ishida , K. Isobe , E. Jehin , B. Joachimczyk , A. Jones , J. Juan , K. Kamiński , M. K. Kamińska , P. Kankiewicz , H. Kasebe , B. Kattentidt , D. -H. Kim , M. -J. Kim , K. Kitazaki , A. Klotz , M. Komraus , I. Konstanciak , R. Könyves - Tóth , K. Kouno , E. Kowald , J. Krajewski , G. Krannich , A. Kreutzer , A. Kryszczyńska , J. Kubánek , V. Kudak , F. Kugel , R. Kukita , P. Kulczak , D. Lazzaro , J. Licandro , F. Livet , P. Maley , N. Manago , J. Mánek , A. Manna , H. Matsushita , S. Meister , W. Mesquita , S. Messner , J. Michelet , J. Michimani , I. Mieczkowska , N. Morales , M. Motyliński , M. Murawiecka , J. Newman , V. Nikitin , M. Nishimura , J. Oey , D. Oszkiewicz , M. Owada , E. Pakštienė , M. Pawłowski , W. Pereira , V. Perig , J. Perła , F. Pilcher , E. Podlewska-Gaca , J. Polák , T. Polakis , M. Polińska , A. Popowicz , F. Richard , J. J. Rives , T. Rodrigues , Ł. Rogiński , E. Rondón , M. Rottenborn , R. Schäfer , C. Schnabel , O. Schreurs , A. Selva , M. Simon , B. Skiff , M. Skrutskie , J. Skrzypek , K. Sobkowiak , E. Sonbas , S. Sposetti , P. Stuart , K. Szyszka , K. Terakubo , W. Thomas , P. Trela , S. Uchiyama , M. Urbanik , G. Vaudescal , R. Venable , Ha. Watanabe , Hi. Watanabe , M. Winiarski , R. Wróblewski , H. Yamamura , M. Yamashita , H. Yoshihara , M. Zawilski , P. Zelený , M. Żejmo , K. Żukowski , S. Żywica

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…

Astrophysics · Physics 2009-02-02 D. G. Korycansky , Gregory Laughlin , Fred C. Adams
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