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A simple formalism is presented to assess how many asteroids contain ore, i.e. commercially profitable material, and not merely a high concentration of a resource. I apply this formalism to two resource cases: platinum group metals (PGMs)…

地球与行星天体物理 · 物理学 2013-12-17 Martin Elvis

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…

空间物理 · 物理学 2014-10-08 Charles Domercant , Aiden Gonzalez

While of order a million asteroids have been discovered, the number in rigorously controlled samples that have precise orbits and rotation periods, as well as well-measured colors, is relatively small. In particular, less than a dozen…

地球与行星天体物理 · 物理学 2015-06-12 Andrew Gould , Jennifer C. Yee

Asteroid mining offers the possibility to revolutionize supply of resources vital for human civilization. Preliminary analysis suggests that Near-Earth Asteroids (NEA) contain enough volatile and high value minerals to make the mining…

天体物理仪器与方法 · 物理学 2019-06-26 Pablo Calla , Dan Fries , Chris Welch

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…

地球与行星天体物理 · 物理学 2018-12-27 Thomas I. Maindl , Roman Miksch , Birgit Loibnegger

The metal content of asteroids is of great interest, not only for theories of their origins and the evolution of the solar system but, in the case of near-Earth objects (NEOs), also for impact mitigation planning and endeavors in the field…

地球与行星天体物理 · 物理学 2014-03-26 Alan W. Harris , Line Drube

We determine the possible detection rate of asteroids with the Bering mission. In particular we examine the outcome of the Bering mission in relation to the populations of Near-Earth Asteroids and main belt asteroids. This is done by…

天体物理学 · 物理学 2007-05-23 Rene Michelsen , Henning Haack , Anja C. Andersen , John L. Joergensen

We present an updated set of near-Earth asteroids with a Yarkovsky-related semimajor axis drift detected from the orbital fit to the astrometry. We find 87 reliable detections after filtering for the signal-to-noise ratio of the Yarkovsky…

地球与行星天体物理 · 物理学 2018-09-19 Alessio Del Vigna , Laura Faggioli , Andrea Milani , Federica Spoto , Davide Farnocchia , Benoit Carry

The bulk density of an asteroid informs us about its interior structure and composition. To constrain the bulk density one needs an estimate for the mass of the asteroid. The mass is estimated by analyzing an asteroid's gravitational…

地球与行星天体物理 · 物理学 2020-01-15 L. Siltala , M. Granvik

Summary: In the past decade both scientists and laymen have probably heard at least once through the newspapers, TV and Internet that a new asteroid has been discovered with non-zero (sometimes "high") probability of collision with the…

空间物理 · 物理学 2013-04-29 Germano D'Abramo

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…

天体物理学 · 物理学 2007-05-23 Philip R. Bidstrup , Henning Haack , Anja C. Andersen , Rene Michelsen , John Leif Jorgensen

Determining the size and orbital distribution of the population of near-Earth asteroids (NEAs) is the focus of intense research, with the most recent models converging to a population of approximately $1000$ NEAs larger than 1 km and up to…

地球与行星天体物理 · 物理学 2016-12-21 Pasquale Tricarico

A comprehensive characterization of the detection efficiency of nine of the major asteroid surveys that have been active over the past two decades is presented. The detection efficiency is estimated on a nightly basis by comparing the…

地球与行星天体物理 · 物理学 2016-03-16 Pasquale Tricarico

Asteroid mining has been proposed as an approach to complement Earth-based supplies of rare earth metals and supplying resources in space, such as water. However, existing studies on the economic viability of asteroid mining have remained…

空间物理 · 物理学 2018-10-11 Andreas M. Hein , Robert Matheson , Dan Fries

Understanding the dynamical evolution of asteroids through the secular Yarkovsky effect requires the determination of many physical properties, including the rotation period. We propose a method aimed at obtaining a robust determination of…

地球与行星天体物理 · 物理学 2025-01-14 D. E. Vavilov , B. Carry

We present a method for calculating precise distances to asteroids using only two nights of data from a single location --- far too little for an orbit --- by exploiting the angular reflex motion of the asteroids due to Earth's axial…

地球与行星天体物理 · 物理学 2015-10-07 Aren N. Heinze , Stanimir Metchev

We modify the probabilistic formalism developed by Elvis (2014) to estimate the number of lunar craters that contain ore-bearing asteroid remnants. When we consider craters at or above a threshold diameter of 1 km, we estimate an upper…

地球与行星天体物理 · 物理学 2025-08-06 Jayanth Chennamangalam , Paul Brook , Martin Elvis , Samuel Peterson

In this article, theory-based analytical methodologies of astrophysics employed in the modern era are suitably operated alongside a test research-grade telescope to image and determine the orbit of a near-earth asteroid from original…

地球与行星天体物理 · 物理学 2021-09-16 Muhammad Farae , Cameron Woo , Anka Hu

The knowledge of the orbit or the ephemeris uncertainty of asteroid presents a particular interest for various purposes. These quantities are for instance useful for recovering asteroids, for identifying lost asteroids or for planning…

地球与行星天体物理 · 物理学 2015-06-15 Josselin Desmars , David Bancelin , Daniel Hestroffer , William Thuillot

This paper presents a robust linear method for impact probability estimation of near-Earth asteroids with the Earth. This method is a significantly modified and improved method, which uses a special curvilinear coordinate system associated…

地球与行星天体物理 · 物理学 2020-01-08 Dmitrii E. Vavilov
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