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Distribution of the near-earth objects

Solar System Research, 2011
This paper analyzes the distribution of the orbits of near-Earth minor bodies from the data on more than 7500 objects. The distribution of large near-Earth objects (NEOs) with absolute magnitudes of H < 18 is generally consistent with the earlier predictions (Bottke et al., 2002; Stuart, 2003), although we have revealed a previously undetected maximum ...
Boris Shustov   +2 more
openaire   +2 more sources

INEO—Imaging of near-Earth objects

Acta Astronautica, 1994
Abstract INEO is a program of four explorer flyby missions for imaging near-Earth objects by means of small spin stabilized spacecrafts. A low-cost approach is achieved by using existing hardware and available scientific instrumentation. For the first mission the payload consists of the flight space model of the Halley multicolour camera and three ...
Iglseder, H. (1)   +13 more
openaire   +3 more sources

Near-Earth Objects

2014
Asteroids and comets probably contributed significantly to the delivery of water and organic materials to the early Earth necessary for the development of life. However, later impacts of near-Earth objects almost certainly played a role in mass extinctions and evolution.
Alan W. Harris   +3 more
openaire   +2 more sources

Physical characterization of the near-Earth object population

The European Physical Journal Plus, 2017
The Near-Earth Object (NEO) population, being the remnants of the building blocks that originally formed our solar system, allows us to understand the initial conditions that were present in the protosolar nebula. Its investigation can provide crucial information on the origin and early evolution of the solar system, and shed light on the delivery of ...
Ieva, S.   +5 more
openaire   +3 more sources

The population of near-Earth objects discovered by Spacewatch [PDF]

open access: possibleEarth, Moon, and Planets, 1996
In the past three years the Spacewatch program at the University of Arizona’s Lunar and Planetary Laboratory has discovered ~45% of the new Earth Approaching asteroids and found evidence for an unheralded population of small (~10m) objects in the inner solar system.
Tom Gehrels, Robert Jedicke
openaire   +1 more source

Near-Earth Objects

2017
The chances of a random piece of rock striking Earth still exists, but probably to a much reduced level of threat. During the early years in the creation of our Solar System, there was plenty of debris that had yet to settle into some form and order, with constant collisions of large bodies before any structure was imposed.
openaire   +2 more sources

The debiased compositional distribution of Near-Earth Objects

2022
&lt;p&gt;We report 491 new near-infrared spectroscopic measurements of 420 Near-Earth Objects (NEOs) collected on NASA&amp;#8217;s IRTF in the context of MITHNEOS (PI: DeMeo). The measurements were combined with previously published data (Binzel et al.
Michaël Marsset   +12 more
openaire   +1 more source

Impacting small Near Earth Objects

Advances in Space Research, 2008
Abstract The design of a low-cost spacecraft to impact on a small, faint Near Earth Object (NEO), poses major challenges. This paper focuses on the terminal phase of such impact mission, analyzing the capability of autonomous Guidance, Navigation and Control (GNC) systems to compensate the deviations in the impact point to achieve a successful ...
J. Gil-Fernández, C. Corral, R. Panzeca
openaire   +2 more sources

Near Earth object mitigation studies

2016 IEEE Aerospace Conference, 2016
Early detection of an object on a collision course with Earth, leading to well-considered and effective measures to mitigate its hazards, is not always possible due to a number of extenuating factors. NASA and the Department of Energy (DOE)'s National Nuclear Security Administration (NNSA) have partnered to develop a full systems framework for ...
Mark Boslough   +6 more
openaire   +2 more sources

Binary Asteroids in the Near-Earth Object Population

Science, 2002
Radar images of near-Earth asteroid 2000 DP107 show that it is composed of an ∼800-meter-diameter primary and an ∼300-meter-diameter secondary revolving around their common center of mass. The orbital period of 1.755 ± 0.007 days and semimajor axis of 2620 ± 160 meters constrain the total mass of the system to 4.6 ± 0.5 × 10 11
Margot, J. L.   +7 more
openaire   +3 more sources

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