The Potentially Hazardous Asteroid 2000 SG344
Open Astronomy, 2016 We computed impact solutions for the potentially dangerous asteroid 2000 SG344, based on 31 optical observations from 1999 May 15.20482 UTC to 2010 October 29 03.60723 UTC.
Wlodarczyk I.
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The dynamically hazardous asteroid 2025 TV10
Astronomy & AstrophysicsContext. Twenty co-orbital asteroids of Venus are currently known, several of which may evolve into potentially hazardous asteroids (PHAs) over timescales of thousands of years. Aims.
Carruba V., Sfair R., Winter O. C.
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Precise CCD astrometric observations of minor planets and comets at the Belgrade observatory during 1997 [PDF]
Serbian Astronomical Journal, 1998 73 precise astrometric positions of seven comets and two minor planets from MPC critical list - 1093 Freda and 4954 Eric - were obtained with the CCD equipped Askania astrograph (13.5/160) of Belgrade Astronomical Observatory.
Protitch-Benishek V., Benishek Vl.
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Thermal Model Calibration for Minor Planets Observed with Wide-Field Infrared Survey Explorer/Neowise [PDF]
, 2011 With the Wide-field Infrared Survey Explorer (WISE), we have observed over 157,000 minor planets. Included in these are a number of near-Earth objects, main-belt asteroids, and irregular satellites which have well measured physical properties (via radar ...
Bauer, J. +9 more
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Apophis source population and Earth encounter frequency of Apophis-like bodies
Astronomy & AstrophysicsContext. Asteroid (99942) Apophis will safely pass by the Earth in April 2029. This extraordinary event will be observable by the naked eye from Africa and western Europe. Aims.
Brož M. +6 more
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On the Transit Potential of the Planet Orbiting iota Draconis [PDF]
, 2010 Most of the known transiting exoplanets are in short-period orbits, largely due to the bias inherent in detecting planets through the transit technique. However, the eccentricity distribution of the known radial velocity planets results in many of those ...
Bergmann, Christoph +6 more
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Quantifying the Contamination of TESS Ecliptic-plane Light Curves by Minor Planets
The Astronomical JournalThough missions devoted to time series photometry focus primarily on targets far beyond the solar system, their observations can be contaminated by foreground minor planets, especially near the ecliptic plane, where solar system objects are most ...
Ben Cassese +8 more
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Integrated photogrammetry and photoclinometry for enhanced 3D surface reconstruction of asteroids
Astronomy & AstrophysicsStereo photogrammetry (SPG) and stereo photoclinometry (SPC) are the main techniques used in the 3D surface reconstruction of asteroids. The SPG approach retrieves accurate 3D geometry with limited spatial resolution, while SPC extracts fine-scale ...
Li Hongliang +8 more
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DIGITAL ARCHIVE OF UKRVO: THE POSITIONAL ACCURACY OF MINOR PLANETS DETERMINATIONS
Odessa Astronomical Publications, 2013 Scanning and astrometric processing of two 30x30 cm photographic plates with images of minor planets were conducted. The plates were obtained at the double wide-angle astrograph (DWAA, 400/2000) on the program of photographic sky survey and the program ...
V. Golovnya, V. Andruk
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Study of ephemeris accuracy of the minor planets [PDF]
The current state of minor planet ephemerides was assessed, and the means for providing and updating these emphemerides for use by both the mission planner and the astronomer were developed.
Brooks, D. R., Cunningham, L. E.
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