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Asteroid photometry has three major applications: providing clues about asteroid surface physical properties and compositions, facilitating photometric corrections, and helping design and plan ground-based and spacecraft observations. The…

地球与行星天体物理 · 物理学 2016-08-31 Jian-Yang Li , Paul Helfenstein , Bonnie J. Buratti , Driss Takir , Beth Ellen Clark

We summarize the comet science provided by surveys. This includes surveys where the detections of comets are an advantageous benefit but were not part of the survey\'s original intent, as well as some pointed surveys where comet science was…

地球与行星天体物理 · 物理学 2022-10-19 J. M. Bauer , Y. R. Fernández , S. Protopapa , L. M. Woodney

Large-area surveys operating at mid-infrared wavelengths have proven to be a valuable means of discovering and characterizing minor planets. Through the use of radiometric models, it is possible to derive physical properties such as…

地球与行星天体物理 · 物理学 2016-08-31 A. Mainzer , F. Usui , D. Trilling

We performed a statistical analysis of the astrometric errors for the major asteroid surveys. We analyzed the astrometric residuals as a function of observation epoch, observed brightness and rate of motion, finding that astrometric errors…

地球与行星天体物理 · 物理学 2017-06-28 Peter Vereš , Davide Farnocchia , Steven R. Chesley , Alan B. Chamberlin

Studies on Near Earth Asteroids (NEAs) throw light on discoveries, identification, orbit prediction and civil alert capabilities, including potential asteroid impact hazards. Due to various new observational programs, the discovery rate of…

地球与行星天体物理 · 物理学 2016-07-21 J. Rukmini , G. Raghavendra , S. A. Ahmed , D. Shanti Priya , Syeda Azeem Unnisa

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

Asteroids detection is a very important research field that received increased attention in the last couple of decades. Some major surveys have their own dedicated people, equipment and detection applications, so they are discovering Near…

天体物理仪器与方法 · 物理学 2019-01-10 D. Copandean , C. Nandra , D. Gorgan , O. Vaduvescu

Collisions are one of the key processes shaping planetary systems. Asteroid families are outcomes of such collisions still identifiable across our solar system. The families provide a unique view of catastrophic disruption phenomena and…

地球与行星天体物理 · 物理学 2022-07-25 Bojan Novakovic , David Vokrouhlicky , Federica Spoto , David Nesvorny

Modern astronomical surveys detect asteroids by linking together their appearances across multiple images taken over time. This approach faces limitations in detecting faint asteroids and handling the computational complexity of trajectory…

地球与行星天体物理 · 物理学 2025-09-25 Nathan Golovich , Trevor Steil , Alex Geringer-Sameth , Keita Iwabuchi , Ryan Dozier , Roger Pearce

Looking ahead to the next decade and imagining the landscape of astronomy in 2020, it is clear that astronomical surveys, large and small, plus extensive follow-up projects, will be a great engine of progress in our profession. Surveys have…

宇宙学与河外天体物理 · 物理学 2009-04-20 Steven T. Myers

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

Asteroids are an indelible part of most astronomical surveys though only a few surveys are dedicated to their detection. Over the years, high cadence microlensing surveys have amassed several terabytes of data while scanning primarily the…

地球与行星天体物理 · 物理学 2023-02-03 Preeti Cowan , Ian A. Bond , Napoleon H. Reyes

Mean motion resonances play a fundamental role in the dynamics of the small bodies of the Solar System. The last decades of the 20th century gave us a detailed description of the dynamics as well as the process of capture of small bodies in…

地球与行星天体物理 · 物理学 2018-06-06 Tabare Gallardo

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…

地球与行星天体物理 · 物理学 2009-06-25 Kevin J. Walsh , Patrick Michel , Derek C. Richardson

We have performed a simulation of a next generation sky survey's (Pan-STARRS 1) efficiency for detecting Earth-impacting asteroids. The steady-state sky-plane distribution of the impactors long before impact is concentrated towards small…

地球与行星天体物理 · 物理学 2011-03-31 Peter Vereš , Robert Jedicke , Richard Wainscoat , Mikael Granvik , Steve Chesley , Shinsuke Abe , Larry Denneau , Tommy Grav

Wide-angle surveys have been an engine for new discoveries throughout the modern history of astronomy, and have been among the most highly cited and scientifically productive observing facilities in recent years. This trend is likely to…

Large and publicly available astronomical archives open up new possibilities to search and study Solar System objects. However, advanced techniques are required to deal with the large amounts of data. These unbiased surveys can be used to…

The regolith-covered surfaces of asteroids preserve records of geophysical processes that have occurred both at their surfaces and sometimes also in their interiors. As a result of the unique micro-gravity environment that these bodies…

地球与行星天体物理 · 物理学 2016-08-31 Naomi Murdoch , Paul Sanchez , Stephen R. Schwartz , Hideaki Miyamoto

I review the status of science with wide field surveys. For many decades surveys have been the backbone of astronomy, and the main engine of discovery, as we have mapped the sky at every possible wavelength. Surveys are an efficient use of…

天体物理学 · 物理学 2009-11-13 A. Lawrence

Asteroids can be considered as sources of contamination of point sources and also sources of confusion noise, depending whether their presence is detected in the image or their flux is under the detection limit. We estimate that at low…

天体物理仪器与方法 · 物理学 2015-05-13 Gy. M. Szabo , A. E. Simon
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