The Arecibo Observatory's legacy and future radar capabilities

被引:6
|
作者
Venditti, Flaviane C. F. [1 ]
Marshall, Sean E. [1 ]
Devogele, Maxime [1 ]
Zambrano-Marin, Luisa F. [1 ]
McGilvray, Anna [1 ]
机构
[1] Univ Cent Florida, Planetary Radar, Arecibo Observ, HC 3 BOX 53995, Arecibo, PR 00612 USA
关键词
Near -Earth object (NEO); Radar; Planetary defense; Space debris; SHAPE MODEL; ORBITAL DEBRIS; EARTH;
D O I
10.1016/j.actaastro.2023.05.023
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Ground-based radar systems are critical for physical and dynamical characterization of near-Earth objects (NEOs) and space debris. The operational aspect and applications of radar for planetary defense and space situational/ domain awareness (SSA/SDA) are similar, but there are some factors that should be taken into account for an instrument to support both areas: planetary defense is focused on asteroids and comets in heliocentric orbit with perihelion distance <1.3 au. Special attention is given to potentially hazardous objects (PHOs), which are NEOs larger than 140 m that can come within 0.05 au (similar to 20 lunar distances) of Earth. Radar can quickly and accurately determine NEOs' future trajectory, therefore, the sooner an object can be observed, the safer it is to assess any possible threat. Radar is also useful to help obtaining information about the objects' properties to plan for an impact mitigation mission if needed. For SSA, the focus is artificial objects orbiting Earth. This document presents the radar capabilities of the legacy Arecibo telescope, and explores synergistic future concepts for planetary defense and SSA.
引用
收藏
页码:610 / 615
页数:6
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