Probing the Dark Solar System: Detecting Binary Asteroids with a Space-Based Interferometric Asteroid Explorer
Andrew G. Sullivan, Do\u{g}a Veske, Zsuzsa M\'arka, Imre Bartos,, Szabolcs M\'arka

TL;DR
This paper explores the potential of space-based gravitational wave interferometers to detect binary asteroids within our solar system, proposing specialized instruments and analyzing their feasibility and scientific value.
Contribution
It introduces the concept of using gravitational wave interferometry for binary asteroid detection and proposes specific interferometer configurations tailored for this purpose.
Findings
LISA has negligible sensitivity to binary asteroid signals.
Proposed interferometers with 4.6 AU and 1 AU arms could detect binary asteroids.
Detection requires technological advancements beyond current proposals.
Abstract
With the inception of gravitational wave astronomy, astrophysical studies using interferometric techniques have begun to probe previously unknown parts of the universe. In this work, we investigate the potential of a new interferometric experiment to study a unique group of gravitationally interacting sources within our solar system: binary asteroids. We present the first study into binary asteroid detection via gravitational signals. We identify the interferometer sensitivity necessary for detecting a population of binary asteroids in the asteroid belt. We find that the space-based gravitational wave detector LISA will have negligible ability to detect these sources as these signals will be well below the LISA noise curve. Consequently, we propose a 4.6 AU and a 1 AU arm-length interferometers specialized for binary asteroid detection, targeting frequencies between and…
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