Discovering Earth's transient moons with the Large Synoptic Survey Telescope
Grigori Fedorets, Mikael Granvik, R. Lynne Jones, Mario Juri\'c,, Robert Jedicke

TL;DR
This paper evaluates the potential for the Large Synoptic Survey Telescope (LSST) to discover Earth's transient moons (TCOs), predicting detection rates and discussing methods to improve discovery efficiency.
Contribution
It provides a detailed simulation-based assessment of LSST's capability to detect TCOs and proposes enhancements to increase discovery rates.
Findings
LSST can detect a TCO approximately once per year with current systems.
Development of specialized tools could increase TCO discovery to once every two months.
Detected TCOs will have apparent magnitudes between 21 and 23, with velocities from 1°/day to 50°/day.
Abstract
Earth's temporarily-captured orbiters (TCOs) are a sub-population of near-Earth objects (NEOs). TCOs can provide constraints for NEO population models in the 1--10-metre-diameter range, and they are outstanding targets for in situ exploration of asteroids due to a low requirement on . So far there has only been a single serendipitous discovery of a TCO. Here we assess in detail the possibility of their discovery with the upcoming Large Synoptic Survey Telescope (LSST), previously identified as the primary facility for such discoveries. We simulated observations of TCOs by combining a synthetic TCO population with an LSST survey simulation. We then assessed the detection rates, detection linking and orbit computation, and sources for confusion. Typical velocities of detectable TCOs will range from 1/day to 50/day, and typical apparent magnitudes from 21…
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