Diagram showing two possible lowest RMS orbit fits for 2018 AG37 depending on the argument of perihelion (ω) given by JPL-SBDB and Project Pluto. JPL-SBDB's solution gives ω=251° corresponding to 2018 AG37 moving away from the Sun and approaching aphelion (Q), while Project Pluto's solution gives ω=225° corresponding to 2018 AG37 having passed aphelion (Q) as moving toward the Sun. Positions shown as of 1 January 2021 (JD 2459215.5).
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