Breakthrough capability for the NASA Astrophysics Explorer Program: Reaching the darkest sky
M.A. Greenhouse, S.W. Benson, R.D. Falck, D.J. Fixsen, J.P. Gardner,, J.B. Garvin, J.W. Kruk, S.R. Oleson, H.A. Thronson

TL;DR
This paper proposes a new mission architecture using Solar Electric Propulsion with Falcon 9 to significantly enhance the science capabilities of NASA's Astrophysics Explorer missions by enabling access to extra-Zodiacal orbit.
Contribution
It introduces a novel launch augmentation approach with SEP technology to increase sensitivity and observing speed without larger telescopes, expanding mission potential.
Findings
SEP stage technology is TRL-6 ready for Explorer missions.
Enabling extra-zodiacal orbit access increases sensitivity by ~13X.
The approach offers a cost-effective alternative to larger systems.
Abstract
We describe a mission architecture designed to substantially increase the science capability of the NASA Science Mission Directorate (SMD) Astrophysics Explorer Program for all AO proposers working within the near-UV to far-infrared spectrum. We have demonstrated that augmentation of Falcon 9 Explorer launch services with a 13 kW Solar Electric Propulsion (SEP) stage can deliver a 700 kg science observatory payload to extra-Zodiacal orbit. This new capability enables up to ~13X increased photometric sensitivity and ~160X increased observing speed relative to a Sun-Earth L2, Earth-trailing, or Earth orbit with no increase in telescope aperture. All enabling SEP stage technologies for this launch service augmentation have reached sufficient readiness (TRL-6) for Explorer Program application in conjunction with the Falcon 9. We demonstrate that enabling Astrophysics Explorers to reach…
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