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University of Florida

SST org page for the University of Florida (UF), Gainesville, FL.

Last updated: 2026-04-14 (session 18)


SST Footprint

Project PI Period TRL Outcome
93925 CHOMPTT β€” Precision Time Transfer John W. Conklin 2015–2020 4β†’9 flew (Dec 2018, Rocket Lab ELaNa XIX)
94153 MOCT β€” Pulse Modulator for Optical Crosslinks John W. Conklin 2016–2018 3β†’4 transitioned (β†’ CLICK optical comms domain)

Both SST projects share the same PI (Conklin) and the same lab (Precision Space Systems Lab). CHOMPTT is the only TRL 9 project in the entire 111-project SST portfolio. MOCT (Miniature Optical Communications Transceiver) developed a pulse-position modulator for CubeSat laser crosslinks β€” same technology domain as MIT's CLICK.

Other UF PI: Norman Fitz-Coy was PI on the LaRC-led Precision ADCS project 106813 (TRL 3β†’5, 2013–2015), which led to SwampSat β€” the first CubeSat to fly control moment gyroscopes (CMGs) in orbit. Fitz-Coy is not the lead org PI but UF was a key contributor.


John W. Conklin β€” People Chain

The most consequential SST-to-flagship people chain in the portfolio.

Background

  • Cornell BS/MEng β†’ Stanford PhD (2009, Hansen Experimental Physics Lab) β†’ Stanford postdoc (3 years) β†’ UF faculty 2012
  • Research focus: precision instruments for Position, Navigation, Timing, and Gravity (PNTG)

SST Phase (2015–2020)

CHOMPTT (93925) demonstrated the first on-orbit measurement of chip-scale atomic clock (CSAC) performance. Key results: - Launched Dec 16, 2018 on Rocket Lab Electron (ELaNa XIX) into 500 km, 85Β° orbit - 3U CubeSat bus built by NASA Ames, 1U OPTI instrument built by UF PSSL - CSACs performed 3Γ— better than manufacturer spec (100 ps Allan deviation over 1 s vs. 300 ps spec) - First-ever on-orbit CSAC Allan deviation measurement achieved - Attempted laser time-transfer to three satellite laser ranging (SLR) facilities - Published: Advances in Space Research (2023), SmallSat 2017, SmallSat 2019 - Confidence: confirmed (NTRS 20190027323, peer-reviewed results in Adv. Space Res.)

MOCT (94153) advanced a software-defined pulse modulator for optical crosslinks using differential pulse-position modulation (DPPM). TRL 3β†’4 in 2 years. The optical crosslink concept connects to the broader CLICK/DORA/OCSD optical comms thread in SST, though no direct project lineage confirmed.

Post-SST Trajectory

Conklin's SST work proved he could design, build, and fly precision timing instruments on CubeSat budgets. His subsequent trajectory:

Project Program Period TRL Role
91511 Deep-space laser comms (DPPM) STRG 2014–2018 2β†’3 PI
23546 Gravitational wave inertial sensors RTF (SMD) 2015–2017 β€” PI
96406 Earth geodesy constellation instruments IIP (SMD) 2020–2022 2β†’3 PI
LISA Charge Management Device (CMD) NASA contract 2020+ β€” PI
5+ additional TechPort projects Various β€” β€” PI/Co-I

LISA CMD: $12.58M contract β€” Conklin is PI for NASA's Charge Management Device for the Laser Interferometer Space Antenna (LISA), a flagship ESA/NASA gravitational wave observatory launching mid-2030s. The CMD uses ultraviolet LEDs and fiber optics to control electric charge on free-floating test masses β€” the same core competency in precision sensing that CHOMPTT demonstrated at CubeSat scale.

Institutional influence: Chair of NASA Physics of the Cosmos Program Analysis Group. Vice-Chair of NASA Astrophysics Advisory Committee.

The Arc

CHOMPTT (SST, ~$1M) β†’ LISA CMD ($12.58M) represents a ~12Γ— funding escalation from CubeSat demo to flagship mission hardware, enabled by the same precision sensing competency. SST gave Conklin his first flight-proven instrument; LISA CMD is the mature version of that same capability applied to a $2B+ mission. This may be the highest-ROI SST investment in the portfolio when measured by downstream mission scale. Confidence: confirmed (UF press releases, NASA contract award, TechPort records).


Norman Fitz-Coy β€” Secondary People Chain

Fitz-Coy was PI on SST precision ADCS 106813 (LaRC-led), developing star trackers and CMGs for CubeSat attitude control. This work transitioned to SwampSat, the first CubeSat to demonstrate CMGs in orbit.

Fitz-Coy and Conklin are both in UF MAE β€” a 2014 UF article features both under "NASA grants" for small satellite technology. UF had two simultaneous SST-funded lines: Conklin (precision timing/sensing) and Fitz-Coy (precision pointing). Both succeeded. Confidence: confirmed (SwampSat flight, UF press).


Collaborators

  • NASA Ames Research Center β€” Built CHOMPTT 3U bus. Roger Hunter (ARC) was SST Program Manager on both CHOMPTT and MOCT.
  • Air Force Research Laboratory β€” Listed as "Other Organization" on CHOMPTT. AFRL has interest in precision timing for PNT.
  • JPL β€” Co-Is on Conklin's IIP geodesy project [96406] (Klipstein, Ziemer, Spero, Wiese). JPL precision instruments community.

Publications

  • Advances in Space Research (2023): "Laser time-transfer facility and preliminary results from the CHOMPTT CubeSat mission" β€” peer-reviewed flight results
  • SmallSat Conference (2017, 2019): CHOMPTT concept-to-launch and preliminary results
  • NTRS 20190027323: Conference abstract on CHOMPTT evolution
  • Multiple LISA/CMD publications in astrophysics journals (post-SST)

Cross-References


Key Takeaway

UF is the SST portfolio's CubeSat-to-flagship bridge. Conklin's CHOMPTT (only TRL 9) demonstrated that CubeSat-scale precision instruments could meet flagship-grade requirements. The CHOMPTT→LISA CMD arc — from a $1M CubeSat demo to a $12.58M contract on a $2B+ observatory — is the clearest example in the SST portfolio of a university PI leveraging SST as a stepping stone to major mission hardware. Combined with Fitz-Coy's SwampSat CMGs, UF produced two independent SST-funded technology transitions through two independent people chains.