MFO-001 | The Pelican Nebula (IC 5070)
- Tom Shankapotomous
- 2 days ago
- 2 min read

Pelican Nebula - IC 5070
Captured: October 23 2025
Location: Massanutten Resort, Virginia — Field Post Alpha (“Mattahausen Ridge”)
Instrument: ZWO Seestar S50 Smart Telescope
Exposure: 281 × 10 s subframes ≈ 47 min total integration
Stack: In-camera stack (Seestar App); raw FITs archived for future Siril/APP re-stack on Linux
Processing: Minimal stretch; no gradient removal or color calibration applied

Target Overview
Object: IC 5070 — The Pelican Nebula
Constellation: Cygnus
Type: Emission (H II) region / stellar nursery
Distance: ≈ 1 ,800 light-years
Angular Size: ≈ 60 × 50 arcmin (~50 ly across)
Associated Objects: NGC 7000 (North America Nebula), Cygnus OB2 association
Dominant Emissions: Hydrogen-α (656 nm), trace O III and S II
Field Narrative
The first deployment of the Mobile Field Observatory was set against the quiet folds of the Shenandoah Valley. From a makeshift clearing near the Mattahausen Resort, the Seestar locked cleanly onto IC 5070 shortly after nautical twilight. Even in the live stack, the nebula’s “beak” and “neck” were visible through light pollution on the eastern horizon.
The resulting stack shows a strong hydrogen signal and excellent structure in the central ionization front. The bright blue-white star near the upper field marks the foreground of Cygnus OB2. Despite the Seestar’s automatic color bias toward red, the image reveals the transition between ionized gas and the dark molecular clouds where new stars form — the true “pelican’s neck.”
Technical Notes
Guiding: Native Seestar tracking — no visible drift over 47 min
Sky Quality: Bortle 4-5; ambient skyglow from Harrisonburg present
Temperature: ≈ 42 °F (6 °C)
Calibration Frames: None (collected light only); darks and flats to be added for Siril processing
Planned Re-process: Linear workflow in Siril with background neutralization, photometric color calibration, and gentle HDR stretch
Target Coordinates: RA 20ʰ 51ᵐ , Dec +44° 25′
Interpretive Notes
IC 5070 is the birthplace of stars. Each crimson fold is plasma recombining after ionization — a slow conversation between radiation and gravity. The light captured here left its source when the Appalachians were still young and icy; it arrived to a portable observatory on a cold Virginia ridge with a battery-powered scope and a steady hand.
Next Steps
Plan two-panel mosaic with adjacent NGC 7000 (North America Nebula) for full region coverage.
Collect Ha/O III data for comparison once Linux workflow is online (MFO-LNX-001).
Evaluate Seestar color bias using photometric calibration test stack under identical conditions.



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