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Observatory Calibration Worksheet

Roll-Off-Roof Observatory β†’ Sky Coverage & Horizon Planner

βœ“ Valid pointing β€” clear of the walls, roof, and local horizon.
Building & Roof Summary
Footprintβ€”
Wall Heightβ€”
Roof Travelβ€”
Roll-off Directionβ€”
Mount Offsetβ€”
Live Pointing
Telescope points atβ€”
Obstruction Limit Hereβ€”
Clearance Marginβ€”
Blocked Byβ€”

Sky Coverage

Sweeps a grid across the whole sky and checks whether each point clears the walls, the parked roof, and your local horizon β€” not a dome shutter, since a roll-off roof either fully opens or fully closes.

Swing Clearance

The whole assembly is rigid and rotates about the mount's pivot β€” so each telescope's farthest point stays a fixed distance from that pivot no matter which way it's pointed. Plan view (looking straight down): the building outline to scale, with one circle per telescope at its actual swing radius against the walls, floor, and ceiling. Circles are spread apart by each telescope's lateral position on the mount so they're readable as separate telescopes, rather than stacked on one exact point β€” the radius (not the exact placement shown) is what the wall-clearance check actually uses. A separate check below catches telescopes hitting each other, which wall clearance alone can't.

1Building & Mount Position

Measured from the building's true geometric center on the floor (not magnetic north). Positive North offset means the mount is closer to the North wall.

cm
cm
cm
cm
positive = North of center
cm
positive = East of center
cm

Building Shape

Most buildings are a simple rectangle β€” the width/length above cover that. Non-rectangular buildings (angled corners, an extension, an irregular footprint) can be described directly as up to 6 walls, each its own distance and angle from center.

2Roll-Off Roof

The roof rolls off past one wall and parks there β€” that parked structure is its own obstruction, not just an open gap.

how far the roof slides past that wall
cm
usually close to wall height; taller if on a raised track
cm

3Optical Axis Offset

Mount type changes the OTA's swing in the 3D preview and how pier side affects it. Doesn't change the wall/roof obstruction math itself β€” that's driven purely by true Alt/Az.

RA axis to OTA aperture center
cm
mm
mm

Telescopes

Telescope 1 uses the OTA length/aperture and GEM Axis / Dec Offset entered above. Enable up to 3 more for additional scopes riding along (guide scope, wide-field rig, etc.) β€” each with its own offset along the main axis and lateral offset to the side, for both wall clearance and scope-to-scope clearance. See the Swing Clearance panel at the bottom of the page.

3D Preview

● Clears ● Blocked

Drag to orbit, scroll to zoom.

Local Horizon

Terrain beyond the building β€” trees, other structures. Layered on top of the wall/roof obstruction; whichever blocks more at a given azimuth wins.

Β°

4Telescope Pointing

Drives the live obstruction calculation and the 3D preview.

Β°
h
Β°
JOG
Step size
Hold to keep jogging. Nudges whichever pointing mode is active above.