βValid 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
β Mount position falls outside the building footprint β check your offset measurements.
β Pointing was pulled up to clear the walls/roof/horizon at this azimuth.
β Declination was raised to the lowest value ever observable from this latitude (lat β 90Β°) β anything below that never clears the horizon, at any hour angle.
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.
Sky Coverage
Reading this
Center = zenith, edge = horizon, up = North, right = East. The plot is stretched to your building's actual width/length ratio β a long, narrow building shows as an ellipse, not a circle. Updates live as you change your setup.
β Green β clear of walls, roof, and horizon β Red β blocked by a wall or the parked roof β Brown β below your local (terrain) horizon
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.
Plan View
Wall / Floor / Ceiling Clearance
Telescope-to-Telescope Clearance
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.
Angle is measured from North (0Β°), clockwise β same convention as azimuth. Distance is the perpendicular distance from the building's center out to that wall.
width of the roof structure, for the peaked-roof taper
mm
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
roof height at the sides, where it meets the walls
cm
peak height, running the length of the roll-off travel
cm
The ridge is assumed to run parallel to the roll-off direction β obstruction is higher looking toward the middle of the roof's width and lower looking toward its edges, tapering linearly between ridge and eave.
cm
cm
A single slope from low to high across the roof's width, rather than a symmetric peak β the more common real-world shape for a roll-off roof, since it's simpler to build on rails than a full gable.
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
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.
along the main axis, from the pivot to this scope's mounting point
cm
to the side of the main axis, e.g. on a side-by-side saddle plate
cm
mm
mm
cm
cm
mm
mm
cm
cm
mm
mm
3D Preview
β Clearsβ Blocked
Drag to orbit, scroll to zoom.
Walls β solid up to wall height, the building's actual footprint
Parked roof box β the rolled-off roof's obstruction, past whichever wall it slides beyond
N / E / S / W β cardinal directions at the walls
Small bar β OTA
Amber line β optical axis
Rust-colored skyline β your local (terrain) horizon limit
Blue arc β the celestial equator (Dec=0); genuinely tilts with latitude, crossing the horizon due East and due West
Bright dot β the elevated celestial pole, at altitude = your latitude β where a polar-aligned GEM's RA axis points
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°
Load a horizon .hrz file β the same azimuth/altitude format Stellarium's custom horizon files use (comma or space separated, "#" comment lines ignored; .csv/.txt also accepted) β or paste/edit the points directly below.
4Telescope Pointing
Drives the live obstruction calculation and the 3D preview.
Β°
h
Β°
Β°
Β°
JOG
Step size
Hold to keep jogging. Nudges whichever pointing mode is active above.