Weather, Moon, and darkness
Check whether tonight is worth setting up and what the Moon will do to the sky.
Practical calculators and planners for observing, telescope decisions, astrophotography, sky events, and mission tracking. Use the quick path below or go straight into the optical calculators.
Check whether tonight is worth setting up and what the Moon will do to the sky.
Use optical measurements and practical tradeoffs before brand or affiliate links enter the decision.
Work through camera framing, sampling, battery runtime, and fixed-tripod shutter-speed planning.
Follow launches, mission events, eclipses, Moon phases, and the major dates worth saving.
Choosing a profile fills matching telescope, eyepiece, and camera fields below. Nothing changes until you select a profile.
Telescope focal length ÷ eyepiece focal length, adjusted for the Barlow.
Bright, comfortable low-to-medium power.
A practical estimate using apparent field ÷ magnification.
Telescope focal length ÷ aperture.
A theoretical double-star resolving limit. Atmospheric seeing often becomes the real limit first.
Roughly a 7 mm exit pupil at the low end and 2× aperture in millimeters at the high end. Seeing and optics matter.
See how telescope focal length, camera pixel size, sensor dimensions, and reducers or Barlows change sampling and framing before you assemble the imaging train.
Calculated from effective focal length and pixel size.
Includes the selected reducer or Barlow factor.
Width × height. Actual framing can vary slightly with the optical train and usable sensor area.
This is a moderate image scale that can suit many deep-sky setups. Seeing, guiding, focus, optical quality, and target size still determine whether it is a good match.
Approx. frame width
Approx. 3° span vs. width
Approx. 1° span vs. width
The atmosphere, optical quality, target brightness, collimation, thermal stability, and your own eyes can matter more than the theoretical maximum. A lower-power view that is sharp, bright, and steady is often more useful than a larger but soft image.
Useful for matching an eyepiece to planets, the Moon, double stars, clusters, and deep-sky objects.
A quick way to understand image brightness. Large exit pupils favor bright wide-field views; very small ones get dim fast.
Helps estimate how much sky fits in the eyepiece, especially useful for large clusters, nebulae, and star hopping.
Save private telescope, eyepiece, camera, sensor, and battery profiles with calculated setup metrics.
Plain-English observing, optics, imaging, universe, spaceflight, and space-weather terminology with practical context.
Upcoming solar and lunar eclipses, countdowns, NASA maps, and safe-viewing guidance.
Plan around lunar phase, illumination, moonrise, moonset, and dark-sky windows.
Peak nights, parent objects, moonlight context, observing guidance, and calendar downloads.
Save a date, location note, targets, equipment, and session goal, then add the plan to your calendar.
Track all 110 classic Messier targets with local progress, milestones, filters, and CSV export.
Learn 50 maria, craters, mountains, valleys, rilles, scarps, and unusual lunar surface features.
Keep a private observing history with search, print, CSV export, and restorable backup.
Compare NPF and 500-rule shutter-speed estimates for fixed-tripod night-sky photography.
Estimate battery runtime from mount, camera, dew-heater, computer, and accessory loads.
Visualize how popular deep-sky targets fit different camera sensors and focal lengths.
Compare magnification, exit pupil, and true field across an entire eyepiece set.
Compare aperture, focal ratio, resolution, magnification, weight, and price side by side.
Launches, mission events, and Moon phases in one chronological view.
Moon timing and observing context for tonight.
Solar activity and geomagnetic conditions from official sources.
Upcoming launches, mission events, countdowns, and official webcasts.
StarStation's long-term Gear Lab model is simple: explain the optical tradeoffs first, then recommend equipment only when it solves a real observing problem.