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Calcimator

Star Party Planner Calculator

Plan a star party by estimating sunset time, moon phase, visible planets, and observable deep-sky objects for your location and date.

About this calculator

This calculator estimates star-party planning conditions from three inputs -- Month, Latitude, and Bortle Class -- using simplified seasonal approximations rather than a precise ephemeris. Est. Sunset (24h) is a smoothed seasonal model (a sine-wave approximation of day length by month and latitude) -- verified across the full declared grid (every month at latitude -60 to 70), its own reachable range is roughly 16:03 to 19:57 local time, so treat it as a rough seasonal estimate, not a precise sunset time; it does not know your longitude, time zone, or elevation, and it cannot represent real high-latitude effects like a much later summer sunset or, above the Arctic/Antarctic Circle, no sunset at all. Moon Illumination has no year input to anchor a real calendar date, so instead of chasing an unreachable "real date" it spreads the 12 calendar months evenly across one illustrative 29.53-day lunar cycle -- deliberately covering the full range of possible conditions across a year (some months near-new/dark, some near-full/bright), not the actual moon phase on any specific real date; check a real lunar calendar before planning around a new moon.

Visible Planets reports a fixed, typical estimate rather than a month-keyed table, because naked-eye planet visibility is set by each planet's own synodic period (116 to 780 days) -- none commensurate with the calendar year -- so there is no real month-to-count relationship to source. Observable DSOs (deep-sky objects) scales a sky-darkness-based catalog count down sharply as Bortle Class rises (worse light pollution hides fainter objects), then scales that by the real geometric fraction of the celestial sphere visible from your Latitude over a full year, (1 + cos(latitude)) / 2 -- highest at the equator, lowest near the poles. This is a geometric visibility estimate, not one tuned to any specific catalog's declination distribution -- the widely-used Messier catalog was itself compiled largely from Northern-hemisphere (49°N) observations, so it skews toward northern declinations in a way this model does not correct for, and it treats Northern and Southern latitudes of the same magnitude identically. Month has no effect on Observable DSOs in this model, since Month only feeds the sunset, moon-phase, and visible-planets estimates.

Inputs

Results

Observable DSOs

64

Est. Sunset (24h)19:07
Moon Illumination26%
Visible Planets3
How to Use This Calculator
  1. Select Month, enter Latitude (°N), and select your Bortle Class (light-pollution level).
  2. Review the Observable DSOs result.
  3. Use Est. Sunset (24h) and Moon Illumination (%) to inform your decision.
  4. Use the chart to visualize the results and explore different scenarios by adjusting inputs.

How the result changes with Latitude (°N)

Latitude (°N)Observable DSOs
2070
3067
6054
7048

What each input means

Month
Month of the planned observing session
Latitude (°N)
Your geographic latitude (positive = north, negative = south)
Bortle Class
Light pollution level on the Bortle Dark-Sky Scale

How this is calculated

Worked example, using the default values

  1. Identify Input Parameters
    3 parameters
    Month (1-12) = 6, Latitude (°N) = 40, Bortle Class (1-9) = 4 = 3 input(s) provided
  2. Calculate Est. Sunset
    Est. Sunset
    19:07 = 19:07
  3. Calculate Moon Illumination
    Moon Illumination
    26 = 26

Engine last updated . Checked against 3 independently-derived tests — how we verify calculators. Built by Paul Gunder, a software engineer, not a licensed financial, medical, or legal professional.

Frequently Asked Questions

Does Moon Illumination reflect the actual moon phase on a specific date?

No. There is no year input, so instead of guessing at a specific year this calculator spreads the 12 calendar months evenly across one illustrative lunar cycle -- deliberately showing the full range from near-new to near-full moon across the year, not the real illumination on any specific calendar date. Before scheduling a star party around a new moon, check a real lunar calendar or astronomy app for the actual date you're planning.

Why doesn't changing Month move Observable DSOs?

Because Observable DSOs is built entirely from Bortle Class and Latitude in this model -- it represents how many deep-sky objects are bright enough to see through your sky's light pollution and geometrically above your horizon, neither of which this calculator ties to time of year. Month only feeds Est. Sunset (24h), Moon Illumination, and Visible Planets.

Why does raising Bortle Class lower Observable DSOs so sharply?

Because light pollution is the single biggest limiter of how many deep-sky objects are visible, and it dominates this calculator's Observable DSOs estimate more than Latitude does -- each step up the Bortle scale (1 = excellent dark-sky site, 9 = inner-city sky) washes out progressively fainter galaxies, nebulae, and star clusters from view, so the count falls steadily from a pristine-sky estimate down toward a city-sky floor.

Is Est. Sunset (24h) accurate enough to plan an exact start time?

Treat it as a rough seasonal estimate, not a precise sunset time. Across the full declared range of Month and Latitude, this model's own output never moves outside roughly 16:03 to 19:57 -- it doesn't account for your exact longitude, elevation, or time zone, and at high latitudes (roughly above 60°) in summer, real sunset can be much later than this model shows, or -- above the Arctic/Antarctic Circle -- may not happen at all. For scheduling an actual event, verify the real sunset and end-of-astronomical-twilight times with a dedicated sunset calculator or astronomy app for your specific coordinates and date.

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