Observing planner
What's worth looking at tonight: the Messier and Caldwell objects and some showpiece stars ranked for your place, sky and telescope through the dark hours, each with an altitude chart; the night's cloud, transparency and dew forecast; a saved observing list, a session log you can download, and the Messier marathon's best night and running order.
Added
Works with
- Telescope mount AstronomyPoint a GoTo mount at it sends the target to slew to
How to use it
Choose where you are, the night, how dark your sky is and your telescope’s aperture. The Tonight tab lists 252 objects — all 110 Messier objects, the 109 of the Caldwell catalogue, and some showpiece double stars, coloured stars and clusters — best first. Tap one for its altitude through the night against the twilight and the Moon.
How to use it
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Place is a city, typed latitude and longitude, or your browser’s location — the same place in every astronomy page here (sky tonight, planet details, the mount).
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Night of is the evening’s date; Tonight follows the clock (after midnight it still means the night you are in).
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Sky is a Bortle class or, better, a reading from a Sky Quality Meter in mag/arcsec² (21.9 is as dark as the Earth gets; a suburb is about 19–20; a city centre 17–18) — the sky darkness page converts between them and estimates yours. The page shows the naked-eye limit and the faintest star your telescope will show (2.7 + 5 log D mm, the rule in the optics calculator, moved up or down with your sky).
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Lowest altitude is the horizon you have: trees, houses and murk near the ground.
Each object is rated easy, moderate, hard, very hard or not visible for that sky and aperture at its best moment, then ranked by how high it gets in the dark hours, that rating, and the Moon. Stars and clusters are judged by their brightness against the telescope’s limit; galaxies and nebulae by their surface brightness (magnitude spread over their area) against the sky’s, with a bonus for aperture. The Moon brightens the sky according to its phase, height and distance from the object — near a full moon most galaxies drop out and the clusters and doubles rise to the top. It is a rough guide, made to put the likely things first; a nebula filter, your eyes and the transparency on the night matter as much.
★ adds an object to My list (kept in this browser, sorted by when each is highest; download it as JSON). Log keeps a session log — the object, the time, seen or not, telescope, eyepiece, magnification, seeing and transparency (1–5), the sky and notes — and downloads it as CSV or JSON (and imports a JSON log back). Point a GoTo mount at it hands the object to the telescope mount page.
Forecast asks Open-Meteo for the hours of the night: total, low, mid and high cloud, humidity, temperature, dew point, wind and gusts, with a verdict. High cloud and humidity spoil transparency even when the sky looks clear; when the temperature comes within 2 °C of the dew point your optics will dew up without a heater or a dew shield. Seeing (how steady the air is) is not forecast.
Messier marathon finds the best nights of a spring for seeing all 110 Messier objects in one night — the nights round the new moon of March or early April, each scored by how many objects a running order can catch from your place — and gives that order with times and altitudes: at each moment the object that will be lost soonest, so the galaxies setting in the west at dusk come first (M74, M77) and the globulars rising into the dawn last (M72, M73, M2, M30). Set the minutes per object, the lowest altitude and how dark the sky must be (the Sun 12° down is usual). From much north of 35° some objects are out of reach.
Works in any current browser, on a phone too.
Where the numbers come from
Positions (J2000) are from SIMBAD (CDS, Strasbourg); magnitudes, sizes and names are the values commonly quoted in the Messier and Caldwell lists (public facts; the compilation is mine). Sun and Moon from the site’s astronomy core (Meeus, Astronomical Algorithms, and VSOP87). Surface brightness is the object’s magnitude spread over the ellipse of its quoted size — an average: many galaxies have a bright core and faint arms. The naked-eye limit from a sky reading uses the usual fit to Schaefer’s model; Bortle classes are mapped to typical SQM readings (class 1: 21.95, 4: 21.0, 5: 20.1, 7: 18.7, 9: 17.6).
Privacy
The place, list and log stay in this browser (localStorage). Nothing leaves it until you press Get the forecast: that sends the place’s latitude and longitude, rounded to 0.001°, to Open-Meteo (free, no key, CORS) and nothing else. Your location from the browser is never put in a link.
Feedback is a gift. Something to improve, a feature to add, or a bug? Tell me.
Runs entirely in your browser — network requests go only to the services named on this page.