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Sky42
Version 1.2 Free

A real sky, drawn from real catalogues.

Sky42 is a scientifically rigorous desktop planetarium for Windows and macOS, drawing over a billion Gaia stars down to magnitude 20, nearly a million galaxies, and every minor planet and comet the Minor Planet Center catalogues. Version 1.2 adds a sky with sunsets and twilight in it, a photographed Moon, photographs of ten thousand galaxies and nebulae from the great Schmidt telescopes, and five thousand years of Sun, Moon and planets — back to the evening Aristotle watched the Moon cover Mars.

1.06 billion Gaia DR3 stars, to G 20
971,205 HYPERLEDA galaxies
Every MPC minor planet & comet
JPL ephemerides, 22 moons
~16,000 working satellites
147,529 double star pairs
Sky42 looking south-southwest from Padova at dusk: a dark blue sky fading to an orange band on the horizon, with the crescent Moon beside Saturn, Venus below them, and Fomalhaut low in the south
Dusk from Padova on 4 January 2025, the Sun ten degrees down: the crescent Moon beside Saturn, Venus below, and only the brightest stars out yet. An hour later the Moon covers Saturn — that picture is further down.
Sky42 1.2 is here. Freeware for non-commercial use — no account, no subscription, no license key. See the terms for what non-commercial means and how the data licenses travel with it.

The sky as it looks, tonight and in 357 BC

Version 1.0 put the catalogues on the chart. Version 1.2 puts the air, the Moon's face and the centuries around them. Seven chapters, each with the picture Sky42 drew for it.

01  Simulator

A sky with a horizon, a sunset and a twilight in it

The Sky brightness button now has two modes. Atlas is the chart you knew: one colour for the whole sky. Simulator paints the sky as the air does — lighter towards the horizon, a glow round the Sun, the orange band of sunset under the blue, and the Earth's shadow rising in the east once the Sun is down.

The air also takes its share of what shines through it. Stars low in the sky fade and turn orange, and the faint ones go; the Sun and the Moon turn yellow and then orange as they set. The Milky Way, now filled with a faint glow inside its outlines, fades under the Moon or a city sky and is gone by twilight, as the real one is.

The simulated sky at sunset from Venice: the Sun on a straight horizon in an orange glow, fading through pale pink to blue higher up
Sunset from Venice on 7 October 2026, looking west-southwest: the Sun on the horizon, the glow round it, and the blue coming back higher up.
02  The Moon

A photographed Moon, and the planets that go behind it

The Moon is drawn from a photograph of its ground, turned the way it really faces you: the seas, the highlands and the rays of Tycho are where they are, and the seas show in the earthshine of a crescent too. Its panel gives the libration, which tells which edge is showing a little of the far side tonight.

When the Moon passes in front of a planet or a star, that is what you see. The planet fades as the edge covers it, is gone while it is behind, and comes back at the other edge. The Almanac lists these occultations as seen from your place — when each begins and ends, at the dark or the bright edge, and how high the Moon stands.

A crescent Moon with its night side lit by earthshine, and Saturn with its moon Titan just off the dark edge
The same evening as the picture at the top, 18:36 in Padova: two minutes before Saturn, with Titan beside it, goes behind the dark edge of the Moon.
03  Ancient skies

Five thousand years, and an evening Aristotle wrote down

The date field now goes back to 3000 BC. With JPL's DE441 from the Catalogue Manager, the Sun, the Moon and the planets go there too, with their eclipses, conjunctions and occultations in the Almanac. The slow swing of the Earth's axis and the slowing of its rotation follow models made for millennia, and dates before 1582 are in the Julian calendar, as history books write them.

In On the Heavens Aristotle says he saw the half Moon pass in front of Mars, which vanished at the dark edge and came out at the bright one. Set Sky42 to Athens on 4 May 357 BC, the date historians give for it, and it is there: a Moon half a day short of first quarter, Mars gone at the dark edge at 19:53 and back at the bright one at 21:10.

Those times say how far they may be off. Nobody timed the Earth's rotation in 357 BC, so Sky42 writes 19:53 ±6 min — and an hour it cannot vouch for to the minute is not printed as if it could.

3000 BCwhere the Sun, Moon and planets now begin
±6 minstated beside every time in Aristotle's century
The Sky42 window set to 4 May 357 BC in Athens: the half Moon with Mars at its dark edge, and the date field reading minus 0356, 357 BC
Athens, 4 May 357 BC, a few minutes before Mars goes behind the dark edge. The date field reads −0356, the year as astronomers count it, with 357 BC beside it.
The Sky42 almanac for Athens in May 357 BC, listing Mars disappearing behind the Moon at 19:53 plus or minus 6 minutes and reappearing at 21:10
The Almanac for that month: Mars disappears at the dark limb and reappears at the bright one, every time with its ±6 minutes.
04  Double & variable stars

Where the companion is tonight, and when the star dims next

Select a double star — or a bright one such as Castor — and Orbit… draws the companion's path round the primary, where it is on the date of the sky, and its position angle and separation for the years ahead. The orbits are the published ones, and Update keeps them current.

For a variable, Light curve… shows the curve the Hipparcos satellite measured, where the star is in its cycle tonight, and the next minima or maxima of the stars that keep time — with a plain warning that the real times can run early or late, because periods change.

3,459orbits of visual binaries
12,500variables with a measured light curve
The Sky42 orbit window for the double star STF 1937 AB: an ellipse with the companion marked, and a table of position angle and separation for coming years
η Coronae Borealis, a 41.6-year orbit: the companion in October 2026, and where it will be each year after.
The Sky42 light curve window for Algol: the folded curve with its deep minimum, a line at tonight's phase, and a list of the next minima
Algol, from 57 Hipparcos measures: the dashed line is tonight, and the list gives its next minima.
05  Eclipses & transits

Eclipses that darken the sky, and a Moon that turns red

The Almanac lists the eclipses of the Moon and of the Sun and the transits of Mercury and Venus, with the time of every stage, how deep each one goes, and how high the Moon or the Sun stands where you are. Double-click one and the sky goes there and stays locked on it, so you can step through the whole event without it leaving the field.

On the chart they look the part: the Moon turns dark brick red as the Earth's shadow crosses it, the daytime sky drops to a deep blue in a total eclipse of the Sun and the planets come out, and Mercury and Venus cross the Sun as black dots.

The Moon half inside the Earth's shadow, brick red on one side and still sunlit on the other, among the stars
The lunar eclipse of 7 September 2025 from Padova, half an hour before totality: the shadow on one side, sunlight still on the other.
06  Images

Your photographs, laid exactly where they belong

Open a plate-solved FITS — or a PNG or TIFF with the file its solver wrote — and Sky42 lays it on the sky in its true place, size and orientation. Drag a file onto the window and it is there. The catalogue stars sit on the stars of the picture, and the chart goes on around it: names, symbols, grids, the tracks of moving bodies.

Each image has its own black point, midtones, white point and opacity, and a button that sets the clock to when it was taken, so that the asteroids and comets in the frame can be named. Where two images overlap, the brighter one shows at each point, so a mosaic stays a mosaic.

Add a folder once, and every solved picture in it and its subfolders appears when you look that way — a few at a time, and never more than the computer can hold. The Images button hides and shows them all, to compare a photograph with the chart.

FITS, PNG, TIFFwith the solution they carry or the one beside them
0.05″a pixel in the Hubble frames shown here
Three overlapping Hubble frames of the spiral galaxy NGC 3621 laid on the Sky42 chart, inside the catalogue ellipse of the galaxy, with catalogue stars drawn over the stars of the photograph
Three Hubble frames of NGC 3621 on the chart, in a 12′ field: the galaxy's catalogue ellipse round them, and Gaia's stars on the stars of the photograph. Data: NASA/ESA Hubble Space Telescope, programme 17189 (PI Thilker), 28 December 2023.
07  Deep-sky photographs

What the galaxy on the chart looks like through a great telescope

Press X and the galaxies, nebulae and globular clusters of the NGC and IC catalogues get a black-and-white photograph, laid exactly in place, from the Digitized Sky Survey: the scanned glass plates of the great Schmidt telescopes at Palomar and Siding Spring. For each object Sky42 picks the red or the blue plate, whichever shows it better.

A photograph appears as you zoom in far enough for it to be worth seeing, and the chart's own stars and names stay on top of it. Under a bright sky it fades the way the faint light of a real galaxy would: dimmer under the Moon, gone in twilight and daylight.

Sky42 comes with the photographs of the Messier objects. All the others are one download from the Catalogue Manager.

10,526galaxies, nebulae and globular clusters photographed
76Messier objects included with Sky42
The galaxies M81 and M82 in Ursa Major on the Sky42 chart, each with its black-and-white photograph laid in place among the chart's stars: the spiral arms of M81 below, the edge-on M82 above, and NGC 3077 in the corner
M81 and M82 in Ursa Major, in a 1.3° field, with NGC 3077 in the corner. Digitized Sky Survey — Provenance: Data taken by ROE and AAO, CalTech, Compression and distribution by Space Telescope Science Institute. Copyright: STScI, ROE, AAO, UK-PPARC, CalTech, National Geographic Society. Full copyright notice.

Also in 1.2

Asteroids in other centuries

The six thousand asteroids that can reach magnitude 15 are drawn where they really were in any year from 1600 to 2500 — and for a single year, a small file adds a hundred and fifty thousand down to magnitude 18. On the day Giordano Bruno died, 17 February 1600, Vesta was a sixth-magnitude point in Leo.

A starting view that looks like the sky

Sky42 opens facing south over a straight horizon, 60° wide, with the ground, the deep sky and the Milky Way on. The first time, it places you in the largest town of your computer's time zone until you choose your own place.

Time that runs both ways

Play, pause, faster and slower, from real time to a year a second — forwards or backwards. The toolbar shows the Julian Date beside the local time, and typing into any of the three moves the other two.

Turn the field, or mirror it

Drag with the right mouse button to turn the chart to any angle, to match a photograph or the eyepiece, and mirror it for a star diagonal. Reset View brings back the standard one when you are lost.

More in the Object panel

When the object rises, culminates and sets, the best time to observe it in a dark sky, its airmass and what the air takes from its brightness, its distance from the Moon, and the constellation it is in.

A search box that takes more

Type a position instead of a name, a Greek letter written out — zeta Her, alf CMa — or a town in your own language when choosing your site: Venezia finds Venice, and 北京 finds Beijing.

Every star Gaia measured to magnitude 20. Every galaxy in HYPERLEDA. Every minor planet the MPC knows.

Not a selection and not a sample: Sky42 draws the complete catalogues, on your own computer, with no connection needed once they are downloaded.

1.06billion
stars, from Gaia DR3
1,060,293,402: every Gaia DR3 source brighter than G 20 — the archive's own count, star for star — each with its parallax, proper motion and colour.
971,205
galaxies, from HYPERLEDA
Nearly a million galaxies beneath the Messier, NGC and IC objects, named on the chart as you zoom in while there is room.
~1.6million
minor planets and comets
Every object the Minor Planet Center catalogues, refreshed from its files whenever you ask — the count grows every day.

What's on the chart

Every layer below is built from a named, cited catalogue — not a texture or an approximation.

Gaia DR3

Over a billion stars, complete to magnitude 20

The star field is ESA's Gaia Data Release 3, down to G = 20: 1,060,293,402 stars, each with its position, parallax, proper motion and colour. The count isn't estimated — it matches the Gaia archive's own count for G < 20, star for star. Click any of them and the inspector gives you its Gaia identifier, G magnitude, BP−RP colour, distance and proper motion.

  • Split into magnitude tiers, so you download only the depth you need: the whole sky to G 9 is 11 MB, the full depth to G 20 about 64 GB. The catalogue manager fetches each tier when you ask for it, and a download that is interrupted picks up where it stopped.
  • The packs are read straight from disk, not copied into memory: a 3.6′ field in a crowded part of the Milky Way, down to magnitude 17.5, draws 1,327 stars in 0.25 ms.
Gaia DR3G < 20Parallax & proper motionTiered download
Sky42 showing a 3-degree Gaia DR3 star field in Cygnus
Gaia DR3 in a 3° field in Cygnus — about 2,700 stars down to magnitude 11.8, coloured by their BP−RP index.
Deep sky

The Messier, NGC and IC objects, and 971,205 galaxies underneath them

The deep sky is two layers, drawn as chart symbols: OpenNGC's Messier, NGC and IC objects, and HYPERLEDA's galaxies below them. Conspicuous nebulae also show their traced shape — 238 closed outlines over 171 objects from OpenNGC, drawn where a ring is at least twelve pixels across, because the catalogue ellipse that suits a galaxy is a circle around a filament for the Veil.

OpenNGCHYPERLEDA I238 traced outlines
Sky42 zoomed into the Andromeda Galaxy showing M31, M32 and M110 with OpenNGC ellipses and the equatorial grid
Deep sky at 3° — M31, M32 and M110 drawn from OpenNGC, with the equatorial grid for scale.
Solar system

The Sun, the Moon, the planets and 22 of their moons, from JPL

Named on the chart and readable in the inspector with their magnitude, elongation, phase angle and light time. Twenty-two moons, from Phobos and Deimos to Triton, are placed from JPL's satellite ephemerides, and each planet is drawn at its own centre rather than its system's. A moon behind its planet or in its shadow is not drawn, so the eclipses and occultations of the Galilean moons happen on screen when they happen in the sky.

  • Zoomed in, Jupiter shows its dark belts and the Great Red Spot, and Saturn its rings in front of and behind the globe, both flattened and turned as they are in the sky.
  • The standard DE440s covers 1849–2150. The catalogue manager can add JPL DE440 for 1550–2650, and DE441 for 3000 BC to 1850. Outside the ephemeris, Sky42 draws no bodies and says why, rather than extrapolating.
DE440s / DE44022 moonsEclipses & occultationsLight time
Sky42 showing Saturn with its rings and the moons Enceladus, Tethys, Dione, Rhea, Titan and Hyperion in a 5.4-arcminute field
Saturn a week before its opposition of October 2026 — the rings open, and the moons from Enceladus out to Titan and Hyperion.
Sky42 showing Jupiter with Io, Europa, Ganymede and Callisto in a 12-arcminute field
Jupiter and the four Galilean moons at a 12′ field, placed from JPL's satellite ephemerides.
Sky & site

A sky that brightens with twilight and the Moon, and hides what it hides

With sky brightness on, the sky turns from night to twilight blue to a deep daytime blue as the Sun rises, and glows around the Moon — wide under a full Moon, barely there under a crescent. A bright sky also hides the faint stars, as it does outside: fewer under a city sky or a full Moon, only the brightest at dusk, none by day.

  • The observer's site has a Bortle scale, from an excellent dark site to an inner-city sky. You can save the places you observe from under a name, with their elevation, time zone and sky.
  • Sky brightness has two modes: Atlas, one colour for the whole chart, and Simulator, with the horizon, the Sun's glow and the colours of twilight.
TwilightMoonlightBortle scaleSaved sites
Sky42 looking south-east from Padova the evening after a full Moon, with the sky glowing blue around the Moon and Saturn beside it
Sky brightness — the evening after the full Moon of 26 September 2026: the sky glows around the Moon, with Saturn beside it, and only the brighter stars are left.
Stars & constellations

88 constellation boundaries, and figures that join real stars

The 88 constellation boundaries are drawn from Delporte's B1875 definition, sampled as the curves they are. The naked eye stars come from the Bright Star Catalogue with their proper names and Bayer designations — Gaia does not have the bright stars, twelve of the fourteen brightest in the sky are absent from it — and the constellation figures join those stars rather than tracing coordinates.

  • The Milky Way is drawn as the outline of its band, three lines from its bright core to its faint edge, with the Magellanic Clouds, and filled with a faint glow that is strongest at the core. The contours are traced from a map of Gaia's own stars, and follow the dust lanes of Cygnus and Sagittarius.
Bright Star CatalogueDelporte B1875d3-celestial figuresMilky Way outline
Sky42 looking east-southeast from Padova on a January evening: Orion, Gemini and Canis Major above the horizon, Jupiter and Mars rising in Leo
A January evening from Padova, looking east-southeast: Orion, Gemini and Canis Major, with Jupiter rising in Leo.
Sky42 looking south on an August evening: Sagittarius and Scorpius above the horizon with the outline of the Milky Way
The Milky Way outline over Sagittarius and Scorpius on an August evening, with the dust lanes rising towards Aquila.
Double & variable stars

147,529 double star pairs and 60,416 variables, filtered your way

A window lists the doubles from the Washington Double Star Catalog by separation, magnitudes and their difference, and the variables from the GCVS by how bright they get, how much they vary, their period and their kind. The table sorts on every column, and a double-click takes the sky there. The stars that pass the filters are marked on the chart and named: two strokes turned towards the companion, or a ring.

  • Both can be found by name in the search box: STF 2758, WDS 18443+3940, R Leo, delta Cep.
  • A star found by name is centred where it is today, not where it was in 2000: fast-moving stars like Barnard's star no longer end up off the middle of a narrow view.
WDSGCVS 5.1Position angle
Sky42 showing Lyra in a 12-degree field with double stars marked by strokes and variable stars by rings, all named
Lyra at 12° — double stars marked by two strokes turned towards the companion, variables by a ring, each one named.
The Sky42 double and variable stars window, listing doubles between 2 and 5 arcseconds apart
Double and variable stars — doubles between 2″ and 5″, sorted by separation; double-click a row to go there.
Minor planets

Every minor planet the MPC catalogues, propagated the way the field of view asks for

Minor planets use MPCORB elements, conservative light-time/parallax screening, H-G photometry and an inspector showing orbital epoch and quality. The default --asteroid-dynamics auto uses fast two-body propagation on wide charts and switches to perturbed ASSIST/IAS15 trajectories when the whole viewport falls below one square degree; kepler and assist remain explicit overrides.

  • The Object panel shows an asteroid's or a comet's orbit: semi-major axis, eccentricity, inclination, perihelion and aphelion, period, and the Tisserand parameter that tells a comet-like orbit from an asteroid-like one.
  • Asteroids and comets are drawn at the size of a star of the same magnitude, so the magnitude legend applies to them too, and their names fade with them.
MPCORBH-G photometryASSIST / IAS15
Sky42 showing numbered minor planets in Libra labelled against the star field
Minor planets in Libra — Proserpina, Frigga, Egeria and their neighbours, placed from MPCORB elements for the chosen date.
Tracks

The path of a planet, an asteroid or a comet among the stars

Draw where a moving body goes over days or months, as seen from your place — Mars's backward loop included — marked with its time every minute, hour, day or month, as you choose or as the zoom suggests. Tracks are computed once and drawn like fixed stars, so moving through time does not recompute them.

TopocentricRetrograde loopsTime marks
Sky42 showing the retrograde loop of Mars in Leo from November 2026 to June 2027, with monthly marks, Jupiter and the Moon
Tracks — Mars's backward loop in Leo around its opposition of February 2027, marked on the first of each month.
Artificial satellites

About 16,000 working satellites, where they are from your place

Satellites are drawn where they are as seen from your site, and only while the Sun lights them, so what is on the chart is what could be seen. Their orbits are downloaded fresh from CelesTrak when you switch them on. Going back in time, a satellite appears only after its launch, and for the last thirty days each one is placed with the orbits of that day.

CelesTrakSGP4Earth's shadow
Sky42 looking west-northwest an hour after sunset, with the ISS near the horizon and sunlit Starlink satellites among the stars
Artificial satellites an hour after sunset — the ISS low in the west and the Starlinks still in sunlight, each where it is as seen from your place.
Almanac

The night ahead, and the months after it

For any day and place: sunrise and sunset, moonrise and moonset, the three twilights, the Moon's phase and the days left to the next equinox or solstice. For the months ahead: the Moon's phases, oppositions, the greatest elongations of Mercury and Venus with their best evening or morning from where you are, and the Moon and planets passing close to each other, to Uranus, Neptune, the Pleiades or a bright star near their path.

  • The Moon's close passes are worked out as seen from your place, where they can be up to a degree closer or farther than from the centre of the Earth, and the almanac says how high the Moon is.
  • Double-click an event to set the sky to that moment, turned to that planet.
Rise & setConjunctionsOppositionsElongations
The Sky42 almanac for Padova on 28 September 2026, with rise and set times, twilights and the events of the coming months
The almanac — the Sun and Moon for one day and place, and the months ahead: phases, oppositions, elongations and close passes.

And behind every view

Navigation & rendering

Continuous pan and zoom, from all-sky to telescopic

Four projections, configurable time and observer, live coordinates under the cursor, and a frame counter that keeps the frame cost honest as catalogues grow. Click a star or a deep sky object to select it and read it in the inspector; search finds it by name.

  • Switchable equatorial and altazimuth grids over a drawn horizon, with the ground filled in below it and the cardinal points named on it.
  • Preferences set the star size from 50% to 300%, how many names the chart writes, and how far down the screen the straight horizon sits. Names stay put while you pan, and a larger window shows more of them.
  • Two rasterisers behind one seam: OpenGL where a 3.3 Core context can be had, NumPy and QImage where it cannot. The choice is automatic, --renderer overrides it, and the status bar says which one is drawing.
4 projectionsStar size & name densityOpenGL / CPU fallback
Coordinate systems

Astrometric, apparent, and observed — three coherent modes

The chart representation covers astrometric ICRS, apparent CIRS of date, and observed place including atmospheric refraction. A separate readout selector lets the cursor and inspector use a different system — for example, an observed chart with catalogue-comparable ICRS right ascension and declination. Apparent CIRS remains the chart default; ICRS remains the numeric default.

ICRSCIRSRefraction
Comets

One universal-variable solver, no threshold on eccentricity

Comets come from the MPC's CometEls with the same observed-place chain, but a solver and a photometry of their own: one universal-variable conic covers the ellipses, the 244 near-parabolic orbits, and the hyperbolic ones. Brightness follows the MPC's M1/K1 total-magnitude model rather than the asteroids' H-G phase law. A comet with no published photometry is drawn and says its magnitude is unknown, instead of silently disappearing.

  • Comae and tails are drawn at the size observers actually report, measured on 37,596 COBS observations, and a comet's predicted brightness agrees with JPL's.
CometElsM1/K1 photometry
Search & selection

Search covers all of it — and says so when a name is ambiguous

The deep sky, the naked eye stars by proper name, Bayer, Flamsteed, HR, HD and HIP, every minor planet by number, name or provisional designation, and the comets. When a name belongs to more than one object — Halley is a minor planet and a comet — the matches are listed instead of counted. Whatever is selected is marked on the chart by four ticks around it, even when it is too faint for the field to draw it: the ticks say the thing is here, without putting a light where there is none.

Cross-catalogue searchSelection reticle
Staying current

Orbital elements refresh atomically, and the app checks itself

Orbital elements can be refreshed from the toolbar or the command line: Sky42 asks the Minor Planet Center whether its files are newer than yours, downloads and rebuilds on a worker thread, and replaces each pack atomically — a cancelled or failed update leaves the previous catalogue byte for byte as it was. The ⋯ menu holds what isn't a layer: the ephemeris table, About Sky42, and Check for Updates, which asks the Sky42 site whether a newer version has been published. Sky42 downloads and installs nothing — the button opens the download page. The same check runs silently at most once a week and speaks only when there's something to say.

  • With minor planets or comets on, Sky42 tells you once when their orbits are more than a month old, and offers to update them. The reminder can be turned off.
  • A user manual comes with the app: press F1, and in a dialog F1 opens it at the section about that window. Preferences can also show a small log of what Sky42 opened, downloaded or could not find.
Atomic replaceWeekly, silent checkBuilt-in manual (F1)

Every layer is a cited source

Attribution travels with the data: every catalogue Sky42 downloads arrives with its own ATTRIBUTION.txt beside it, carrying the credit and the citation its authors ask for.

Stars — Gaia DR3 European Space Agency mission Gaia, processed by the Gaia Data Processing and Analysis Consortium (DPAC). Gaia Collaboration, Prusti et al., A&A 595, A1, 2016; Vallenari et al., A&A 674, A1, 2023. CC BY-NC 3.0 IGO · Credit: ESA/Gaia/DPAC
Deep sky — OpenNGC By Mattia Verga. The nebula outlines are OpenNGC's own too, traced by hand over DSS2 Color imagery with Aladin at CDS Strasbourg. CC-BY-SA-4.0
Galaxies — HYPERLEDA I Paturel et al., A&A 412, 45, 2003, via VizieR VII/237. Asks to be cited rather than licensed. Citation requested
More deep sky — via VizieR Barnard's 349 dark nebulae (1927, VizieR VII/220A); Sharpless's HII regions (ApJS 4, 257, 1959, VizieR VII/20); open clusters from Dias et al. (A&A 389, 871, 2002, v3.5, VizieR B/ocl). Citation requested
Constellation boundaries VizieR VI/49 (Davenhall & Leggett, Royal Observatory Edinburgh, 1989), from the boundaries E. Delporte fixed for the IAU in 1930.
Bright stars Bright Star Catalogue, 5th Rev. Ed. (Hoffleit & Warren, 1991, VizieR V/50); Hipparcos cross-index (Kostjuk, 2002, VizieR IV/27A); proper names from the IAU Catalog of Star Names. CC-BY (names)
Constellation figures — d3-celestial By Olaf Frohn. Chosen over Stellarium's after measuring both: 743 segments against 844, the same 88 constellations, no share-alike on the data. BSD-3-Clause
Ephemeris — JPL DE440s Park, Folkner, Williams & Boggs, AJ 161:105, 2021. Produced by the Jet Propulsion Laboratory; covers 1849–2150.
Minor planets & comets MPCORB and CometEls from the Minor Planet Center, a service of the IAU hosted by the Smithsonian Astrophysical Observatory. MPC use guidelines
Ancient ephemeris — JPL DE441 The part of DE441 from 3000 BC to 1850, cut out unchanged. Park, Folkner, Williams & Boggs, AJ 161:105, 2021; Jet Propulsion Laboratory, California Institute of Technology.
The Earth's rotation in the past Stephenson, Morrison & Hohenkerk, Measurement of the Earth's rotation: 720 BC to AD 2015, Proc. R. Soc. A 472, 2016, from ancient eclipses and timed occultations. CC BY 4.0
The Moon's face — NASA SVS CGI Moon Kit, NASA's Scientific Visualization Studio, from the LROC Wide Angle Camera mosaic (NASA / GSFC / Arizona State University). Credit: NASA's Scientific Visualization Studio
Deep-sky photographs — Digitized Sky Survey Provenance: Data taken by ROE and AAO, CalTech, Compression and distribution by Space Telescope Science Institute. Copyright: STScI, ROE, AAO, UK-PPARC, CalTech, National Geographic Society. Full copyright notice. Free for non-commercial use with this credit
Binary star orbits — ORB6 Sixth Catalog of Orbits of Visual Binary Stars, Matson, Williams, Hartkopf & Mason, U.S. Naval Observatory.
Light curves — Hipparcos Hipparcos Epoch Photometry Annex (ESA 1997, SP-1200, VizieR I/239); eclipsing binary elements from Kreiner, Acta Astronomica 54, 207, 2004.
Observing places 2,690 MPC observatory codes; 34,140 GeoNames cities15000 towns with IANA time zones; Natural Earth 1:110m coastlines. CC-BY-4.0 / public domain
Natural satellites — JPL/NAIF Satellite ephemerides by R. A. Jacobson and collaborators, Jet Propulsion Laboratory, California Institute of Technology, refitted for Sky42.
Artificial satellites — CelesTrak General perturbations elements of the active satellites, from CelesTrak, downloaded when the layer is switched on and propagated with SGP4.
Double stars — WDS The Washington Visual Double Star Catalog, Mason et al., AJ 122, 3466, 2001, maintained at the U.S. Naval Observatory; via VizieR B/wds. Citation requested
Variable stars — GCVS 5.1 General Catalogue of Variable Stars, Samus et al., Astronomy Reports 61, 80, 2017, Sternberg Astronomical Institute; via VizieR B/gcvs. Citation requested
Milky Way — NASA SVS Contours traced from the Deep Star Maps 2020 Milky Way background of the NASA/Goddard Space Flight Center Scientific Visualization Studio, from Gaia DR2 (ESA/Gaia/DPAC). CC BY-NC 3.0 IGO

Drag, wheel, click — and a key per layer

Drag to pan, wheel to zoom on the cursor, click to select, double click to centre, arrow keys to step.

Solar systemP
Minor planetsM
CometsK
SatellitesS
Milky WayW
Deep sky objectsD
Nebula outlinesO
FiguresF
Constellation boundariesB
Named naked eye starsN
Double stars2
Variable starsV
Sky brightnessL
HorizonH
GroundG
Alt-az gridA
Equatorial gridE
EclipticC
ZenithZ
All namesT
Your imagesI
Deep-sky photosX
Play / pauseSpace
Lock on objectCtrl+K
Reset viewCtrl+0
Night modeCtrl+N
User manualF1

Release history

Sky42 1.0 is the first public release. From here on, every version is listed with what it adds, changes and fixes.

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Free, standalone, and yours to keep

Sky42 1.0 is freeware for non-commercial use — for Windows and macOS, no account, no subscription, and nothing that stops working when you're offline.

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Version 1.0.0  ·  Windows & macOS