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From the Sun to Andromeda at true distances — 3D star map

A map that places the major stars within 2,000 light-years of the Sun at their true three-dimensional positions, so the distances between them become something you can look at.

Stars lifted off the celestial sphere

Looking up at night, every star seems pinned to the inside of one shell. Even the stars that outline a single constellation are, in reality, unrelated to each other and scattered at wildly different distances. This map strips that shell away and puts each star back at the depth it actually occupies. Proxima Centauri, the nearest star of all, and Deneb, far beyond it, sit inside the same volume here, which makes it plain that stars of similar apparent brightness can be nowhere near each other.

Reading distance by turning the map

Drag to rotate the map and, as the direction you are looking from shifts, the front-to-back relationships between stars come out. The moment that matters is when two stars that looked adjacent from one angle spring far apart as soon as you turn. The wheel or a pinch lets you fill the view with the Sun's immediate surroundings or pull back until the full 2,000 light-year range fits, and selecting a star confirms which one sits where. It opens in a browser with nothing to install, and the same rotation works by touch on a phone.

About the distances

Star positions are laid out from measured distance data. Distance measurements are most reliable for nearby stars and grow less certain further out, so the arrangement close to the Sun can be trusted more tightly than the region running from a few hundred out to 2,000 light-years. The point of the map is less to read individual figures than to get a feel for how the distances compare. Where an exact value matters, check it against a published catalogue.

Good ways to use it

When you need to explain why a constellation figure only holds together from Earth's particular vantage point, turning this map once does the work faster than describing it. If the light-year refuses to feel like a real quantity, seeing the gap between the nearest star and a familiar bright one helps it land. Working out which stars are genuinely our neighbours also changes how the night sky reads afterwards. Any star you select here has a fuller entry waiting in the object encyclopedia on this site.

Look it up here

  • How far is Sirius from the Sun, really? 8.6 light-years — it opens with Sirius selected, and the card's distance view puts the Sun and Sirius in one frame with the 8.6-year light-travel gap. Show it here →
  • How many years does light take from the Sun to Betelgeuse? About 640 years — it opens with Betelgeuse selected, and the distance view puts the 640-light-year gap to the Sun in one frame. Show it here →
  • What is the closest star to the Sun? Proxima Centauri is closest at 4.25 light-years, and the 3D map shows the real gap between it and the Sun. Show it here →
  • Which star is the brightest in the night sky? Sirius is the brightest star in the night sky, and tonight's view marks where it stands and how high. Show it here →
  • Is Betelgeuse about to go supernova? It is a red supergiant near the end of its life, bound to explode on no fixed date; the 3D map shows its bulk up close. Show it here →
  • Can I rotate the stars and see their 3D layout? A rotation-only 3D view lets you spin the neighbouring stars to any angle and see which ones lie in front. Show it here →

FAQ

How far out does the map go?

It covers the major stars within 2,000 light-years of the Sun. On the scale of the galaxy that is a small neighbourhood, but most of the bright stars visible to the naked eye fall inside it, so the familiar ones from the night sky are nearly all here.

Are the stars in a constellation close to each other?

Usually not. A constellation is a pattern drawn between stars that merely happen to lie in a similar direction as seen from Earth, so when you rotate the map the members of one constellation often turn out to be separated by enormous gaps in depth.

Where is the closest star to the Sun?

Proxima Centauri sits right beside the Sun. Zoom in on the Sun's surroundings and it turns up immediately; zoom back out until Deneb is in frame and the contrast between the nearest star and a distant one becomes obvious in a single move.

→ Keep reading in the object index → Sky news

NowSky is an educational, conceptual visualization tool; it may differ from actual astronomical phenomena and observational data.

Details

All figures, orbits, surface renderings and event reconstructions (eclipses, probe trajectories, etc.) on this site are approximate, simplified models for education. Timing, positions, scales and appearances may differ from reality. Items marked as targets (e.g. future mission schedules) are hypothetical reference dates.

All information is provided "as is" with no warranty of accuracy, completeness or currency. It must not be used as a basis for any practical decision — observation planning, navigation, research or commercial use — and the operator accepts no liability for any direct or indirect damages arising from its use. For authoritative astronomical data, consult official sources such as NASA, ESA, the IAU, NASA JPL Horizons (precision ephemerides) or the U.S. Naval Observatory.

How the three-dimensional layout is built

Direction on the sky combined with a measured distance, converted to rectangular coordinates.

Details

Each star is placed from its right ascension, declination and catalogue distance. Those distances are measurements, so uncertainty grows with range and the outer part of the map is more approximate than the part near the Sun.

Dot sizes carry brightness and spectral class. They are not physical diameters, which would be far too small to render at this scale.

Data caveats

Distance uncertainty grows with range.

Details

Parallax pins nearby stars to within a few percent, but past a few hundred light-years published values diverge. Hypergiants are the worst case: UY Scuti and Stephenson 2-18 shift by factors with each new distance measurement.

Even the Milky Way's diameter runs anywhere from 100,000 to 200,000 light-years depending on the definition. The 2,000 light-years shown here is a very small piece of it.