Convert and calculate astronomical distances in light-years (\(\text{ly}\)), kilometers (\(\text{km}\)), miles (\(\text{mi}\)), astronomical units (\(\text{AU}\)), and parsecs (\(\text{pc}\)). Compute speed of light travel times, lookback epochs, and relativistic interstellar spacecraft flight durations with Lorentz time dilation (\(\gamma\)).
Input any distance unit to convert and simulate relativistic flight times.
40.17 Trillion km • 1.302 Parsecs
| 🌟 Light-Years (\(\text{ly}\)) | 4.2465 ly |
| 📐 Kilometers (\(\text{km}\)) | 4.017 × 10¹³ km |
| 🇺🇸 Miles (\(\text{mi}\)) | 2.496 × 10¹³ mi |
| 🪐 Astronomical Units (\(\text{AU}\)) | 268,553 AU |
| 🌌 Parsecs (\(\text{pc}\)) | 1.3020 pc |
| ⏱️ Light Travel Duration | 4.25 Years |
| 🌍 Earth Frame Flight Time | 21.23 Years |
| 🚀 Astronaut Proper Time (\(\tau\)) | 20.80 Years |
A light-year (\(\text{ly}\)) is a fundamental unit of astronomical length defined by the International Astronomical Union (IAU) as the exact physical distance traversed by electromagnetic radiation (light) traveling in an unperturbed vacuum during one Julian year (\(365.25\,\text{days}\) or \(31,557,600\,\text{seconds}\)).
Comparative scale from planetary orbits to deep extragalactic superclusters.
| Celestial Landmark | Distance (Light-Time / ly) | Kilometers (km) | Astronomical Units (AU) | Parsecs (pc) | Voyager 1 Flight Time |
|---|---|---|---|---|---|
| The Moon | \(1.28\,\text{Light-Seconds}\) | \(384,400\,\text{km}\) | \(0.00257\,\text{AU}\) | \(1.25 \times 10^{-8}\,\text{pc}\) | \(6.28\,\text{Hours}\) |
| The Sun | \(8.32\,\text{Light-Minutes}\) | \(1.496 \times 10^8\,\text{km}\) | \(1.000\,\text{AU}\) | \(4.85 \times 10^{-6}\,\text{pc}\) | \(101.8\,\text{Days}\) |
| Voyager 1 Probe | \(22.5\,\text{Light-Hours}\) | \(2.43 \times 10^{10}\,\text{km}\) | \(\sim 163\,\text{AU}\) | \(7.90 \times 10^{-4}\,\text{pc}\) | \(47\,\text{Years (Elapsed)}\) |
| Proxima Centauri | \(4.2465\,\text{ly}\) | \(4.017 \times 10^{13}\,\text{km}\) | \(268,553\,\text{AU}\) | \(1.302\,\text{pc}\) | \(74,900\,\text{Years}\) |
| Sirius A | \(8.611\,\text{ly}\) | \(8.147 \times 10^{13}\,\text{km}\) | \(544,570\,\text{AU}\) | \(2.640\,\text{pc}\) | \(151,900\,\text{Years}\) |
| Milky Way Center (Sgr A*) | \(26,670\,\text{ly}\) | \(2.523 \times 10^{17}\,\text{km}\) | \(1.686 \times 10^9\,\text{AU}\) | \(8,177\,\text{pc}\) (\(8.18\,\text{kpc}\)) | \(470.5\,\text{Million Years}\) |
| Andromeda Galaxy (M31) | \(2.537 \times 10^6\,\text{ly}\) | \(2.400 \times 10^{19}\,\text{km}\) | \(1.604 \times 10^{11}\,\text{AU}\) | \(778,000\,\text{pc}\) (\(778\,\text{kpc}\)) | \(44.7\,\text{Billion Years}\) |
| Observable Universe Radius | \(46.5 \times 10^9\,\text{ly}\) | \(4.40 \times 10^{23}\,\text{km}\) | \(2.94 \times 10^{15}\,\text{AU}\) | \(14.26 \times 10^9\,\text{pc}\) (\(14.26\,\text{Gpc}\)) | \(8.19 \times 10^{14}\,\text{Years}\) |
\(1\,\text{AU} = 149.6\,\text{Million km}\). The gold standard for measuring planetary orbits, asteroid belts, and interplanetary spacecraft paths within stellar systems.
\(1\,\text{ly} = 63,241\,\text{AU}\). The most intuitive metric for interstellar distances, galactic scales, and public scientific communication.
\(1\,\text{pc} = 3.262\,\text{ly}\). The preferred geometric unit among professional astronomers, directly linked to parallax angle measurements (\(d = 1/p\)).
Because the speed of light is finite (\(c \approx 300,000\,\text{km/s}\)), every astronomical observation is inherently a look into the past. When you look at an object \(D\) light-years away, you are seeing it as it existed exactly \(D\) years ago:
Light from the Sun left \(8.3\,\text{minutes}\) ago. Light from Proxima Centauri is \(4.25\,\text{years}\) old. Light reaching our eyes tonight from the Andromeda Galaxy (\(2.54\,\text{million light-years}\) away) embarked during the early Pleistocene epoch, before early humans walked the Earth!
The James Webb Space Telescope observes primordial galaxies at \(z > 14\) whose light has traveled for over \(13.5\,\text{billion years}\), allowing scientists to witness the direct formation of the very first generation of stars and supermassive black holes.
Under Special Relativity, an astronaut traveling at velocity \(v = \beta c\) experiences time dilation governed by the Lorentz factor \(\gamma = 1/\sqrt{1-\beta^2}\): $$\tau_{\text{ship}} = \frac{t_{\text{Earth}}}{\gamma} = \frac{d}{v} \sqrt{1 - \left(\frac{v}{c}\right)^2}$$ At \(v = 0.999\,c\) (\(\gamma \approx 22.36\)), a journey to the center of the Milky Way (\(26,670\,\text{light-years}\)) takes \(26,697\,\text{years}\) in Earth frame, but only \(1,194\,\text{years}\) for crew onboard!
Accelerating a \(1,000\,\text{kg}\) spacecraft to \(90\%\) of light speed (\(\gamma = 2.294\)) requires \((\gamma - 1)mc^2 \approx 1.16 \times 10^{20}\,\text{Joules}\) of energy—equivalent to the annual electrical energy consumption of the entire planet Earth.
Authoritative answers to common questions about light-years, cosmic distances, speed of light travel times, and relativistic interstellar physics.