Light Year to Foot Converter

Convert light years to feet with our free online length converter.

Quick Answer

1 Light Year = 3.104003e+16 feet

Formula: Light Year × conversion factor = Foot

Use the calculator below for instant, accurate conversions.

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All conversion formulas on UnitsConverter.io have been verified against NIST (National Institute of Standards and Technology) guidelines and international SI standards. Our calculations are accurate to 10 decimal places for standard conversions and use arbitrary precision arithmetic for astronomical units.

Last verified: February 2026Reviewed by: Sam Mathew, Software Engineer

Light Year to Foot Calculator

How to Use the Light Year to Foot Calculator:

  1. Enter the value you want to convert in the 'From' field (Light Year).
  2. The converted value in Foot will appear automatically in the 'To' field.
  3. Use the dropdown menus to select different units within the Length category.
  4. Click the swap button (⇌) to reverse the conversion direction.
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How to Convert Light Year to Foot: Step-by-Step Guide

Converting Light Year to Foot involves multiplying the value by a specific conversion factor, as shown in the formula below.

Formula:

1 Light Year = 3.1040e+16 feet

Example Calculation:

Convert 10 light years: 10 × 3.1040e+16 = 3.1040e+17 feet

Disclaimer: For Reference Only

These conversion results are provided for informational purposes only. While we strive for accuracy, we make no guarantees regarding the precision of these results, especially for conversions involving extremely large or small numbers which may be subject to the inherent limitations of standard computer floating-point arithmetic.

Not for professional use. Results should be verified before use in any critical application. View our Terms of Service for more information.

What is a Light Year and a Foot?

1 light-year = 9,460,730,472,580,800 meters (EXACT)

The light-year is a unit of length in astronomy, defined as the distance light travels in one Julian year (exactly 365.25 days) in a vacuum. It is derived from:

1 light-year = (speed of light) × (1 Julian year)
1 ly = 299,792,458 m/s × 31,557,600 seconds
1 ly = 9,460,730,472,580,800 meters

Light-Year is Distance, Not Time

Common misconception: "Light-year measures time."

Reality: The light-year measures distance, using time as a reference.

Analogy:

  • "New York is 3 hours from Boston" (3 hours of driving ≈ 180 miles)
  • "Proxima Centauri is 4.24 years from Earth" (4.24 years of light travel ≈ 40 trillion km)

Both use time to describe distance, but they measure space, not duration.

Why Use Light-Years Instead of Kilometers?

Scale problem: Interstellar distances in kilometers are incomprehensible:

  • Proxima Centauri: 40,208,000,000,000 km (40.2 trillion km)
  • Andromeda Galaxy: 23,740,000,000,000,000,000 km (23.7 quintillion km)

Light-years make it intuitive:

  • Proxima Centauri: 4.24 ly (4 years of light travel)
  • Andromeda Galaxy: 2.5 million ly (we see it as it was 2.5 million years ago)

The "lookback time" advantage: Light-years automatically tell you when you're seeing an object. "100 light-years away" = "seeing it 100 years in the past."

Speed of Light: The Universal Constant

The light-year depends on the speed of light (c), one of nature's fundamental constants:

c = 299,792,458 meters per second (EXACT)

Key properties:

  • Nothing with mass can travel at or exceed c
  • Light travels at c in a vacuum, regardless of observer's motion (Einstein's relativity)
  • c is the same in all reference frames (no "absolute rest" in the universe)

Scale:

  • c = 299,792 km/s (~300,000 km/s)
  • In 1 second: Light circles Earth 7.5 times
  • In 1 minute: Light travels 18 million km (Earth to Sun in 8 min 19 sec)
  • In 1 year: Light travels 9.46 trillion km (1 light-year)

Light-Year vs. Parsec vs. Astronomical Unit

Three distance units for different astronomical scales:

| Unit | Meters | Use Case | |----------|-----------|--------------| | Astronomical Unit (AU) | 1.496 × 10¹¹ m (150M km) | Solar System (planets, asteroids) | | Light-year (ly) | 9.461 × 10¹⁵ m (9.46T km) | Interstellar (nearby stars, galaxies) | | Parsec (pc) | 3.086 × 10¹⁶ m (30.86T km) | Professional astronomy (galactic/extragalactic) |

Conversions:

  • 1 light-year = 63,241 AU (63,000× Earth-Sun distance)
  • 1 parsec = 3.26 light-years = 206,265 AU

Why each exists:

  • AU: Human-scale for our cosmic neighborhood
  • Light-year: Intuitive for the public (distance = time × speed)
  • Parsec: Technical (distance where 1 AU subtends 1 arcsecond parallax)

Astronomers often use parsecs in papers but light-years in public communication.

The foot is a unit of length in the British imperial and United States customary systems of measurement. Since the international yard and pound agreement of 1959, one foot has been defined as exactly 0.3048 meters, which equals precisely 12 inches or 1/3 of a yard.

The foot is denoted by the symbol ft or by a single prime mark (e.g., 6′ means 6 feet). When combined with inches, the notation uses both symbols: 5′-9″ means 5 feet, 9 inches (69 inches total, or approximately 1.75 meters).

The foot occupies a unique position in the imperial system as the most commonly used length unit for human-scale measurements—distances that relate directly to human body size, living spaces, and immediate environments. While inches handle smaller precision work and miles cover long distances, feet describe the comfortable middle ground of everyday human experience.

Note: The Light Year is part of the imperial/US customary system, primarily used in the US, UK, and Canada for everyday measurements. The Foot belongs to the imperial/US customary system.

History of the Light Year and Foot

Pre-Light-Speed Era (Ancient - 1676)

Ancient assumptions: For millennia, humans assumed light traveled instantaneously. Aristotle (4th century BCE) argued light had no travel time—"light is the presence of something, not motion."

Galileo's failed experiment (1638): Galileo attempted to measure light speed using lanterns on distant hills. One person uncovers a lantern; another uncovers theirs upon seeing the first. The delay would reveal light's speed.

Result: No detectable delay (light travels 300,000 km/s; Galileo's hills were ~1 km apart, giving a 0.000003-second delay—impossible to measure with 17th-century tools).

Ole Rømer's Breakthrough (1676)

The observation: Danish astronomer Ole Rømer studied Jupiter's moon Io, which orbits Jupiter every 42.5 hours. He noticed Io's eclipses (passing behind Jupiter) occurred earlier when Earth was approaching Jupiter and later when Earth was receding.

The insight: The discrepancy wasn't Io's orbit—it was light travel time. When Earth was closer to Jupiter, light had less distance to travel; when farther, more distance.

Calculation:

  • Earth's orbital diameter: ~300 million km (2 AU)
  • Io eclipse time difference: ~22 minutes
  • Light speed: 300 million km / 22 min ≈ 227,000 km/s

Result: First proof that light has finite speed (underestimated by 24%, but revolutionary).

Implication: If light takes time to travel, then distances could be measured in "light travel time"—the seed of the light-year concept.

Stellar Aberration (1728)

James Bradley's discovery: Bradley observed that stars appear to shift position annually in small ellipses (aberration), caused by Earth's orbital motion combined with light's finite speed.

Analogy: Raindrops fall vertically, but if you run, they appear to come at an angle. Similarly, Earth's motion makes starlight appear tilted.

Calculation: Bradley measured aberration angle (~20 arcseconds) and Earth's orbital speed (30 km/s):

c = (Earth's speed) / tan(aberration angle)
c ≈ 301,000 km/s

Result: Refined light speed to within 0.4% of the modern value.

First Stellar Distance (1838)

Friedrich Bessel's parallax measurement: Bessel measured the parallax of 61 Cygni—the first successful stellar distance measurement. As Earth orbits the Sun, nearby stars appear to shift against distant background stars.

Result: 61 Cygni is 10.3 light-years away (modern: 11.4 ly).

Significance: Bessel's work required thinking in "light travel distance." Though he didn't use the term "light-year," his 1838 paper calculated: "Light from 61 Cygni takes 10.3 years to reach Earth."

The term "light-year" emerges: By the 1850s-1860s, astronomers adopted "light-year" for convenience. Early spellings varied ("light year," "light-year," "lightyear"), but "light-year" standardized by 1900.

Terrestrial Light-Speed Measurements (1849-1862)

Armand Fizeau (1849): First terrestrial measurement of light speed using a rotating toothed wheel. Light passed through a gap, reflected off a mirror 8.6 km away, and returned. By spinning the wheel faster, the light could be blocked by the next tooth.

Result: 315,000 km/s (5% high, but groundbreaking).

Léon Foucault (1862): Improved Fizeau's method using rotating mirrors. Achieved 298,000 km/s (within 1% of modern value).

Albert Michelson (1879-1926): Refined measurements to extreme precision:

  • 1879: 299,910 km/s
  • 1926: 299,796 km/s (within 12 km/s of modern value)

The Meter Redefinition (1983)

The problem: The meter was defined as 1/10,000,000 of the distance from the equator to the North Pole (via Paris), later refined using a platinum-iridium bar. But this was imprecise—the bar's length changed with temperature.

The solution: In 1983, the International Bureau of Weights and Measures redefined the meter in terms of the speed of light:

1 meter = distance light travels in 1/299,792,458 of a second

This fixed the speed of light at exactly 299,792,458 m/s, making the light-year a derived but precise unit:

1 ly = 299,792,458 m/s × 31,557,600 s = 9,460,730,472,580,800 m (EXACT)

Implication: The meter is now defined by light. The light-year, parsec, and astronomical unit all derive from this constant.

Modern Cosmology (20th-21st Century)

Edwin Hubble (1924-1929): Hubble measured distances to galaxies, proving the universe extends far beyond the Milky Way. Andromeda Galaxy: 2.5 million light-years (originally underestimated at 900,000 ly).

Hubble's Law (1929): Galaxies recede from us at speeds proportional to their distance. The farther away, the faster they move (universe is expanding).

Cosmic microwave background (1965): Arno Penzias and Robert Wilson detected the CMB—light from 380,000 years after the Big Bang, now 13.8 billion light-years away (but due to expansion, the source is now 46 billion light-years distant).

James Webb Space Telescope (2022): JWST observed galaxies 13.4 billion light-years away—seeing the universe as it was 400 million years after the Big Bang.

The observable universe: The farthest light we can see is 46 billion light-years away (accounting for cosmic expansion). Beyond this, the universe has expanded so much that light hasn't reached us yet.

The foot represents one of humanity's oldest measurement units, with origins predating written records.

Ancient Origins: The foot concept emerged independently in multiple ancient civilizations, all based on the approximate length of a human foot. The Egyptian royal cubit (20.6 inches) divided into smaller units approximating foot measurements. The Greek pous measured roughly 11.6 inches, while the Roman pes (foot) standardized at approximately 11.65 modern inches (296 mm).

Roman Influence: When Romans conquered Britain, they brought the pes, which heavily influenced British measurement traditions. The Roman foot divided into 12 unciae (inches), establishing the 12-inch relationship that persists today. Even after the Roman Empire fell, this measurement structure survived in English-speaking regions.

Medieval Variations: Throughout medieval Europe, foot measurements varied dramatically by region and ruler. Different "feet" existed simultaneously—the Tower foot, the London foot, and various guild-specific feet. King Henry I of England (r. 1100-1135) reportedly standardized the yard as the distance from his nose to his outstretched thumb, making the foot one-third of that distance.

Statute Definitions: In 1266, King Henry III's Composition of Yards and Perches defined relationships between feet, yards, and rods for land measurement. The 1324 statute by Edward II attempted further standardization, though regional variations persisted for centuries.

English Standardization: The British Weights and Measures Act of 1824 established the Imperial foot throughout the British Empire. This Imperial foot differed slightly from the US foot after American independence—the US maintained measurements from pre-1824 British standards.

1959 International Agreement: The international yard and pound agreement unified English-speaking countries. The United States, United Kingdom, Canada, Australia, New Zealand, and South Africa agreed that 1 yard equals exactly 0.9144 meters, making 1 foot exactly 0.3048 meters (304.8 mm). This ended over a century of slight differences between US and British feet.

US Survey Foot Retirement: From 1893 to 2023, the United States maintained two different feet—the international foot (0.3048 m exactly) and the US survey foot (0.30480061 m, or 1200/3937 meters). The survey foot was used for land surveys and mapping. On January 1, 2023, the National Geodetic Survey officially retired the US survey foot, making all American measurements use the international foot exclusively.

Aviation Standard: In 1947, the International Civil Aviation Organization (ICAO) standardized altitude measurements worldwide in feet. This remains universal today—even pilots in fully metric countries like France, Germany, and Japan report altitude in feet. This standardization prevents confusion and enhances safety in international aviation.

Common Uses and Applications: light years vs feet

Explore the typical applications for both Light Year (imperial/US) and Foot (imperial/US) to understand their common contexts.

Common Uses for light years

1. Stellar Distances and Exoplanets

Astronomers use light-years to describe distances to stars and planetary systems.

Example: TRAPPIST-1 system

  • Distance: 39 ly
  • 7 Earth-sized planets, 3 in habitable zone
  • Red dwarf star, 9% Sun's mass
  • Discovered: 2017 (Spitzer Space Telescope)

Example: Kepler-452b ("Earth's cousin")

  • Distance: 1,400 ly
  • Orbits a Sun-like star in the habitable zone
  • 1.6× Earth's diameter
  • Potentially rocky with liquid water

Exoplanet nomenclature:

  • "HD 209458 b is 159 ly away" (hot Jupiter, first exoplanet with detected atmosphere)
  • "Proxima b is 4.24 ly away" (nearest potentially habitable exoplanet)

2. Galactic Structure and Astronomy

Milky Way dimensions:

  • Diameter: ~100,000 ly
  • Thickness (disk): ~1,000 ly
  • Sun's distance from galactic center: 26,000 ly
  • Galactic rotation: Sun orbits the galaxy every 225-250 million years (1 "galactic year")

Spiral arms:

  • Milky Way has 4 major arms: Perseus, Scutum-Centaurus, Sagittarius, Norma
  • Sun is in the Orion Arm (minor spur between Perseus and Sagittarius)

Globular clusters:

  • Spherical collections of ancient stars orbiting the Milky Way
  • M13 (Hercules Cluster): 25,000 ly
  • Omega Centauri: 15,800 ly (largest globular cluster, 10 million stars)

3. Cosmology and the Expanding Universe

Hubble's Law:

v = H₀ × d

Where:

  • v = recession velocity (km/s)
  • H₀ = Hubble constant (70 km/s per megaparsec ≈ 21.5 km/s per million light-years)
  • d = distance (light-years)

Example: A galaxy 100 million light-years away recedes at:

v = 21.5 km/s/Mly × 100 Mly = 2,150 km/s

Cosmological redshift: As the universe expands, light stretches to longer wavelengths (redshift). The farther the galaxy, the greater the redshift.

z = (observed wavelength - emitted wavelength) / emitted wavelength

  • z = 0: No redshift (nearby objects)
  • z = 1: Wavelength doubled (universe half its current size)
  • z = 6: Early galaxies (universe 1/7 its current size)
  • z = 1,100: CMB (universe 1/1,100 its current size)

4. Lookback Time (Viewing Cosmic History)

Every light-year is a journey into the past.

10 ly: Early 2010s (when smartphones became ubiquitous) 100 ly: 1920s (Roaring Twenties, right after WWI) 1,000 ly: Dark Ages/Early Middle Ages (Vikings, fall of Rome) 10,000 ly: End of last Ice Age, dawn of agriculture 100,000 ly: Early Homo sapiens, before language 1 million ly: Human ancestors, stone tools 13.8 billion ly: 380,000 years after the Big Bang (CMB)

The cosmic horizon: We can't see beyond 46 billion ly (comoving distance). Light from farther hasn't reached us yet.

5. SETI and Interstellar Communication

Drake Equation: Estimates the number of active, communicative civilizations in the Milky Way. Light-years define the "communication horizon."

Example: If a civilization 100 ly away sent a radio signal in 1924, we'd receive it in 2024. If we reply, they'd get our message in 2124—a 200-year round trip.

Fermi Paradox: "Where is everybody?" If intelligent life exists, why haven't we detected it?

  • Milky Way is 100,000 ly across
  • Radio signals travel at light speed
  • A civilization 50,000 ly away could have sent signals 50,000 years ago (we might receive them in 25,000 years)

SETI targets:

  • Tau Ceti (11.9 ly): Sun-like star with planets
  • Epsilon Eridani (10.5 ly): Young star with debris disk
  • Proxima Centauri (4.24 ly): Nearest star, has a habitable-zone planet

6. Science Fiction and Cultural Impact

Star Trek:

  • Warp speed: Faster-than-light travel
  • "Warp 1" = speed of light (c)
  • "Warp 9" = 1,516× c (covers 1,516 ly in 1 year)
  • Necessity: Alpha Centauri (4.24 ly) takes 4.24 years at light speed—impractical for storytelling

Interstellar travel challenges:

  • Nearest star: 4.24 ly at light speed (current fastest spacecraft: Voyager 1 at 0.006% c would take 75,000 years)
  • Time dilation: At 99.9% c, 4.24 years pass on Earth, but only 60 days for travelers (Einstein's relativity)
  • Energy: Accelerating 1 kg to 10% c requires 4.5 × 10¹⁴ joules (100,000× a car's gasoline tank)

Generation ships: If we can't go faster than light, use multi-generational spacecraft:

  • 10,000-year journey to Proxima Centauri at 0.04% c
  • Crew born, live, and die onboard
  • Descendants arrive

7. Educational Outreach

Light-years make the universe accessible to the public.

Analogy: "Andromeda is 2.5 million light-years away" = "We see Andromeda as it was 2.5 million years ago, before Homo sapiens evolved."

Scale models: If the Solar System fit in your hand (Sun to Neptune = 10 cm):

  • Proxima Centauri: 2.7 km away
  • Galactic center: 13,000 km away (Earth's diameter!)
  • Andromeda: 125,000 km away (to the Moon and back, 1.5 times)

When to Use feet

Residential Construction and Remodeling

Home construction in America operates in feet for layout and square feet for area calculations. Foundation plans show exterior dimensions (e.g., 40' × 60' house footprint = 2,400 sq ft per floor). Interior walls use standard 8-foot studs for 8-foot ceiling heights, or 9-foot and 10-foot studs for taller ceilings.

Lumber lengths come in 2-foot increments: 6', 8', 10', 12', 14', 16' boards. This modular system allows efficient layout with minimal waste. A wall spanning 16 feet can use a single 16-foot top plate rather than joining shorter pieces.

Plywood and drywall sheets measure 4' × 8' (32 square feet per sheet). With standard 16-inch stud spacing, three studs span 48 inches (4 feet), perfectly matching sheet width. This dimensional coordination throughout the building industry stems from foot-based planning.

Standard door heights are 6'8" (80 inches), accommodating people up to about 6'5" with clearance. Door widths vary: 2'6" (30"), 2'8" (32"), 3'0" (36"). Window rough openings are specified in feet and inches: 3'0" × 4'0" window.

Architectural Design and Floor Plans

Architects draw floor plans at scales based on feet: 1/4" = 1'0" (common residential) or 1/8" = 1'0" (larger buildings). Blueprint dimensions appear as feet-inches notation: 12'-6" means 12 feet, 6 inches (150 inches total).

Room planning uses standard furniture dimensions understood in feet:

  • Queen bed: approximately 5' × 6'8"
  • King bed: approximately 6'4" × 6'8"
  • Sofa: 6-8 feet long
  • Dining table (seats 6): 3' × 6'
  • Dining table (seats 8): 3'6" × 7'

Designers ensure adequate circulation space: 3 feet minimum for walkways, 4 feet preferred. A 12' × 15' bedroom comfortably fits a king bed with nightstands and leaves walkway space.

Building codes specify requirements in feet: egress windows must have 5.7 square feet of opening, stair landings must be at least 3 feet deep, hallways must be at least 3 feet wide.

Commercial Real Estate and Office Space

Commercial property leasing operates in square feet. Office space leases quote price per square foot annually: $30/sq ft/year means a 1,000 sq ft office costs $30,000 per year ($2,500/month). Retail space commands higher rates, often $40-100+/sq ft/year in prime locations.

Office planning uses square feet per employee: 150-250 sq ft per person including shared spaces, or 50-75 sq ft for individual workstations. A company with 50 employees needs approximately 7,500-12,500 square feet total.

Commercial buildings describe floor plate size in square feet: a 100' × 120' floor plate provides 12,000 sq ft of rentable space per floor. Column spacing (typically 20-30 feet in modern buildings) affects layout flexibility.

Retail space measures street frontage in feet—20 feet, 40 feet, 60 feet of storefront directly influences visibility and foot traffic. Corner locations with frontage on two streets command premium rent.

Swimming and Aquatics

Swimming pools use feet for all dimensions. A typical residential pool might measure 16' × 32' (512 sq ft surface area) with shallow end 3'6" and deep end 8'0". Lap pools are typically 8-10 feet wide by 40-50 feet long.

Competition pools follow precise foot-based specifications:

  • Short course: 75 feet (25 yards, 6-8 lanes)
  • Olympic pool: 164 feet (50 meters, 10 lanes) with 6'6" minimum depth

Pool safety regulations require depth markers at 3', 4', 5', 6', 8', and deeper. "NO DIVING" signs appear in areas less than 9 feet deep. These measurements help swimmers quickly assess safety.

Interior Design and Space Planning

Interior designers work in feet for furniture placement and room flow. Industry standards include:

  • Seating area: 8' × 10' minimum for sofa, chairs, coffee table
  • Dining area: Allow 3 feet per chair, 3-4 feet circulation around table
  • Kitchen work triangle: 12-26 feet total (sum of distances between sink, stove, refrigerator)
  • Island clearance: 3-4 feet on all sides for traffic flow
  • TV viewing distance: 1.5-2.5× the diagonal screen size

A 12' × 18' living room (216 sq ft) allows space for a seating arrangement, TV console, and traffic flow. A 10' × 10' room (100 sq ft) feels cramped with more than a bed and dresser.

Window treatment specialists measure window width and height in feet and inches to calculate fabric requirements. Curtains typically extend 4-8 inches beyond window frame on each side, requiring precise foot-inch measurements.

Theater and Entertainment Venues

Stage dimensions, screen sizes, and venue layouts use feet:

  • Proscenium width: 30-50 feet (typical theater)
  • Stage depth: 20-40 feet
  • Fly space: 60-80+ feet (above stage for scenery)
  • Movie screen width: 40-90 feet (commercial theaters)
  • IMAX screen: 72' × 52' (standard), 97' × 76' (largest)

Theatrical lighting positions specify trim height (distance from stage floor to light) in feet: 12', 18', 24'. Sound engineers place speakers based on feet of distance to achieve proper coverage—one speaker per 30-50 feet of venue length.

Venue capacity relates to square footage: 6-7 square feet per person for standing room, 10-12 sq ft per person for chair seating with aisles, 15-20 sq ft per person for banquet seating with tables.

Firefighting and Emergency Services

Fire departments specify equipment reach in feet: 75-foot aerial ladders, 100-foot platform trucks. Building codes restrict height based on fire equipment access—many jurisdictions limit wood-frame construction to 75 feet (roughly 7 stories) due to ladder reach limitations.

Hose lengths standardize at 50 feet or 100 feet. Firefighters calculate distance from hydrant to building entrance in feet to determine hose requirements. Water pressure calculations use feet of elevation: each foot of elevation change requires roughly 0.43 PSI pressure adjustment.

Emergency responders use feet for scene measurements: accident scenes, crime scenes, and disaster areas document positions and distances in feet. "Vehicle came to rest 150 feet beyond point of impact" provides clear spatial understanding.

Landscaping and Irrigation

Landscape contractors measure yards in feet for material calculations and cost estimates. Sod comes in rolls typically 2' × 5' (10 sq ft). Mulch, topsoil, and gravel calculate coverage in square feet at various depths: 1 cubic yard covers 324 sq ft at 1 inch depth, or 81 sq ft at 4 inches depth.

Irrigation system design uses feet for sprinkler spacing: 15-foot spacing for spray heads, 30-40 foot spacing for rotary heads. Drip irrigation calculates emitter placement in feet: 12-18 inches for flower beds, 2-3 feet for shrubs.

Tree planting requires spacing in feet based on mature spread: 15-20 feet apart for small trees, 30-40 feet for large shade trees, 50+ feet for massive specimens. "Plant trees 30 feet from building foundations" prevents root damage to structures.

Property grading specifies slope in inches per foot: 2-3 inches of drop per 10 feet of distance away from house foundations prevents water intrusion.

Additional Unit Information

About Light Year (ly)

1. Is a light-year a unit of time or distance?

Distance. Despite the name containing "year," the light-year measures distance—how far light travels in one year.

Analogy: "New York is 3 hours from Boston" means 3 hours of driving (distance ~180 miles), not that New York exists for 3 hours.

Why the confusion? The name uses time (year) as a reference, but the quantity measured is distance (9.46 trillion km).

Correct usage:

  • "Proxima Centauri is 4.24 light-years away" (distance)
  • "Light takes 4.24 years to reach us from Proxima Centauri" (time)

2. How far is a light-year in kilometers and miles?

Exactly 9,460,730,472,580,800 meters.

Rounded values:

  • Metric: ~9.46 trillion km (9.461 × 10¹² km)
  • Imperial: ~5.88 trillion miles (5.879 × 10¹² mi)

Why "exactly"? Since 1983, the meter is defined via the speed of light (exactly 299,792,458 m/s). A Julian year is exactly 31,557,600 seconds. Thus:

1 ly = 299,792,458 m/s × 31,557,600 s = 9,460,730,472,580,800 m (EXACT)

3. What is the closest star to Earth in light-years?

Excluding the Sun: Proxima Centauri at 4.24 light-years.

Including the Sun: The Sun at 0.0000158 light-years (1 AU, 8 min 19 sec light travel time).

Proxima Centauri details:

  • Part of Alpha Centauri system (triple star: A, B, Proxima)
  • Red dwarf, 12% Sun's mass
  • Has at least 1 confirmed planet (Proxima b) in the habitable zone

Why no closer stars? Space is mostly empty. The next nearest star after Proxima is Barnard's Star (5.96 ly).

Perspective: At Voyager 1's speed (17 km/s), reaching Proxima Centauri would take 75,000 years.

4. How long does it take light to travel 1 light-year?

Exactly 1 Julian year = 365.25 days.

This is the definition: A light-year is the distance light travels in one year.

Breakdown:

  • 1 year = 365.25 days
  • 1 day = 86,400 seconds
  • 1 year = 31,557,600 seconds
  • At 299,792,458 m/s, light travels 9,460,730,472,580,800 m in 1 year

Implication: If you see a star 100 light-years away, the light left that star 100 years ago. You're viewing the past.

5. Why use light-years instead of kilometers for measuring space?

Convenience and intuition.

Interstellar distances in kilometers are incomprehensible:

  • Proxima Centauri: 40,208,000,000,000 km (40.2 trillion km)
  • Andromeda Galaxy: 23,740,000,000,000,000,000 km (23.7 quintillion km)

In light-years:

  • Proxima Centauri: 4.24 ly
  • Andromeda Galaxy: 2.5 million ly

Lookback time advantage: Light-years automatically convey when you're seeing something. "Betelgeuse is 548 ly away" means you see it as it was in 1476 (Renaissance).

Human brains handle ratios better than enormous numbers.

6. Can anything travel faster than light?

No object with mass can reach or exceed the speed of light (Einstein's special relativity).

Why: As an object approaches light speed, its relativistic mass increases, requiring infinite energy to reach c.

Exceptions (not "faster than light" but close):

  1. Tachyons (hypothetical): Particles that always travel faster than c (never proven to exist)
  2. Expansion of space: Distant galaxies recede faster than c due to cosmic expansion (space itself expands, objects don't move through space faster than c)
  3. Quantum entanglement: Information can't be transmitted faster than c, but entangled particles correlate instantaneously (doesn't violate relativity—no usable information transferred)

Warp drives (theoretical): Alcubierre drive concept: Compress space in front, expand behind. You stay stationary in a "bubble," but the bubble moves faster than c. Requires exotic matter (negative energy density), which may not exist.

7. What is the farthest object we can see in light-years?

Cosmic Microwave Background (CMB): 46 billion light-years (comoving distance).

Why farther than 13.8 billion ly (age of universe)? The universe has been expanding. Light from the CMB took 13.8 billion years to reach us, but the source is now 46 billion ly away due to expansion.

Farthest observed galaxy: JADES-GS-z13-0 (James Webb Space Telescope, 2022)

  • Light travel time: 13.4 billion years
  • We see it as it was 400 million years after the Big Bang
  • Current distance (comoving): ~32 billion ly

Observable universe: Radius: 46 billion ly (sphere of ~550 sextillion km radius). Beyond this, light hasn't reached us yet.

8. How do astronomers measure distances in light-years?

Method depends on distance:

1. Parallax (nearby stars, <1,000 ly): As Earth orbits the Sun (2 AU baseline), nearby stars shift against distant background stars. Measuring the parallax angle gives distance.

Formula:

distance (parsecs) = 1 / parallax angle (arcseconds)
distance (ly) = 3.26 / parallax angle

Example: Proxima Centauri has 0.7687 arcsecond parallax → 1.30 pc = 4.24 ly

2. Standard candles (intermediate, 1,000-1 billion ly): Objects with known intrinsic brightness (Cepheid variables, Type Ia supernovae). Measure apparent brightness, calculate distance.

3. Redshift (distant galaxies, >1 billion ly): Universe expansion stretches light (redshift). Greater redshift = greater distance. Use Hubble's Law and cosmological models.

9. Why do astronomers sometimes use parsecs instead of light-years?

Parsecs (pc) are more natural for parallax measurements (the primary method for measuring stellar distances).

Definition: 1 parsec = distance at which 1 AU subtends 1 arcsecond of parallax

Conversion: 1 parsec = 3.26 light-years

Usage:

  • Professional astronomy: Parsecs, kiloparsecs (kpc), megaparsecs (Mpc)
  • Public communication: Light-years (more intuitive)

Example:

  • Galactic center: 8 kpc (professional) = 26,000 ly (public)

Why parsecs exist: They simplify calculations. Distance (pc) = 1 / parallax angle (arcseconds). Using light-years requires extra conversion steps.

10. What does it mean to "look back in time"?

Every photon carries a timestamp. Light takes time to travel, so we see distant objects as they were when the light left.

Examples:

  • Sun (8 light-minutes): You see it as it was 8 minutes ago
  • Proxima Centauri (4.24 ly): You see it as it was 4.24 years ago (2020 if viewing in 2024)
  • Andromeda (2.5 million ly): You see it as it was 2.5 million years ago (before Homo sapiens)
  • CMB (13.8 billion ly): You see the universe as it was 380,000 years after the Big Bang

Implication: Astronomy is historical science. The farther you look, the further back in time you see.

11. Could we ever travel to another star?

Theoretically yes, practically extraordinarily difficult.

Challenges:

1. Distance:

  • Nearest star: Proxima Centauri (4.24 ly = 40.2 trillion km)
  • Fastest spacecraft (Voyager 1): 17 km/s (0.006% light speed)
  • Travel time at Voyager 1 speed: 75,000 years

2. Energy: Accelerating 1 kg to 10% light speed:

E ≈ 4.5 × 10¹⁴ joules (entire energy output of a small city for a year)

3. Time dilation: At 99% light speed, time slows for travelers (Einstein's relativity):

  • Earth: 4.3 years pass
  • Spacecraft: 7 months pass for crew

Proposed solutions:

  • Generation ships: Multi-generational voyages (10,000+ years)
  • Nuclear pulse propulsion (Project Orion): Explode nukes behind ship for thrust (10-20% c possible)
  • Light sails (Breakthrough Starshot): Lasers push ultra-light probes to 20% c (reach Proxima in 20 years)
  • Antimatter rockets: Matter-antimatter annihilation (100% mass-energy conversion, but antimatter production is prohibitively expensive)

12. What is the observable universe, and why is it 46 billion light-years if the universe is only 13.8 billion years old?

Observable universe = region from which light has had time to reach us.

Why 46 billion ly, not 13.8 billion ly? The universe has been expanding for 13.8 billion years. Objects whose light took 13.8 billion years to reach us have moved farther away due to expansion.

Example:

  • Light from a galaxy left 13.4 billion years ago (400M years after Big Bang)
  • During 13.4 billion years, the universe expanded
  • That galaxy is now ~32 billion ly away

Comoving vs. light travel distance:

  • Light travel distance: How long light has been traveling (13.8 billion years max)
  • Comoving distance: Where the object is now, accounting for expansion (46 billion ly radius)

Observable universe:

  • Radius: 46 billion ly (comoving)
  • Diameter: 93 billion ly
  • Beyond this: Universe exists, but light hasn't reached us yet (and never will, due to accelerating expansion)

About Foot (ft)

How many inches are in a foot?

There are exactly 12 inches in 1 foot. This relationship is fundamental to the imperial measurement system and has remained constant since ancient Roman times, when the pes (foot) was divided into 12 unciae (inches).

The 12-inch division offers mathematical convenience—12 is evenly divisible by 2, 3, 4, and 6, making fractional measurements easier in practical work. You can divide a foot into halves (6"), thirds (4"), quarters (3"), or sixths (2") with whole-number results.

Converting feet to inches: Multiply feet by 12

  • 5 feet = 5 × 12 = 60 inches
  • 7.5 feet = 7.5 × 12 = 90 inches

Converting inches to feet: Divide inches by 12

  • 72 inches = 72 ÷ 12 = 6 feet
  • 100 inches = 100 ÷ 12 = 8.33 feet = 8 feet, 4 inches

Mixed notation: 5'9" means 5 feet, 9 inches = (5 × 12) + 9 = 69 inches total.

How many feet are in a yard?

There are exactly 3 feet in 1 yard. This relationship dates back to medieval English measurements, where the yard represented a stride or the distance from the nose to an outstretched thumb of King Henry I.

The yard serves as a larger unit convenient for measuring fabric, sports fields, and medium distances. In American football, progress is measured in yards (first down = 10 yards = 30 feet), but field dimensions are often specified in feet (field width = 160 feet = 53⅓ yards).

Converting yards to feet: Multiply yards by 3

  • 10 yards = 10 × 3 = 30 feet
  • 100 yards = 100 × 3 = 300 feet (length of football field)

Converting feet to yards: Divide feet by 3

  • 90 feet = 90 ÷ 3 = 30 yards (baseball base paths)
  • 18 feet = 18 ÷ 3 = 6 yards (first down in football)

How many feet are in a mile?

There are exactly 5,280 feet in 1 mile. This seemingly arbitrary number results from historical compromises between different English measurement systems.

Historical origin: The Roman mile (mille passus) measured 1,000 paces (about 5,000 feet). Medieval England used furlongs for agricultural land measurement (660 feet = 1 furlong). Queen Elizabeth I standardized the mile in 1593 as exactly 8 furlongs, making 1 mile = 8 × 660 = 5,280 feet.

Common conversions:

  • 1 mile = 5,280 feet
  • 0.5 mile = 2,640 feet
  • 0.25 mile = 1,320 feet
  • 1,000 feet = 0.189 miles (about 3 city blocks)

Why it matters: Aircraft measure runway length in feet (7,000-foot runway, 10,000-foot runway), while navigation uses nautical miles (6,076 feet) or statute miles (5,280 feet). Real estate describes proximity in feet for nearby amenities ("500 feet to park") and miles for distant locations ("3 miles to downtown").

What's the difference between feet and square feet?

Feet (linear feet) measure distance in one dimension—length along a line. Use feet for measuring height, room length, fence lines, rope, baseboards, or any one-dimensional measurement.

Square feet measure area in two dimensions—the surface of a two-dimensional space. Use square feet for flooring, walls, ceilings, land area, or any flat surface.

The relationship: Square feet = length (in feet) × width (in feet)

  • A room 12 feet long × 15 feet wide = 180 square feet
  • A wall 10 feet wide × 8 feet tall = 80 square feet

Why confusion happens: A room with 54 linear feet of baseboard (12+15+12+15) contains 180 square feet of floor area. These are different measurements of the same room—perimeter versus area.

Cost implications: Contractors price differently:

  • Fencing: $15-40 per linear foot installed
  • Flooring: $3-12 per square foot installed
  • Painting: $2-6 per square foot

Always clarify whether a price quote is per linear foot or per square foot—the difference is substantial.

Why does aviation use feet for altitude worldwide?

Aviation universally uses feet for altitude measurement, even in countries that otherwise use metric exclusively, for safety and standardization. This system was established by the International Civil Aviation Organization (ICAO) in 1947.

Historical reason: When commercial aviation developed in the 1920s-1940s, British and American manufacturers dominated, and altimeters measured in feet. As aviation became international, standardizing on the existing system proved safer and cheaper than converting all aircraft instruments and training.

Safety benefits: Universal altitude standards prevent confusion during international flights. When a French pilot, Japanese air traffic controller, and American pilot all say "flight level three-five-zero," everyone knows it means 35,000 feet. No conversion errors, no miscommunication, no accidents from unit confusion.

Vertical separation: Aircraft flying opposite directions maintain 1,000-foot vertical separation (2,000 feet above 29,000'). This separation is calibrated into procedures, training, and equipment worldwide. Changing to meters would require recalibrating countless procedures and risking lives during the transition.

Exceptions: China and Russia use meters for some domestic operations below 29,500 feet, but convert to feet-based flight levels for international flights and at high altitudes. This hybrid system is gradually shifting toward full feet-based standards.

Practical result: Pilots must understand feet regardless of nationality. Pilot training worldwide includes feet-based altitude management, making it one of the few truly universal measurements.

How do I convert feet to meters accurately?

To convert feet to meters, multiply by 0.3048. This is the exact conversion factor established by the 1959 international agreement.

Formula: meters = feet × 0.3048

Examples:

  • 1 foot = 1 × 0.3048 = 0.3048 meters
  • 5 feet = 5 × 0.3048 = 1.524 meters
  • 6 feet = 6 × 0.3048 = 1.8288 meters
  • 10 feet = 10 × 0.3048 = 3.048 meters
  • 100 feet = 100 × 0.3048 = 30.48 meters

Reverse conversion (meters to feet): Divide by 0.3048, or multiply by 3.28084

  • 1 meter = 1 ÷ 0.3048 = 3.28084 feet
  • 5 meters = 5 × 3.28084 = 16.404 feet
  • 10 meters = 10 × 3.28084 = 32.808 feet

Quick mental approximation: For rough estimates, remember 1 meter ≈ 3.3 feet (or more precisely, 3.28 feet). This gives close results:

  • 10 meters ≈ 33 feet (actual: 32.8 feet)
  • 100 meters ≈ 330 feet (actual: 328 feet)

For professional work requiring precision (construction, engineering, manufacturing), always use the exact factor 0.3048 rather than approximations.

What does feet-inches notation mean?

The notation 5′-9″ (or 5'9") means 5 feet, 9 inches. The single prime ′ (or apostrophe ') represents feet, while the double prime ″ (or quote ") represents inches.

Reading the notation:

  • 6′ = six feet = 72 inches
  • 6″ = six inches = 0.5 feet
  • 5′-9″ = five feet, nine inches = 69 inches total = 5.75 feet decimal
  • 12′-6½″ = twelve feet, six and a half inches = 150.5 inches = 12.542 feet decimal

Why the dash? The dash or hyphen between feet and inches makes the notation clearer in blueprints and prevents confusion. Without it, 5'9" might be misread, though the prime symbols make the meaning clear.

Common uses:

  • Human height: "She's 5'6" tall"
  • Room dimensions: "12' × 15' bedroom"
  • Construction drawings: Wall length shown as 24'-3½"

Converting to total inches: Multiply feet by 12, then add inches:

  • 5'9" = (5 × 12) + 9 = 60 + 9 = 69 inches

Converting from total inches: Divide by 12 for feet, use remainder for inches:

  • 75 inches = 75 ÷ 12 = 6 remainder 3 = 6'3"

Why is the foot still used instead of meters?

The United States continues using feet instead of meters primarily due to infrastructure investment, industry standardization, and cultural identity—not because feet offer any technical advantage.

Infrastructure costs: Converting to metric would require replacing billions of feet-based measurements throughout American infrastructure:

  • 4 million miles of road signs showing feet/miles
  • Building codes and standards written in feet
  • Millions of blueprints, survey records, and property deeds
  • Construction materials sized in feet (8' studs, 4'×8' sheets)
  • Manufacturing equipment calibrated in decimal feet (thousandths of an inch)

Estimated conversion cost: $370 billion to $1 trillion.

Industry standardization: American construction, real estate, aviation, and manufacturing operate entirely in feet. Changing would require:

  • Retraining millions of workers
  • Replacing tools, measuring devices, and equipment
  • Converting countless technical documents
  • Updating software systems and databases

Cultural familiarity: Americans instinctively understand feet—"six feet tall," "ten feet away," "twenty feet deep." These measurements connect to body scale and everyday experience. Most Americans don't have intuitive feel for meters, making conversion feel arbitrary and confusing.

Partial adoption: The US actually uses metric in science, medicine, military, and some industries. Soft drinks come in liters, track races use meters, pharmaceuticals dose in milligrams. Americans live in a hybrid system.

Failed conversions: The 1975 Metric Conversion Act made metric "preferred" but voluntary. Without enforcement, most industries continued with feet. Public backlash against metric road signs in the 1980s ended highway conversion attempts.

International exceptions: Aviation worldwide uses feet for altitude. Maritime navigation uses nautical miles and fathoms. Even metric countries maintain some imperial measurements in specific contexts, showing that pure metric conversion isn't always practical or necessary.

How fast does light travel in a foot?

In vacuum, light travels one foot in approximately 1.0167 nanoseconds. In computer networking and high-frequency trading, this is a critical measurement—engineers often say "a nanosecond is a foot" as a rule of thumb for how fast signals move through cables.

Why is a "foot" divided into 12 inches instead of 10?

The number 12 is a "Highly Composite Number." It can be divided evenly into 2, 3, 4, and 6. This was incredibly useful for ancient builders and tradesmen who didn't have calculators. They could easily calculate "half a foot" (6"), "a third of a foot" (4"), or "a quarter of a foot" (3") without dealing with decimals like 3.333.

Is my physical foot actually one foot long?

Probably not! The average male foot is about 10.5 inches (26.6 cm) long, and the average female foot is about 9.5 inches (24 cm). The "standard foot" measurement was likely based on a very large foot (perhaps a king's) or a foot wearing a heavy boot.

What is the "Board Foot" used in lumber?

A board foot is actually a unit of volume, not length. It represents a piece of wood that is 1 foot long, 1 foot wide, and 1 inch thick. When you buy expensive hardwood, the price is usually "per board foot."

How many feet are in a "Standard Story" of a building?

In residential construction, a floor is typically 8 to 10 feet high. In commercial office buildings, it's often 12 to 14 feet to allow for air conditioning ducts and wiring above the ceiling.

Can a pilot choose to fly in meters?

No. In almost every country in the world, air traffic control mandates the use of feet for altitude. If a pilot used meters, they might collide with another plane. The only major exceptions have historically been Russia and China, and even they are moving toward the international feet-based standard.

What is a "Square Foot" vs. a "Linear Foot"?

Linear feet measure length (like a fence). Square feet measure area (like a carpet). A 10' x 10' room has 40 linear feet of walls but 100 square feet of floor.

Is the UK foot different from the US foot?

Since 1959, they are identical. Before 1959, the UK foot was about 2 parts per million shorter than the US foot.

How many feet are in a Fathom?

A Fathom is exactly 6 feet. It was traditionally the distance between a man's outstretched arms and is still used today to measure water depth in maritime navigation.

Why do we use a prime mark (') for feet?

The single prime (') comes from the Latin minuta, meaning "small part." The double prime (") for inches comes from secunda minuta, or "second small part." Interestingly, this is the same reason we use these symbols for minutes and seconds in time!

How many feet are in a "Rod"?

A rod is a historical unit of length equal to 16.5 feet. It was used in land surveying because four rods equal one "chain" (66 feet), and 80 chains equal exactly one mile.

What is the "Cubic Foot" of a refrigerator?

In the US, appliance capacity is measured in cubic feet. A 20 cubic foot refrigerator can hold approximately 566 liters of food. This is the volume of a space 1 foot high, 1 foot wide, and 1 foot deep, multiplied by 20.

How many feet is the world's deepest ocean point?

The Challenger Deep in the Mariana Trench is approximately 35,876 feet (10,935 meters) below sea level. If you put Mount Everest (29,032 feet) inside it, there would still be over a mile of water above the peak.

Why do some rulers have "architect's scales" in feet?

Architect's rulers allow you to draw large buildings on small paper. A common scale is 1/4 inch = 1 foot. This means every quarter-inch mark on your drawing represents 12 inches of a real building.

How many feet is a "Standard Leap" in the Long Jump?

The world record for the men's long jump is 29 feet, 4.25 inches (8.95 meters), set by Mike Powell in 1991.

Can I calculate feet by counting my steps?

Yes! A standard walking step (pace) for an adult is roughly 2.5 feet. If you count 40 steps, you have walked approximately 100 feet.

How many feet is an Olympic Swimming Pool?

A standard Olympic pool is 50 meters long, which is approximately 164 feet. In the US, many high school and community pools are "short course," meaning they are exactly 25 yards (75 feet) or 25 meters (82 feet).

What is a "Square Foot" of leather?

Tanneries sell leather by the square foot. Because hide shapes are irregular, specialized machines "scan" the skin to calculate the total square footage for pricing.

Is the "Metric Foot" a real thing?

Unofficially, yes. In some metric countries transitioning away from imperial units, builders sometimes use a "Metric Foot" of exactly 30 centimeters. It is roughly 1.5% shorter than a real foot but makes decimal math easier on construction sites.

How much is an acre in feet?

One acre equals 43,560 square feet. This measurement originates from medieval English land measurement, where an acre represented the amount of land a yoke of oxen could plow in one day.

Common acre configurations:

  • 1 acre = 43,560 square feet
  • 1 acre ≈ 208.7 feet × 208.7 feet (if square)
  • 1 acre = 660 feet × 66 feet (one furlong × one chain, historical farming measurement)

Practical examples:

  • 0.25 acre = 10,890 sq ft ≈ 104.4' × 104.4' (quarter-acre suburban lot)
  • 0.5 acre = 21,780 sq ft ≈ 147.6' × 147.6'
  • 2 acres = 87,120 sq ft ≈ 295.2' × 295.2'
  • 5 acres = 217,800 sq ft ≈ 466.7' × 466.7'

Football field comparison: An American football field including end zones measures 360 feet × 160 feet = 57,600 square feet = 1.32 acres. Without end zones, the playing field (300' × 160') is 48,000 sq ft = 1.1 acres.

Why it matters: Real estate describes land in acres but building sites in square feet or lot dimensions in feet. A half-acre lot might be 150' × 145', or 100' × 218'—multiple configurations yield the same area. Knowing the conversion helps visualize land size when shopping for property.

Zoning impact: Minimum lot sizes appear in ordinances as both acres and square feet: "0.5 acre minimum" = "21,780 square feet minimum." Subdivisions calculate density in units per acre: 4 houses per acre, 12 apartments per acre.

What's the origin of "six feet under"?

The phrase "six feet under" meaning burial or death originates from traditional grave depth—coffins were buried approximately six feet below ground surface.

Historical practice: The six-foot depth became standard in England during the 1665 Great Plague of London. Officials ordered plague victims buried "at least six foot deep" to prevent disease spread and discourage grave robbers. This depth kept odors contained and protected bodies from scavengers.

Modern burial depth: Contemporary cemeteries typically bury caskets 4-6 feet deep, though some jurisdictions specify different depths. The "six feet" measurement became culturally embedded as the standard, even when actual practice varies.

Measurement significance: Six feet provides enough earth to protect the coffin from surface disturbance (weather, animals, agriculture) while remaining practical to dig manually. Deeper burials exponentially increase labor, while shallower burials risk exposure.

Cultural persistence: The phrase "six feet under" persists in English as a euphemism for death, demonstrating how foot-based measurements embedded themselves in language and culture beyond mere physical measurement.

Conversion Table: Light Year to Foot

Light Year (ly)Foot (ft)
0.515,520,013,123,359,580
131,040,026,246,719,160
1.546,560,039,370,078,744
262,080,052,493,438,320
5155,200,131,233,595,800
10310,400,262,467,191,600
25776,000,656,167,979,000
501,552,001,312,335,958,000
1003,104,002,624,671,916,000
2507,760,006,561,679,790,000
50015,520,013,123,359,580,000
1,00031,040,026,246,719,160,000

People Also Ask

How do I convert Light Year to Foot?

To convert Light Year to Foot, enter the value in Light Year in the calculator above. The conversion will happen automatically. Use our free online converter for instant and accurate results. You can also visit our length converter page to convert between other units in this category.

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What is the conversion factor from Light Year to Foot?

The conversion factor depends on the specific relationship between Light Year and Foot. You can find the exact conversion formula and factor on this page. Our calculator handles all calculations automatically. See the conversion table above for common values.

Can I convert Foot back to Light Year?

Yes! You can easily convert Foot back to Light Year by using the swap button (⇌) in the calculator above, or by visiting our Foot to Light Year converter page. You can also explore other length conversions on our category page.

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What are common uses for Light Year and Foot?

Light Year and Foot are both standard units used in length measurements. They are commonly used in various applications including engineering, construction, cooking, and scientific research. Browse our length converter for more conversion options.

For more length conversion questions, visit our FAQ page or explore our conversion guides.

All Length Conversions

Meter to KilometerMeter to HectometerMeter to DecimeterMeter to CentimeterMeter to MillimeterMeter to InchMeter to FootMeter to YardMeter to MileMeter to Nautical MileMeter to MicrometerMeter to NanometerMeter to Light YearMeter to Astronomical UnitMeter to ParsecMeter to AngstromMeter to Point (Typography)Meter to Mil/ThouMeter to FathomMeter to FurlongMeter to Link (Gunter's)Meter to PaceMeter to SpanMeter to DigitMeter to Cable LengthMeter to EllMeter to FingerMeter to Roman MileMeter to StadionMeter to Chi (Chinese)Meter to Shaku (Japanese)Meter to Li (Chinese)Meter to ToiseMeter to BoltMeter to RopeMeter to SmootMeter to SajeneMeter to KenMeter to WaMeter to VaraMeter to AlnMeter to Cubit (Royal/Egyptian)Meter to VerstaMeter to ArpentMeter to Ri (Japanese)Meter to KlafterMeter to YojanaMeter to SkeinKilometer to MeterKilometer to HectometerKilometer to DecimeterKilometer to CentimeterKilometer to MillimeterKilometer to InchKilometer to FootKilometer to YardKilometer to MileKilometer to Nautical MileKilometer to MicrometerKilometer to NanometerKilometer to Light YearKilometer to Astronomical UnitKilometer to ParsecKilometer to AngstromKilometer to Point (Typography)Kilometer to Mil/ThouKilometer to FathomKilometer to FurlongKilometer to Link (Gunter's)Kilometer to PaceKilometer to SpanKilometer to DigitKilometer to Cable LengthKilometer to EllKilometer to FingerKilometer to Roman MileKilometer to StadionKilometer to Chi (Chinese)Kilometer to Shaku (Japanese)Kilometer to Li (Chinese)Kilometer to ToiseKilometer to BoltKilometer to RopeKilometer to SmootKilometer to SajeneKilometer to KenKilometer to WaKilometer to VaraKilometer to AlnKilometer to Cubit (Royal/Egyptian)Kilometer to VerstaKilometer to ArpentKilometer to Ri (Japanese)Kilometer to KlafterKilometer to YojanaKilometer to SkeinHectometer to MeterHectometer to KilometerHectometer to DecimeterHectometer to CentimeterHectometer to MillimeterHectometer to InchHectometer to FootHectometer to YardHectometer to MileHectometer to Nautical MileHectometer to MicrometerHectometer to NanometerHectometer to Light YearHectometer to Astronomical UnitHectometer to ParsecHectometer to AngstromHectometer to Point (Typography)Hectometer to Mil/ThouHectometer to FathomHectometer to FurlongHectometer to Link (Gunter's)Hectometer to PaceHectometer to SpanHectometer to Digit

Verified Against Authority Standards

All conversion formulas have been verified against international standards and authoritative sources to ensure maximum accuracy and reliability.

NIST Guide for the Use of SI

National Institute of Standards and TechnologyOfficial US standards for length measurements

SI Brochure

Bureau International des Poids et MesuresInternational System of Units official documentation

Last verified: February 19, 2026