Nanometer to Parsec Converter

Convert nanometers to parsecs with our free online length converter.

Quick Answer

1 Nanometer = 3.240756e-26 parsecs

Formula: Nanometer × conversion factor = Parsec

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: December 2025Reviewed by: Sam Mathew, Software Engineer

Nanometer to Parsec Calculator

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How to Convert Nanometer to Parsec: Step-by-Step Guide

Converting Nanometer to Parsec involves multiplying the value by a specific conversion factor, as shown in the formula below.

Formula:

1 Nanometer = 3.2408e-26 parsecs

Example Calculation:

Convert 10 nanometers: 10 × 3.2408e-26 = 3.2408e-25 parsecs

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 Nanometer and a Parsec?

A nanometer (symbol: nm) is a unit of length in the International System of Units (SI) equal to one billionth (10⁻⁹) of a meter:

1 nm = 0.000000001 m = 1 × 10⁻⁹ m

Why Is the Nanometer Scale Special?

The nanometer occupies a unique position between the atomic world and the microscopic world visible under optical microscopes:

1. Atomic to Molecular Scale:

  • Individual atoms: 0.1-0.3 nm diameter (hydrogen to larger elements)
  • Small molecules: 0.3-2 nm (water, glucose, amino acids)
  • Large biomolecules: 2-100 nm (proteins, DNA, ribosomes)

2. Quantum Effects Dominate:

  • At nanometer scales, quantum mechanical effects become significant
  • Electrons exhibit wave-particle duality
  • Quantum tunneling allows particles to pass through barriers
  • Energy levels become quantized (discrete rather than continuous)
  • Materials exhibit size-dependent properties (quantum dots change color with size)

3. Surface Area to Volume Ratio:

  • Nanoparticles have enormous surface area relative to volume
  • This makes them extremely reactive and useful for catalysis
  • Example: Gold is chemically inert in bulk but highly reactive as 5nm nanoparticles

4. Optical Properties Change:

  • Materials interact differently with light at nanometer scales
  • Nanostructures can manipulate light in ways impossible with bulk materials
  • Metamaterials with negative refractive index
  • Plasmonic effects in metal nanoparticles

The Nanometer in Context

Too Small to See with Optical Microscopes:

  • Optical microscopes use visible light (wavelengths 400-700nm)
  • Diffraction limit: Cannot resolve features smaller than ~200nm (half the wavelength)
  • Viewing nanometer-scale structures requires:
    • Electron microscopes (transmission or scanning, resolution to 0.1nm)
    • Scanning probe microscopes (STM, AFM, can "feel" individual atoms)
    • X-ray crystallography (infers structure from diffraction patterns)

Larger Than Individual Atoms:

  • Atoms: 0.1-0.3nm diameter
  • Nanometer scale: 1-100nm (roughly 3-300 atoms wide)
  • This is the realm of molecules, nanoparticles, viruses, and proteins

and Standards

Geometric Definition

The parsec is defined through trigonometric parallax:

1 parsec = the distance at which 1 astronomical unit (AU) subtends an angle of 1 arcsecond (1″)

Mathematically:

  • 1 parsec = 1 AU / tan(1″)
  • Since 1″ = 1/3600 degree = π/648,000 radians ≈ 4.8481 × 10⁻⁶ radians
  • For small angles: tan(θ) ≈ θ (in radians)
  • 1 parsec ≈ 1 AU / 4.8481 × 10⁻⁶ ≈ 206,265 AU

Exact IAU Value

The International Astronomical Union (IAU) defines the parsec exactly as:

1 parsec = 648,000/π AU ≈ 206,264.806247 AU

Using the IAU-defined astronomical unit (1 AU = 149,597,870,700 meters exactly as of 2012):

1 parsec = 30,856,775,814,913,673 meters (exactly)

Or approximately:

  • 3.0857 × 10¹⁶ meters
  • 30.857 trillion kilometers
  • 19.174 trillion miles

Relationship to Light-Year

The light-year (distance light travels in one Julian year) relates to the parsec:

1 parsec ≈ 3.26156 light-years

More precisely: 1 pc = 3.261563777 ly (using Julian year of 365.25 days)

Standard Multiples

Kiloparsec (kpc): 1 kpc = 1,000 pc ≈ 3,262 ly

  • Used for distances within galaxies
  • Milky Way diameter: ~30 kpc

Megaparsec (Mpc): 1 Mpc = 1,000,000 pc ≈ 3.26 million ly

  • Used for intergalactic distances
  • Andromeda Galaxy: ~0.77 Mpc

Gigaparsec (Gpc): 1 Gpc = 1,000,000,000 pc ≈ 3.26 billion ly

  • Used for cosmological distances
  • Observable universe radius: ~14 Gpc

Note: The Nanometer is part of the metric (SI) system, primarily used globally in science and trade. The Parsec belongs to the imperial/US customary system.

History of the Nanometer and Parsec

of the Nanometer and Nanotechnology

Early Foundations: Unknowingly Working at the Nanoscale (Pre-1900)

Ancient Nanomaterials (400 BCE - 1600 CE):

  • Roman Lycurgus Cup (4th century CE): Contains gold-silver nanoparticles (~70nm) that make glass appear red in transmitted light, green in reflected light
  • Medieval stained glass windows: Colloidal gold and other metal nanoparticles create vibrant colors
  • Ancient artisans unknowingly created nanomaterials through empirical recipes

Michael Faraday's Colloidal Gold (1857):

  • British scientist Michael Faraday systematically studied colloidal gold suspensions
  • Discovered that gold nanoparticles (5-100nm) exhibit ruby-red color, unlike bulk gold's yellow
  • First scientific recognition that material properties change at nanometer scale
  • Published "Experimental Relations of Gold (and Other Metals) to Light"
  • Laid foundation for nanoscience, though the term wouldn't exist for over a century

Theoretical Foundations (1900-1959)

Quantum Mechanics (1900-1930):

  • Max Planck (1900): Quantum theory—energy is quantized
  • Albert Einstein (1905): Photons (light quanta) and photoelectric effect
  • Niels Bohr (1913): Atomic model with discrete electron orbits
  • Erwin Schrödinger (1926): Wave equation describing electron behavior
  • These developments revealed that matter behaves fundamentally differently at atomic/molecular scales

Electron Microscopy (1931):

  • Ernst Ruska and Max Knoll invented the transmission electron microscope (TEM)
  • First images of structures below optical resolution (sub-100nm)
  • Enabled visualization of viruses, cell organelles, and eventually nanoparticles

The Birth of Nanotechnology Concept (1959-1980)

Richard Feynman's Vision (1959):

  • Famous lecture "There's Plenty of Room at the Bottom" at Caltech
  • Envisioned manipulating individual atoms to build materials and machines
  • Predicted writing entire Encyclopedia Britannica on head of a pin
  • Proposed molecular-scale machinery and atom-by-atom fabrication
  • Didn't use term "nanotechnology" but inspired the field

Norio Taniguchi Coins "Nanotechnology" (1974):

  • Japanese scientist Norio Taniguchi first used term "nanotechnology"
  • Referred to precision machining and material processing with tolerances below 1 micrometer
  • Initially described top-down manufacturing (machining, lithography)
  • Later expanded to bottom-up assembly (molecular self-assembly)

The Nanotechnology Revolution (1981-Present)

Scanning Tunneling Microscope - STM (1981):

  • Gerd Binnig and Heinrich Rohrer (IBM Zurich) invented STM
  • First instrument to "see" and manipulate individual atoms
  • Uses quantum tunneling effect to scan surfaces with atomic resolution
  • Won Nobel Prize in Physics (1986)
  • 1989: IBM scientists arranged 35 xenon atoms to spell "IBM" (first atomic-scale manipulation)

Atomic Force Microscope - AFM (1986):

  • Gerd Binnig, Calvin Quate, and Christoph Gerber invented AFM
  • Can image and manipulate atoms on insulators (not just conductors like STM)
  • "Feels" surface topography with nanometer-scale probe
  • Revolutionized nanoscale characterization across materials science, biology, chemistry

Fullerenes and Carbon Nanotubes (1985-1991):

  • Harold Kroto, Robert Curl, Richard Smalley discovered buckminsterfullerene (C₆₀, 1985)
    • Soccer-ball-shaped carbon molecule, ~0.7nm diameter
    • Nobel Prize in Chemistry (1996)
  • Sumio Iijima discovered carbon nanotubes (1991)
    • Cylindrical carbon structures, 1-100nm diameter, micrometers long
    • Exceptional strength, electrical conductivity, thermal properties
    • Sparked explosion of nanomaterials research

Semiconductor Nanometer Process Nodes (1990s-Present):

Moore's Law and the Nanometer Era:

  • Gordon Moore (1965): Predicted transistor count per chip would double every ~2 years
  • Drove relentless miniaturization of semiconductor features

Process Node Timeline:

  • 130 nm (2001): Intel Pentium 4, first widespread "nanometer node"
  • 90 nm (2004): AMD Athlon 64, Intel Pentium 4 Prescott
  • 65 nm (2006): Intel Core 2 Duo, beginning of multi-core era
  • 45 nm (2007): Intel Core 2 Duo (Penryn), high-k metal gates introduced
  • 32 nm (2010): Intel Core i3/i5/i7 (Westmere)
  • 22 nm (2012): Intel Ivy Bridge, first 3D FinFET transistors (non-planar)
  • 14 nm (2014): Intel Broadwell, Apple A8
  • 10 nm (2017): Intel Cannon Lake (limited), Samsung/TSMC volume production
  • 7 nm (2019): AMD Ryzen 3000, Apple A12, extreme ultraviolet (EUV) lithography
  • 5 nm (2020): Apple M1, AMD Ryzen 5000 (TSMC), advanced EUV
  • 3 nm (2022): Apple M2 Pro/Max (late 2022), Apple A17 (2023)
  • 2 nm (Development): Expected mid-2020s, pushing physical limits

Note: Modern "process nodes" (7nm, 5nm, 3nm) are marketing terms more than actual physical dimensions. A "5nm" chip doesn't necessarily have 5nm transistors; the smallest features may be 20-30nm. The naming reflects relative density improvements.

Contemporary Nanotechnology (2000-Present)

Nanomedicine:

  • Nanoparticle drug delivery: Liposomes, polymeric nanoparticles target tumors
  • mRNA vaccines (Pfizer-BioNTech, Moderna COVID-19 vaccines): Use lipid nanoparticles (~100nm) to deliver mRNA
  • Gold nanoparticles for cancer therapy, diagnostics
  • Quantum dots for biological imaging

Nanomaterials:

  • Graphene (2004 isolation by Andre Geim and Konstantin Novoselov): Single-atom-thick carbon sheet, extraordinary properties
  • Quantum dots: Semiconductor nanocrystals (2-10nm) that emit specific colors based on size
  • Aerogels: Ultra-low-density nanoporous materials

Consumer Applications:

  • Sunscreen: Titanium dioxide and zinc oxide nanoparticles (transparent, UV-blocking)
  • Anti-reflective coatings: Nanoporous silica on eyeglasses, displays
  • Stain-resistant fabrics: Nanoparticle coatings
  • Catalytic converters: Platinum nanoparticles

and Evolution

Pre-Parsec Era: The Parallax Quest (1600s-1830s)

The concept of stellar parallax dates to ancient Greek astronomy, but detecting it required centuries of technological advancement.

Galileo Galilei (1610) suggested that if Earth orbits the Sun, nearby stars should show annual parallax shifts against distant background stars. No parallax was detected, leading geocentrists to argue Earth must be stationary.

James Bradley (1728) discovered stellar aberration (apparent star position shifts due to Earth's orbital motion combined with finite light speed), confirming Earth's motion but still failing to detect parallax—stars were simply too distant.

Friedrich Wilhelm Bessel achieved the first successful parallax measurement in 1838 for 61 Cygni, determining a distance of about 10.3 light-years (3.16 parsecs, though the term didn't exist yet). This triumph came using a heliometer—a split-lens telescope enabling precise angular measurements.

Thomas Henderson measured Alpha Centauri's parallax (1832-1833, published 1839), and Friedrich Struve measured Vega's (1837), establishing parallax as the fundamental distance measurement method.

Coining the Term (1913)

Herbert Hall Turner (1861-1930), British astronomer and director of Oxford University Observatory, coined "parsec" in 1913. Before this, astronomers expressed stellar distances awkwardly:

  • In astronomical units (requiring numbers in the hundreds of thousands)
  • In light-years (popular but not directly tied to measurement method)
  • In "parallax seconds" (inverse of parallax angle, but confusing terminology)

Turner recognized that astronomers naturally thought in terms of parallax angles. For a star with parallax angle p (in arcseconds), the distance d is simply:

d (in parsecs) = 1 / p (in arcseconds)

This elegant relationship made the parsec immediately practical. A star with 0.5″ parallax is 2 parsecs away; 0.1″ parallax means 10 parsecs; 0.01″ parallax means 100 parsecs.

IAU Adoption (1922-1938)

The 1922 IAU General Assembly in Rome endorsed the parsec as the standard unit for stellar distances, though adoption wasn't immediate or universal.

The 1938 IAU General Assembly in Stockholm formally standardized the parsec definition based on the astronomical unit and arcsecond, solidifying its status.

By the 1950s, the parsec dominated professional astronomy literature, though popular science continued preferring light-years for general audiences.

Space Age Precision (1960s-Present)

Hipparcos satellite (1989-1993): European Space Agency mission measured parallaxes for 118,000 stars with milliarcsecond precision, extending reliable parsec-based distances to hundreds of parsecs.

Gaia mission (2013-present): ESA's Gaia spacecraft has revolutionized astrometry, measuring parallaxes for 1.8 billion stars with microarcsecond precision. This extends direct parsec measurements to 10,000+ parsecs (10+ kiloparsecs), mapping our galaxy's structure in unprecedented detail.

2012 IAU redefinition: The IAU redefined the astronomical unit as exactly 149,597,870,700 meters (no longer based on Earth's actual orbit, which varies slightly). This made the parsec exactly 648,000/π AU, providing a stable definition independent of Earth's orbital variations.

Common Uses and Applications: nanometers vs parsecs

Explore the typical applications for both Nanometer (metric) and Parsec (imperial/US) to understand their common contexts.

Common Uses for nanometers

of the Nanometer in Modern Contexts

1. Technology and Electronics

Semiconductors:

  • Process node naming (3nm, 5nm, 7nm chips)
  • Transistor gate lengths, interconnect widths
  • Thin film thicknesses (oxides, metals, dielectrics)

Displays:

  • QLED quantum dots (2-10 nm) for color purity
  • OLED organic layers (~100 nm thick)
  • Anti-reflective coatings (100-150 nm)

Data Storage:

  • Hard drive head-to-platter spacing (~3-5 nm flying height)
  • Magnetic domain sizes (~10-50 nm)
  • Flash memory cell feature sizes (~15-30 nm)

2. Optics and Photonics

Wavelength Specifications:

  • Laser wavelengths (UV: 193 nm, 248 nm, 355 nm; visible: 405 nm, 532 nm, 650 nm)
  • Optical filter bandwidths (specify transmission/reflection in nm ranges)
  • Spectroscopy (absorption/emission peaks reported in nanometers)

Thin Film Optics:

  • Anti-reflective coatings (multiple layers, each 50-150 nm)
  • Dichroic mirrors and filters (nanometer-scale multilayers)
  • Photonic crystals (periodic structures, 100-500 nm)

3. Materials Science and Nanotechnology

Nanoparticle Synthesis:

  • Specifying target particle size (gold nanoparticles: 5, 10, 20, 50, 100 nm)
  • Quantum dots (size determines optical properties)
  • Ceramic nanoparticles for catalysis, coatings

Thin Films and Coatings:

  • Physical vapor deposition (PVD), chemical vapor deposition (CVD)
  • Layer thicknesses: 1-1,000 nm
  • Atomic layer deposition (ALD): atomic-scale control (~0.1 nm/cycle)

Surface Characterization:

  • Atomic force microscopy (AFM) measures roughness in nanometers
  • Ellipsometry measures film thickness (0.1-1,000 nm range)
  • Scanning electron microscopy (SEM) images nanoscale features

4. Biology and Medicine

Molecular Dimensions:

  • Protein sizes (5-50 nm typical)
  • Virus dimensions (20-400 nm)
  • Cell membrane thickness (~7-10 nm lipid bilayer)

Nanomedicine:

  • Nanoparticle drug carriers (50-200 nm optimal for cellular uptake)
  • mRNA vaccine lipid nanoparticles (~100 nm)
  • Diagnostic nanoparticles (gold, quantum dots, magnetic)

Microscopy:

  • Electron microscopy resolution (TEM: 0.1-1 nm, SEM: 1-10 nm)
  • Super-resolution optical microscopy (breaks diffraction limit, ~20-50 nm resolution)

5. Environmental Science

Air Quality:

  • Ultrafine particles: < 100 nm diameter (penetrate deep into lungs)
  • PM 2.5: Particulate matter < 2,500 nm (2.5 μm) diameter
  • Nanoparticle pollutants from combustion, industrial processes

Water Filtration:

  • Nanofiltration membranes: pore sizes 1-10 nm (remove ions, small molecules)
  • Graphene oxide membranes: sub-nanometer channels for desalination

6. Metrology and Precision Measurement

Surface Roughness:

  • Optical surfaces: Roughness < 1 nm RMS (root mean square) for high quality
  • Semiconductor wafers: < 0.1 nm RMS for epitaxial growth

Film Thickness:

  • Quality control in manufacturing (coatings, semiconductors)
  • Techniques: Ellipsometry, X-ray reflectivity, profilometry

7. Research and Development

Nanoscience Research:

  • Synthesizing new nanomaterials with specific dimensions
  • Characterizing structure-property relationships
  • Exploring quantum effects at nanoscale

Academic Publications:

  • Specifying material dimensions (nanoparticle size, film thickness, feature size)
  • Nanometer is standard unit in materials science, nanotechnology, condensed matter physics

When to Use parsecs

Stellar Astronomy and Parallax Measurements

The parsec's primary use is measuring stellar distances via trigonometric parallax:

Parallax formula: d (parsecs) = 1 / p (arcseconds)

Ground-based observatories: Measure parallaxes to ~0.01″ accuracy, reliable to ~100 pc

Hipparcos satellite: Measured parallaxes to ~0.001″ (1 milliarcsecond), reliable to ~1,000 pc (1 kpc)

Gaia spacecraft: Measures parallaxes to ~0.00001″ (10 microarcseconds) for bright stars, reliable to ~10 kpc for many stars

Applications:

  • Calibrating the cosmic distance ladder (using Cepheid variables, RR Lyrae stars)
  • Determining absolute magnitudes of stars
  • Studying stellar populations and galactic structure
  • Measuring proper motions and space velocities

Galactic Structure and Dynamics

Kiloparsecs (kpc) describe structures within galaxies:

Milky Way structure:

  • Galactic center (Sagittarius A*): 8.2 kpc from Sun
  • Galactic disk radius: ~15 kpc
  • Central bulge: ~1.5 kpc radius
  • Spiral arms: trace patterns 10-15 kpc in radius
  • Dark matter halo: extends to ~60 kpc

Rotation curves: Plot orbital velocity vs. distance (in kpc) from galactic center, revealing dark matter

Star formation regions: Giant molecular clouds span 10-100 pc

Globular clusters: Orbit 10-60 kpc from galactic center

Extragalactic Astronomy

Megaparsecs (Mpc) measure distances between galaxies:

Galaxy surveys: Map millions of galaxies to distances of 1,000+ Mpc, revealing large-scale structure (walls, filaments, voids)

Tully-Fisher relation: Links galaxy rotation speed to luminosity, enabling distance estimates in Mpc

Type Ia supernovae: Standard candles for measuring distances to 1,000+ Mpc

Galaxy clusters: Typical separation between major clusters ~10-50 Mpc

Superclusters: Structures spanning 100-200 Mpc (like Laniakea Supercluster containing Milky Way)

Cosmology and Universe Expansion

Megaparsecs and gigaparsecs describe cosmological distances:

Hubble constant (H₀): Measured in km/s per Mpc—describes universe expansion rate

  • Current value: H₀ ≈ 67-73 (km/s)/Mpc (tension between measurement methods)
  • Interpretation: Galaxy 1 Mpc away recedes at ~70 km/s; 100 Mpc away recedes at ~7,000 km/s

Hubble's Law: v = H₀ × d (where d is in Mpc, v is recession velocity)

Comoving distance: Cosmological distance accounting for universe expansion, measured in Mpc or Gpc

Redshift surveys: Map galaxy distribution to 1,000+ Mpc (z ~ 0.1-0.3 redshift)

Baryon acoustic oscillations: ~150 Mpc characteristic scale in galaxy distribution, used as "standard ruler"

Astrophysical Research Papers

Parsecs are the default distance unit in professional astronomy journals:

Observational papers: Report star/galaxy distances in pc, kpc, or Mpc

Theoretical models: Express scale lengths in parsecs (e.g., "disk scale length of 3 kpc")

Computer simulations: Use parsec-based units (or comoving kpc/Mpc for cosmological sims)

Standard convention: Professional astronomers think and calculate in parsecs, converting to light-years only for public communication

Additional Unit Information

About Nanometer (nm)

1. How small is a nanometer?

A nanometer is extraordinarily small—one billionth of a meter (0.000000001 m). To grasp this scale: A human hair is about 80,000-100,000 nm wide, so you could fit 80,000-100,000 nanometers across a single hair. A sheet of paper is ~100,000 nm thick. The DNA double helix is 2 nm wide. A typical protein molecule is 5-50 nm. A single gold atom is ~0.3 nm diameter, so 1 nanometer spans approximately 3-4 atoms. If a nanometer were enlarged to 1 centimeter, a meter would stretch 10,000 kilometers—farther than the distance from New York to Tokyo. At this scale, quantum mechanical effects dominate: electrons behave as waves, particles can tunnel through barriers, and material properties become size-dependent.

2. How many nanometers are in a micrometer?

There are exactly 1,000 nanometers in 1 micrometer (μm). The relationship: 1 μm = 1,000 nm, or 1 nm = 0.001 μm. This factor of 1,000 comes from the metric prefix system: micro (μ) = 10⁻⁶ and nano (n) = 10⁻⁹, so 10⁻⁶ ÷ 10⁻⁹ = 10³ = 1,000. Examples: A typical bacterium (E. coli) is 2 μm long = 2,000 nm. A red blood cell is 7-8 μm diameter = 7,000-8,000 nm. A virus is 20-400 nm = 0.02-0.4 μm. Human hair is 80 μm = 80,000 nm. The nanometer-to-micrometer boundary (~100-1,000 nm) roughly separates the realm of individual molecules and nanoparticles (nm) from the realm of cells and microorganisms (μm).

3. Why are nanometers important in technology?

Nanometers are the scale at which quantum mechanical effects emerge, enabling revolutionary technologies. At 1-100 nm, materials exhibit size-dependent properties impossible to achieve in bulk: gold nanoparticles turn red; semiconductor quantum dots emit precise colors based on size; carbon nanotubes become stronger than steel. Semiconductor chips have shrunk to 3-5nm process nodes, packing billions of transistors into fingernail-sized dies—enabling smartphones, AI, cloud computing. Nanometer precision allows atomic layer deposition (building materials atom-by-atom), molecular diagnostics (detecting single protein molecules), targeted drug delivery (100nm nanoparticles accumulate in tumors), and metamaterials (nanoscale structures that bend light impossibly). The nanometer sits at the sweet spot: large enough to fabricate with advanced tools (electron beam lithography, STM manipulation), small enough to exploit quantum effects and interact with individual molecules—making it the frontier of 21st-century technology.

4. What's the difference between a nanometer and an angstrom?

A nanometer (nm) equals 10 angstroms (Å). The angstrom (1 Å = 0.1 nm = 10⁻¹⁰ meters) was historically used in atomic physics, chemistry, and crystallography because atomic diameters and chemical bond lengths conveniently fall in the 1-5 Å range (hydrogen atom: ~1 Å, carbon-carbon bond: 1.54 Å). However, the angstrom is not an SI unit, and modern scientific practice favors nanometers and picometers. Example: The diameter of a DNA double helix is 2 nm = 20 Å. The spacing between DNA base pairs is 0.34 nm = 3.4 Å. A silicon atom is 0.21 nm = 2.1 Å diameter. While older papers and crystallography software often report structures in angstroms, nanometers are now standard in nanotechnology, materials science, and most contemporary research. If you see Å, just divide by 10 to convert to nanometers.

5. Can you see something that's 1 nanometer?

No, you cannot see 1 nanometer with any optical microscope, and barely even with your eyes' theoretical maximum resolution. Human eyes can resolve ~50-100 micrometers (50,000-100,000 nm) at best. Optical microscopes are limited by the diffraction limit—approximately half the wavelength of light used. Visible light ranges 400-700 nm, so the best optical resolution is ~200-300 nm (using UV light and oil immersion). To "see" 1 nm structures, you need: Transmission Electron Microscope (TEM): Uses electron beams (wavelength ~0.01 nm at high voltage), achieving 0.1-1 nm resolution—can image individual atoms. Scanning Tunneling Microscope (STM) or Atomic Force Microscope (AFM): "Feel" surfaces by scanning a sharp tip (1-atom-wide apex) across the sample, mapping topography with sub-nanometer precision. So yes, we can "see" nanometer and sub-nanometer features, but not with light—we use electrons or physical probes.

6. Why are modern chips called "3nm" or "5nm" when features aren't actually that small?

Modern process node names (3nm, 5nm, 7nm) are marketing terms reflecting relative density improvements, not actual physical dimensions. Historically, process nodes indicated the smallest feature size (e.g., Intel's 130nm process in 2001 had ~130nm gate lengths). But as scaling slowed and 3D transistor designs (FinFETs) emerged, the relationship broke down. Today: A "5nm" chip from TSMC might have gate lengths ~20-30nm, metal pitch ~30-40nm, and the tightest pitch structures ~24-28nm. The "5nm" refers roughly to an equivalent density compared to hypothetical scaling trends. A "3nm" chip is denser than "5nm," but actual dimensions are larger than 3nm. Why keep the naming? Industry convention, marketing (smaller number sounds more advanced), and rough correlation with transistor density. Different manufacturers' "5nm" may differ significantly. Bottom line: Process nodes indicate generation and relative performance/density, not literal nanometer measurements.

7. What's the smallest thing ever manipulated by humans?

Humans have manipulated individual atoms (~0.1-0.3 nm), the smallest stable units of matter. 1989: IBM scientists used a Scanning Tunneling Microscope (STM) to arrange 35 xenon atoms to spell "IBM" on a nickel surface—the first atomic-scale manipulation. 1990s-present: Researchers built molecular structures atom-by-atom: molecular gears, switches, quantum corrals (rings of atoms to confine electrons). 2012: Physicists stored 1 bit of data in a single holmium atom (~0.25 nm diameter) using magnetic orientation. Subatomic particles: Particle accelerators (LHC) manipulate protons (~0.0016 nm diameter) and study quarks (~10⁻³ to 10⁻⁴ nm, though quarks can't be isolated). Quantum engineering: Controlling individual electron spins, photon states, and qubits for quantum computing. So while atoms (~0.1-0.3 nm) are the smallest stable structures we manipulate routinely, we probe and control phenomena down to 10⁻⁵ nm scales in particle physics.

8. How does nanotechnology differ from regular technology?

Nanotechnology operates at 1-100 nm scale where quantum mechanical effects become significant and surface-area-to-volume ratios are enormous, enabling properties impossible in bulk materials. Differences: Scale: Nanotech manipulates individual molecules, atoms, or nanostructures; regular tech uses bulk materials. Quantum effects: At nanoscale, quantum tunneling, quantized energy levels, and wave-particle duality dominate; bulk materials follow classical physics. Size-dependent properties: Gold nanoparticles (5-50 nm) are red/purple and reactive; bulk gold is yellow and inert. Quantum dots (2-10 nm) emit precise colors tuned by size—impossible with bulk semiconductors. Surface area: Nanoparticles have immense surface area relative to volume, making them superb catalysts, drug carriers, and sensors. Bottom-up assembly: Nanotech often uses molecular self-assembly or atom-by-atom fabrication; traditional manufacturing is top-down (machining, cutting). Applications: Nanotech enables mRNA vaccines (lipid nanoparticles), 3nm computer chips, targeted cancer therapy, and quantum computing—revolutionary advances impossible with conventional approaches.

9. Is nanotechnology safe?

Nanotechnology safety is highly material-specific—some nanomaterials are safe, others pose risks. Concerns: 1) Toxicity: Some nanoparticles (carbon nanotubes, certain metal oxides) can damage cells, cause inflammation, or penetrate biological barriers (blood-brain barrier). Silver nanoparticles, widely used in antimicrobial products, can harm aquatic life. 2) Environmental persistence: Nanoparticles may accumulate in ecosystems with unknown long-term effects. 3) Inhalation: Ultrafine airborne nanoparticles (~10-100 nm) penetrate deep into lungs, potentially causing respiratory issues. Safety measures: Extensive testing: New nanomaterials undergo toxicology studies before commercial use. Regulation: FDA, EPA, EU regulate nanomaterials in drugs, food, cosmetics, and industrial applications. Encapsulation: Many nanoparticles (e.g., in sunscreen, food) are embedded in matrices, preventing release. Established safety: Some nanomaterials are demonstrably safe (titanium dioxide and zinc oxide in sunscreen used for decades; lipid nanoparticles in mRNA vaccines tested extensively). Conclusion: Nanotech isn't universally safe or dangerous—each material requires careful evaluation.

10. How do semiconductor fabs create nanometer-scale features?

Modern semiconductor fabrication uses photolithography with extreme precision and multi-step patterning. Extreme Ultraviolet (EUV) Lithography: Uses 13.5 nm wavelength light (generated by tin plasma) to pattern features. Wavelength is much smaller than older 193 nm UV lithography, enabling finer patterns. Process: 1) Coat silicon wafer with photoresist (~50-100 nm layer). 2) Project circuit pattern onto resist using EUV light through precision optics. 3) Exposed resist dissolves, leaving pattern. 4) Etch exposed silicon, deposit materials, etc. 5) Repeat hundreds of times (modern chips: 20-25+ mask layers). Multi-patterning: Single exposure can't achieve tightest pitches, so features are created through multiple aligned exposures (self-aligned double patterning, etc.). Atomic Layer Deposition (ALD): Deposits ultra-thin films (~0.1-1 nm precision) for gates, insulators. FinFET 3D transistors: Vertical silicon fins (~5-7 nm wide) provide better gate control at nanoscale. Extreme precision: Alignment accuracy: ~1-2 nm. Temperature control: ±0.01°C. Cleanrooms: <1 particle/cubic meter. Took decades of R&D and billions in equipment development to achieve 3-5nm nodes.

11. What's the limit of miniaturization in computer chips?

Miniaturization faces several fundamental limits expected to halt around 1-2 nm nodes (late 2020s-early 2030s): 1) Atomic scale: Silicon atoms are ~0.21 nm diameter. At 1-2 nm features, structures are just 5-10 atoms wide—difficult to control dopant placement and variability. 2) Quantum tunneling: Electrons can "tunnel" through barriers < 1-2 nm thick, causing leakage current and preventing transistors from turning off. 3) Heat dissipation: Power density in chips approaches limits of cooling technology. Shrinking further increases current density and heat. 4) Manufacturing precision: Atomic-level variations affect device performance. Placing individual dopant atoms precisely is extremely difficult. Beyond silicon: Future options include: New materials (carbon nanotubes, graphene, 2D materials). 3D stacking (vertical integration). New transistor architectures (gate-all-around FETs, tunnel FETs). Beyond CMOS (quantum computing, photonic computing, neuromorphic chips). Moore's Law (doubling transistor count every 2 years) is already slowing. The 1 nm node may be the practical limit for silicon, necessitating entirely new computing paradigms.

12. Can nanotechnology create molecular machines?

Yes! Molecular machines—nanometer-scale structures that perform mechanical work—exist naturally and are being engineered artificially. Natural molecular machines: Ribosomes (~20 nm): Synthesize proteins, translating mRNA into amino acid chains (Nobel Prize 2009 for structure determination). ATP synthase (~10 nm): Rotary motor in mitochondria, spins at ~100 Hz to produce ATP (cellular energy currency). Kinesin motors (~10 nm): "Walk" along microtubules, transporting cargo within cells. DNA polymerase: Copies DNA, moving along strands, proof-reading, and assembling nucleotides. Synthetic molecular machines (Nobel Prize in Chemistry 2016): Molecular motors: Light-driven rotors, chemically-driven linear motors (synthesized by Fraser Stoddart, Jean-Pierre Sauvage, Ben Feringa). DNA origami machines: Programmable nanoscale structures that fold, unfold, or grasp objects. Potential applications: Nanoscale drug delivery, molecular computing, self-assembling materials, targeted cell repair. Challenges: Operating in biological environments, controlling motion precisely, scaling up production. Molecular machines are early-stage but represent frontier of nanotechnology.


About Parsec (pc)

What does "parsec" stand for?

Parsec is a portmanteau of "parallax of one arcsecond."

It represents the distance at which Earth's orbital radius (1 AU) subtends an angle of exactly one arcsecond (1/3600 of a degree). British astronomer Herbert Hall Turner coined the term in 1913 to provide a convenient unit directly tied to the parallax measurement method.

How is a parsec measured?

Parsecs are measured using trigonometric parallax:

  1. Observe a nearby star from Earth when Earth is on one side of its orbit
  2. Observe the same star six months later when Earth is on the opposite side
  3. Measure the apparent shift in the star's position against distant background stars
  4. Half this shift is the parallax angle p (in arcseconds)
  5. Calculate distance: d = 1/p parsecs

Modern method: Space telescopes like Gaia measure parallax angles with microarcsecond precision, enabling distance measurements to thousands of parsecs.

Is a parsec bigger than a light-year?

Yes, one parsec is significantly larger:

1 parsec ≈ 3.26 light-years

More precisely: 1 pc = 3.261563777 ly

Example: Proxima Centauri at 1.3 parsecs equals 4.24 light-years away.

Why the difference matters: Confusing parsecs with light-years introduces 3× error in distances.

Why do astronomers prefer parsecs over light-years?

Astronomers prefer parsecs for several reasons:

1. Direct observational connection: Parallax angle p (arcseconds) directly gives distance d = 1/p (parsecs). No complicated conversion needed.

2. Professional standard: IAU endorsed parsecs in 1922; they're now universal in research papers and textbooks.

3. Convenient multiples: Kiloparsecs (kpc) for galactic distances, megaparsecs (Mpc) for cosmological distances provide natural scales.

4. Hubble constant units: Universe expansion rate naturally expressed in (km/s)/Mpc.

5. Definition stability: Light-year depends on year length definition (tropical, Julian, sidereal); parsec defined purely by geometry.

Light-years remain popular in public communication because "year" is familiar, while "parallax arcsecond" requires technical knowledge.

How many astronomical units are in a parsec?

1 parsec = 206,265 astronomical units (AU) (approximately)

More precisely: 1 pc = 206,264.806247 AU

This number arises from: 1 pc = 1 AU / tan(1″), and since 1″ = π/648,000 radians:

  • 1 pc = 1 AU / (π/648,000) = 648,000/π AU ≈ 206,265 AU

Context: Since 1 AU ≈ 150 million km (Earth-Sun distance), 1 parsec ≈ 31 trillion km.

What is a kiloparsec and megaparsec?

Kiloparsec (kpc): 1 kpc = 1,000 parsecs ≈ 3,262 light-years

  • Used for: Galactic-scale distances
  • Examples: Sun to Milky Way center (8 kpc), galaxy diameters (10-50 kpc)

Megaparsec (Mpc): 1 Mpc = 1,000,000 parsecs ≈ 3.26 million light-years

  • Used for: Intergalactic distances, cosmology
  • Examples: Andromeda Galaxy (0.77 Mpc), Virgo Cluster (16.5 Mpc), Hubble constant measured in (km/s)/Mpc

Gigaparsec (Gpc): 1 Gpc = 1,000,000,000 parsecs ≈ 3.26 billion light-years

  • Used for: Large-scale cosmological structures
  • Example: Observable universe radius (~14 Gpc)

Is the parsec an SI unit?

No, the parsec is not an SI unit. The SI unit of length is the meter (m).

However, the parsec is:

  • Recognized by the IAU (International Astronomical Union)
  • Accepted for use with SI in astronomy contexts
  • Defined exactly in terms of the AU (which is defined exactly in meters)

Why not SI?: The parsec arose naturally from astronomical practice and remains far more practical than expressing stellar distances in meters (which would require numbers like 10¹⁶ to 10²³).

Analogy: Like the electronvolt (eV) in particle physics, the parsec is a specialized unit indispensable to its field despite not being SI.

How far can parallax measure distances?

Ground-based telescopes: ~0.01 arcsecond precision → reliable to ~100 parsecs

Hubble Space Telescope: ~0.001 arcsecond (1 milliarcsecond) → reliable to ~1,000 parsecs (1 kpc)

Hipparcos satellite (1989-1993): ~0.001 arcsecond → 118,000 stars measured to 100-1,000 pc

Gaia spacecraft (2013-present): ~0.00001 arcsecond (10 microarcseconds) for bright stars → reliable to ~10,000 parsecs (10 kpc)

  • Measured 1.8 billion stars
  • Revolutionary precision enables mapping entire Milky Way disk

Fundamental limit: Stars beyond 10-20 kpc have unmeasurably small parallaxes with current technology. For greater distances, astronomers use indirect methods (Cepheids, Type Ia supernovae, redshift).

Did Han Solo make the Kessel Run in "less than 12 parsecs"?

Famous Star Wars quote: "She made the Kessel Run in less than twelve parsecs."

The issue: Parsec measures distance, not time. Saying "less than 12 parsecs" for a speed achievement is like saying "I drove to work in less than 5 miles."

Fan explanations (retroactive justifications):

  • The Kessel Run involves navigating near black holes; a shorter distance means a more dangerous, direct route
  • Skilled pilots can shave distance by flying closer to gravitational hazards
  • This reinterprets "12 parsecs" as boasting about route optimization, not speed

Real answer: George Lucas likely confused parsecs with a time unit when writing the script. The line became famous enough that later writers invented explanations making it technically correct.

Takeaway: In real astronomy, parsecs always measure distance, never time.

How do parsecs relate to the Hubble constant?

The Hubble constant (H₀) describes universe expansion and is typically expressed as:

H₀ ≈ 70 (km/s)/Mpc

Interpretation: For every megaparsec of distance, recession velocity increases by ~70 km/s.

Examples using Hubble's Law (v = H₀ × d):

  • Galaxy 1 Mpc away: recedes at ~70 km/s
  • Galaxy 10 Mpc away: recedes at ~700 km/s
  • Galaxy 100 Mpc away: recedes at ~7,000 km/s
  • Galaxy 1,000 Mpc away: recedes at ~70,000 km/s

Hubble length: c/H₀ ≈ 4,400 Mpc (14.4 billion ly) - characteristic distance scale of observable universe

Why Mpc?: Using megaparsecs keeps Hubble constant values convenient (70 rather than 0.000000000070 if using parsecs, or 2.3 × 10⁻¹⁸ if using SI meters).

What's the farthest distance ever measured in parsecs?

Observable universe radius: ~14,000 Mpc = 14 Gpc (46 billion light-years comoving distance)

Most distant galaxy observed (as of 2023): JADES-GS-z13-0 at redshift z ≈ 13.2

  • Comoving distance: ~4,200 Mpc (13.7 billion light-years light-travel distance)
  • Due to universe expansion, it's now ~10,000 Mpc (32 billion light-years) away

Cosmic microwave background: Emitted 380,000 years after Big Bang

  • Comoving distance to CMB surface: ~14,000 Mpc (46 billion light-years)

Beyond measurement: The observable universe has a finite size (~14 Gpc radius) due to finite age and light speed. Objects beyond this "cosmological horizon" are unobservable because their light hasn't reached us yet.

Conversion Table: Nanometer to Parsec

Nanometer (nm)Parsec (pc)
0.50
10
1.50
20
50
100
250
500
1000
2500
5000
1,0000

People Also Ask

How do I convert Nanometer to Parsec?

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What is the conversion factor from Nanometer to Parsec?

The conversion factor depends on the specific relationship between Nanometer and Parsec. 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 Parsec back to Nanometer?

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What are common uses for Nanometer and Parsec?

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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: December 3, 2025