Second to Planck Time Converter

What is Planck Time?

Planck time (symbol: tP) is a fundamental unit of time in the Planck system of natural units, representing the time required for light traveling at speed c (the speed of light in vacuum) to traverse a distance of one Planck length (ℓP).

Mathematical definition:

tP = √(ℏG/c⁵)

Where:

• ℏ (h-bar) = reduced Planck constant = 1.054571817 × 10⁻³⁴ J·s
• G = gravitational constant = 6.67430 × 10⁻¹¹ m³/(kg·s²)
• c = speed of light in vacuum = 299,792,458 m/s (exact)

Numerical value:

tP ≈ 5.391247 × 10⁻⁴⁴ seconds

Or written out in full: 0.000000000000000000000000000000000000000000053912 seconds

Alternative calculation (from Planck length):

tP = ℓP / c

Where:

• ℓP = Planck length ≈ 1.616255 × 10⁻³⁵ meters
• c = speed of light ≈ 2.998 × 10⁸ m/s

This gives: tP ≈ 1.616 × 10⁻³⁵ m ÷ 2.998 × 10⁸ m/s ≈ 5.39 × 10⁻⁴⁴ s

Physical Significance

Planck time represents several profound concepts in physics:

1. Shortest meaningful time interval:

• Below Planck time, the uncertainty principle combined with general relativity makes the very concept of time measurement meaningless
• Energy fluctuations ΔE required to measure sub-Planck-time intervals would create black holes that obscure the measurement

2. Quantum gravity timescale:

• At durations approaching Planck time, quantum effects of gravity become comparable to other quantum effects
• Spacetime curvature fluctuates quantum-mechanically
• Classical smooth spacetime breaks down into "quantum foam"

3. Fundamental temporal quantum:

• Some theories (loop quantum gravity, causal sets) suggest time may be fundamentally discrete at the Planck scale
• Continuous time may be an emergent property valid only above Planck time
• Spacetime may consist of discrete "chronons" of duration ~tP

4. Cosmological boundary:

• The Planck epoch (0 to ~10⁻⁴³ s after Big Bang) is the earliest era describable only by a theory of quantum gravity
• Before ~1 Planck time after the Big Bang, our current physics cannot make predictions

Why Planck Time is a Limit

Heisenberg Uncertainty Principle + General Relativity:

To measure a time interval Δt with precision, you need energy uncertainty ΔE where:

ΔE · Δt ≥ ℏ/2

For extremely small Δt (approaching Planck time), the required ΔE becomes enormous:

ΔE ≈ ℏ/Δt

When Δt → tP, the energy ΔE becomes so large that:

ΔE/c² ≈ mP (Planck mass ≈ 2.18 × 10⁻⁸ kg)

This mass concentrated in a region of size ℓP (Planck length) creates a black hole with Schwarzschild radius comparable to ℓP, making measurement impossible—the measurement apparatus itself becomes a black hole that obscures what you're trying to measure!

Conclusion: You cannot meaningfully measure or discuss events happening faster than Planck time because the act of measurement destroys the very spacetime you're trying to probe.

Planck Time vs. Other Small Times

Planck time is incomprehensibly smaller than any directly measurable duration:

Attosecond (10⁻¹⁸ s):

• Shortest time intervals directly measured by physicists (attosecond laser pulses)
• 10²⁶ times longer than Planck time
• Used to study electron motion in atoms

Zeptosecond (10⁻²¹ s):

• Time for light to cross a hydrogen molecule
• 10²³ times longer than Planck time
• Measured in 2020 experiments

Chronon (hypothetical):

• Proposed discrete time quantum in some theories
• Possibly equal to Planck time (5.39 × 10⁻⁴⁴ s)
• Unproven experimentally

Planck time is to one second as one second is to ~10²⁶ times the age of the universe!

Natural Units and Dimensional Analysis

In Planck units (also called natural units), fundamental constants are set to 1:

• c = 1 (speed of light)
• ℏ = 1 (reduced Planck constant)
• G = 1 (gravitational constant)
• kB = 1 (Boltzmann constant, sometimes)

In this system:

• Planck time = 1 tP (the fundamental unit)
• Planck length = 1 ℓP
• Planck mass = 1 mP
• All physical quantities expressed as dimensionless ratios

Example: The age of the universe ≈ 4.35 × 10¹⁷ seconds ≈ 8 × 10⁶¹ tP (in Planck units)

Advantage: Equations simplify dramatically. Einstein's field equations become cleaner, and fundamental relationships emerge more clearly.

Disadvantage: Numbers become extremely large (for macroscopic phenomena) or extremely small (for everyday quantum phenomena), making intuitive understanding difficult.

Max Planck and the Birth of Natural Units (1899-1900)

1899: Planck's Blackbody Radiation Problem

Max Planck was investigating blackbody radiation—the spectrum of light emitted by hot objects. Classical physics (Rayleigh-Jeans law) predicted infinite energy at short wavelengths (the "ultraviolet catastrophe"), which obviously didn't match experiments.

October 1900: Planck's Quantum Hypothesis

To resolve this, Planck proposed that energy is emitted in discrete packets (quanta):

E = hν

Where:

• E = energy of quantum
• h = Planck's constant ≈ 6.626 × 10⁻³⁴ J·s
• ν = frequency of radiation

This radical idea—energy quantization—launched quantum mechanics.

1899: Planck Derives Natural Units

While developing his theory, Planck realized he could define fundamental units using only universal constants, independent of human conventions:

Planck's original natural units:

1. Planck length: ℓP = √(ℏG/c³) ≈ 1.616 × 10⁻³⁵ m
2. Planck mass: mP = √(ℏc/G) ≈ 2.176 × 10⁻⁸ kg
3. Planck time: tP = √(ℏG/c⁵) ≈ 5.391 × 10⁻⁴⁴ s
4. Planck temperature: TP = √(ℏc⁵/Gk²B) ≈ 1.417 × 10³² K

Planck's 1899 statement:

"These necessarily retain their meaning for all times and for all civilizations, including extraterrestrial and non-human ones, and can therefore be designated as 'natural units.'"

Planck recognized these weren't practical units for measurement but represented fundamental scales where quantum effects (ℏ), gravity (G), and relativity (c) all become equally important.

Irony: Planck himself thought his quantum hypothesis was a temporary mathematical trick, not a fundamental truth. He spent years trying to eliminate the quantum from his theory, unaware he'd discovered one of physics' deepest principles!

Early Quantum Mechanics: Ignoring Planck Units (1900-1950s)

For the first half of the 20th century, physicists focused on developing quantum mechanics and general relativity as separate theories:

Quantum Mechanics (1900s-1930s):

• Bohr model (1913)
• Schrödinger equation (1926)
• Heisenberg uncertainty principle (1927)
• Dirac equation (1928)
• Quantum electrodynamics (1940s)

No gravity involved—Planck time seemed irrelevant.

General Relativity (1915-1950s):

• Einstein's field equations (1915)
• Black holes (Schwarzschild 1916, Kerr 1963)
• Expanding universe (Hubble 1929)
• Big Bang cosmology (Lemaître 1927, Gamow 1948)

No quantum mechanics involved—Planck time seemed irrelevant.

Problem: The two theories use incompatible frameworks:

• Quantum mechanics: Probabilistic, discrete, uncertainty principle
• General relativity: Deterministic, continuous, smooth spacetime

At normal scales, you can use one or the other. But at Planck scales (Planck time, Planck length), you need both simultaneously—and they clash!

John Wheeler and Quantum Foam (1950s-1960s)

1955: John Archibald Wheeler's Quantum Geometry

Princeton physicist John Wheeler began exploring what happens when quantum mechanics meets general relativity at extreme scales.

Wheeler's key insight (1955): At the Planck scale, spacetime itself undergoes quantum fluctuations, creating a foamy, turbulent structure he called "quantum foam" or "spacetime foam."

Quantum Foam visualization:

• At durations longer than Planck time: Spacetime appears smooth
• At durations approaching Planck time: Spacetime becomes violently fluctuating
• Virtual black holes constantly form and evaporate
• Wormholes appear and disappear
• Topology of space changes randomly

Wheeler (1957):

"At very small distances and times, the very structure of spacetime becomes foam-like, with quantum fluctuations creating and destroying tiny wormholes."

Significance of Planck time:

• Below tP, the concept of a fixed spacetime background breaks down
• Geometry itself becomes a quantum variable
• Time may not even be fundamental—could emerge from deeper, timeless quantum processes

1967: Wheeler coins "black hole"

Wheeler's work on extreme gravity (black holes) and quantum mechanics (uncertainty) converged at Planck scales, making Planck time a central concept in quantum gravity.

Big Bang Cosmology and the Planck Epoch (1960s-1980s)

1965: Cosmic Microwave Background Discovered

Penzias and Wilson detect CMB radiation, confirming Big Bang theory. Cosmologists trace the universe backward in time toward the initial singularity.

The Planck Epoch Problem:

Standard Big Bang cosmology describes:

• t = 10⁻⁴³ s (near Planck time): Universe extremely hot (~10³² K), quantum gravity dominates
• t = 10⁻³⁵ s: Electroweak unification breaks, inflation begins (possibly)
• t = 10⁻¹¹ s: Quark-gluon plasma forms
• t = 1 s: Nucleosynthesis begins (protons, neutrons form)

But before t ≈ 10⁻⁴³ s (the Planck epoch):

• General relativity predicts a singularity (infinite density, infinite curvature)
• Quantum mechanics says you can't have infinite precision (uncertainty principle)
• Our physics breaks down!

Conclusion: The Planck epoch (from t = 0 to t ≈ tP) is the ultimate frontier—we need quantum gravity to describe it, but we don't have a complete theory yet.

1970s-1980s:

• Inflation theory (Alan Guth, 1980): Exponential expansion possibly beginning near Planck time
• Hawking radiation (Stephen Hawking, 1974): Black holes evaporate quantum-mechanically, connecting quantum mechanics and gravity
• No-boundary proposal (Hartle-Hawking, 1983): Time may become space-like before Planck time, eliminating the initial singularity

String Theory and Loop Quantum Gravity (1980s-2000s)

Two major approaches to quantum gravity emerged, both treating Planck time as fundamental:

String Theory (1980s-present):

Core idea: Fundamental entities are 1-dimensional "strings" vibrating in 10 or 11 dimensions, not point particles.

Planck time significance:

• Strings have characteristic length ~Planck length, vibration period ~Planck time
• Below Planck time, spacetime may have extra compactified dimensions
• String interactions occur on timescales of Planck time

Predictions:

• Minimum measurable time ≈ Planck time (spacetime uncertainty relation)
• Smooth spacetime emerges only above Planck scale

Loop Quantum Gravity (1980s-present):

Core idea: Spacetime itself is quantized—space is a network of discrete loops (spin networks), time consists of discrete steps.

Planck time significance:

• Fundamental "quantum of time" is exactly Planck time
• Below Planck time, continuous time doesn't exist
• Time evolution proceeds in discrete jumps of tP

Predictions:

• Planck time is the smallest possible duration
• Big Bang singularity replaced by a "Big Bounce" occurring at Planck-scale densities

Current status (2024): Neither theory is experimentally confirmed. Both agree Planck time marks the limit of classical spacetime.

Modern Developments (2000s-Present)

2010s: Causal Set Theory

Proposal: Spacetime is fundamentally a discrete set of events (points) with causal relations, not a continuous manifold.

Planck time: Natural timescale for spacing between discrete events.

2015: Planck Satellite Data

ESA's Planck satellite measures cosmic microwave background with unprecedented precision, probing conditions at t ≈ 10⁻³⁵ s after Big Bang—still 9 orders of magnitude later than Planck time, but the closest we've ever looked to the beginning.

2020s: Quantum Gravity Phenomenology

Physicists search for testable predictions of quantum gravity effects:

• Modified dispersion relations for light (different colors travel at slightly different speeds over cosmic distances)
• Violations of Lorentz invariance at Planck scale
• Quantum fluctuations of spacetime affecting gravitational wave signals

No conclusive evidence yet, but experiments are improving.

Current understanding:

• Planck time is universally accepted as the boundary where quantum gravity becomes necessary
• No experiment will ever directly probe Planck time (would require particle colliders the size of galaxies!)
• Theoretical understanding remains incomplete—quantum gravity is one of physics' greatest unsolved problems

1. Theoretical Physics and Quantum Gravity

Primary use: Planck time defines the scale where quantum gravity effects become important.

String Theory:

• Fundamental strings have vibration modes with periods ~Planck time
• String interactions (splitting, joining) occur on Planck-time timescales
• Calculations use Planck time as the natural unit

Loop Quantum Gravity:

• Discrete time steps ("chronons") of duration Planck time
• Spacetime evolution proceeds in jumps of tP
• Continuous time is emergent approximation above Planck scale

Causal Set Theory:

• Discrete spacetime events separated by intervals ~Planck time
• Fundamental structure: causal relations between events, not continuous time

Quantum Foam Models:

• Virtual black holes form and evaporate on Planck-time timescales
• Spacetime topology fluctuates with characteristic time ~tP

All quantum gravity approaches treat Planck time as the fundamental temporal quantum.

2. Early Universe Cosmology (Planck Epoch)

The Planck Epoch: From Big Bang singularity to t ≈ 10⁻⁴³ seconds

Why it matters:

• Before ~tP, standard cosmology (general relativity) breaks down
• Conditions: Temperature ~10³² K, energy density ~10¹¹³ J/m³
• All four forces (gravity, electromagnetic, strong, weak) were unified
• Physics: Requires quantum gravity—no complete theory exists

Modern cosmological models:

Inflationary cosmology:

• Some models have inflation beginning near Planck time
• Exponential expansion may solve horizon and flatness problems
• Planck-scale quantum fluctuations seed later galaxy formation

Cyclic/Ekpyrotic models:

• Universe may undergo cycles of expansion and contraction
• "Bounce" at Planck-scale densities, avoiding singularity
• Planck time sets timescale for bounce

Quantum cosmology (Hartle-Hawking):

• "No-boundary proposal": Universe has no beginning, time becomes space-like before Planck time
• Planck time marks transition from Euclidean (imaginary time) to Lorentzian (real time) spacetime

Observational consequence: We can never directly observe the Planck epoch—it's forever hidden behind the opaque plasma of the early universe. Our best observations (CMB) reach back to ~380,000 years after Big Bang, billions of orders of magnitude later than Planck time.

3. Black Hole Physics

Schwarzschild radius and Planck mass:

A black hole with mass equal to Planck mass (mP ≈ 2.18 × 10⁻⁸ kg) has:

• Schwarzschild radius = 2GmP/c² ≈ Planck length (ℓP ≈ 1.62 × 10⁻³⁵ m)
• Light crossing time = ℓP/c ≈ Planck time (tP ≈ 5.39 × 10⁻⁴⁴ s)

Significance: Planck-mass black holes are the smallest possible black holes before quantum effects dominate.

Hawking radiation timescale:

Black holes evaporate via Hawking radiation. Evaporation time:

tevap ≈ (5120π/ℏc⁴) × G² M³

For Planck-mass black hole (M = mP):

tevap ≈ tP (approximately Planck time!)

Meaning: The smallest quantum black holes evaporate in about one Planck time—they're extremely short-lived.

Larger black holes:

• Solar-mass black hole (M☉ = 2 × 10³⁰ kg): tevap ≈ 10⁶⁷ years
• Supermassive black hole (10⁹ M☉): tevap ≈ 10¹⁰⁰ years (googol years)

Near the singularity: Deep inside a black hole, approaching the singularity, spacetime curvature becomes extreme. At distances ~Planck length from the singularity, quantum gravity effects on timescales ~Planck time become important. Classical general relativity predicts infinite curvature; quantum gravity (unknown) likely prevents true singularity.

4. Limits of Measurement and Computation

Heisenberg Uncertainty Principle:

To measure time interval Δt with energy uncertainty ΔE:

ΔE · Δt ≥ ℏ/2

For Δt = tP:

ΔE ≈ ℏ/(2tP) ≈ mPc² (Planck energy ≈ 10⁹ J)

Problem: This energy concentrated in a Planck-length region creates a black hole, making measurement impossible.

Conclusion: Planck time is the fundamental limit on time measurement precision.

Bremermann's limit (computational speed):

Maximum rate of information processing for a self-contained system of mass M:

Rate ≤ 2Mc²/ℏ (operations per second)

For mass confined to Planck length (creates Planck-mass black hole):

Maximum rate ≈ c⁵/ℏG = 1/tP ≈ 1.855 × 10⁴⁴ operations/second

Meaning: Planck time sets the absolute speed limit for any computational process—no computer, even in principle, can perform operations faster than ~10⁴⁴ per second per Planck mass of material.

Ultimate laptop: A 1 kg laptop operating at this maximum rate would:

• Perform 10⁵² operations/second (far beyond any current computer)
• Require energies approaching Planck scale (would become a black hole!)
• Theoretical limit only—physically impossible to approach

5. Dimensional Analysis and Natural Units

Fundamental equations simplify in Planck units (c = ℏ = G = 1):

Einstein's field equations:

Standard form: Gμν = (8πG/c⁴) Tμν

Planck units (G = c = 1): Gμν = 8π Tμν

Much simpler! Planck units reveal fundamental relationships without clutter of conversion factors.

Schwarzschild radius:

Standard: rs = 2GM/c² Planck units: rs = 2M (where M is in Planck masses)

Hawking temperature:

Standard: T = ℏc³/(8πGMkB) Planck units (also kB = 1): T = 1/(8πM)

Theoretical physics calculations: High-energy physicists and cosmologists often work in natural units where ℏ = c = 1, making Planck time the fundamental timescale. Results are later converted back to SI units for comparison with experiment.

6. Philosophy of Time

Is time fundamental or emergent?

Planck time raises profound questions about the nature of time itself:

Discrete time hypothesis:

• Some quantum gravity theories (loop quantum gravity, causal sets) suggest time consists of discrete "ticks" of duration ~Planck time
• Below Planck time, "time" doesn't exist—it's like asking what's north of the North Pole
• Continuous time is an illusion, valid only at scales >> Planck time

Emergent time hypothesis:

• Time may not be fundamental at all—could emerge from timeless quantum entanglement (Wheeler-DeWitt equation suggests timeless universe)
• Planck time marks the scale where the emergent approximation breaks down
• At Planck scale, "before" and "after" may be meaningless concepts

Block universe and eternalism:

• If spacetime is a 4D block (past, present, future all equally real), Planck time sets the "grain size" of this block
• Events separated by less than Planck time may not have well-defined temporal ordering

Implications for free will, causality: If time is discrete at Planck scale, does strict determinism hold? Or do quantum fluctuations at Planck time introduce fundamental randomness into time evolution?

These remain open philosophical and scientific questions.

7. Speculative Physics and Limits of Knowledge

Can we ever test Planck-scale physics?

Direct particle collider:

• Energy required: Planck energy ≈ 10⁹ J (≈ energy of lightning bolt, concentrated in one particle!)
• LHC (most powerful collider, 2024): 10⁴ TeV = 1.6 × 10⁻⁶ J per collision
• Shortfall: Need 10¹⁵ times more energy
• Size: Planck-energy collider would need radius ~10¹³ light-years (larger than observable universe!)

Indirect observations:

Quantum gravity phenomenology:

• Search for deviations from standard physics caused by Planck-scale effects
• Example: Lorentz invariance violation—different photon colors travel at slightly different speeds due to quantum foam
• Current limits: No violations detected, but experiments improving

Gravitational waves:

• LIGO/Virgo detect spacetime ripples from black hole mergers
• Future detectors might detect quantum fluctuations of spacetime at Planck scale
• Challenge: Effects are stupendously small

Cosmic microwave background:

• CMB fluctuations may preserve imprint of Planck-epoch quantum fluctuations
• Planck satellite (2013-2018) measured CMB with unprecedented precision
• Indirect window into physics near Planck time, but not direct observation

Conclusion: We will likely never directly probe Planck time experimentally. Understanding Planck-scale physics requires theoretical breakthroughs (complete quantum gravity theory), not bigger experiments.