Second to Day Converter

Convert seconds to days with our free online time converter.

Quick Answer

1 Second = 0.0000116 days

Formula: Second × conversion factor = Day

Use the calculator below for instant, accurate conversions.

Our Accuracy Guarantee

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

Second to Day Calculator

How to Use the Second to Day Calculator:

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

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

Formula:

1 Second = 1.1574e-5 days

Example Calculation:

Convert 60 seconds: 60 × 1.1574e-5 = 0.000694444 days

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 Second and a Day?

What Is a Second?

The second (symbol: s) is the SI base unit of time, defined with extraordinary precision using atomic physics rather than astronomical observations.

Official SI definition (since 1967): The second is the duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the caesium-133 atom at absolute zero temperature and at rest.

In simpler terms:

  • Caesium-133 atoms oscillate at a precise frequency when energized
  • One second equals exactly 9,192,631,770 of these oscillations
  • This provides a natural, unchanging standard independent of Earth's rotation

Why this matters: This atomic definition provides accuracy to better than 1 second in 100 million years for modern atomic clocks, enabling:

  • GPS navigation (accuracy requires nanosecond precision)
  • Global telecommunications synchronization
  • Scientific experiments requiring extreme precision
  • Financial transaction timestamps
  • Internet infrastructure coordination

Second vs. Other Time Units

Subdivisions of the second:

  • 1 decisecond (ds) = 0.1 s = 10⁻¹ s (rarely used)
  • 1 centisecond (cs) = 0.01 s = 10⁻² s (stopwatch hundredths)
  • 1 millisecond (ms) = 0.001 s = 10⁻³ s (computer operations)
  • 1 microsecond (μs) = 0.000001 s = 10⁻⁶ s (electronics, photography)
  • 1 nanosecond (ns) = 0.000000001 s = 10⁻⁹ s (computer processors, GPS)
  • 1 picosecond (ps) = 10⁻¹² s (laser physics, molecular vibrations)
  • 1 femtosecond (fs) = 10⁻¹⁵ s (ultrafast lasers, chemical reactions)

Multiples of the second:

  • 60 seconds = 1 minute
  • 3,600 seconds = 1 hour
  • 86,400 seconds = 1 day
  • 604,800 seconds = 1 week
  • 31,536,000 seconds = 1 year (365 days)
  • 31,557,600 seconds = 1 Julian year (365.25 days)

The day (symbol: d) is a unit of time equal to 24 hours, 1,440 minutes, or 86,400 seconds.

Official civil definition: Since 1967, one day is defined as exactly 86,400 SI seconds, where each second equals 9,192,631,770 periods of caesium-133 radiation. Therefore:

  • 1 day = 86,400 × 9,192,631,770 = 793,927,920,332,800,000 caesium-133 oscillations
  • This equals approximately 794 quadrillion atomic oscillations

Astronomical definitions:

  1. Solar day (apparent solar day):

    • Time between two successive transits of the Sun across the local meridian (noon to noon)
    • Varies throughout year: ±16 minutes due to Earth's elliptical orbit and axial tilt
    • Mean solar day: Average of all solar days = 24 hours exactly (86,400 seconds)
    • This is the basis for civil timekeeping
  2. Sidereal day:

    • Time for Earth to rotate 360° relative to distant stars
    • 23 hours, 56 minutes, 4.09 seconds (86,164.09 seconds)
    • ~4 minutes shorter than solar day
    • Used in astronomy for telescope tracking and star charts
  3. Synodic day (planetary science):

    • Time for same position of sun in sky on other planets
    • Mars sol: 24 hours, 39 minutes, 35 seconds
    • Venus day: 116.75 Earth days (very slow rotation)

Why the difference?

  • Earth rotates 360° in one sidereal day
  • But Earth also orbits the Sun (~1° per day along orbit)
  • Must rotate an additional ~1° (4 minutes) for sun to return to same position
  • Result: Solar day = sidereal day + ~4 minutes
  • Over one year: 365 solar days, but 366 sidereal days (one extra rotation)

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

History of the Second and Day

Ancient Origins: Babylonian Mathematics (3000 BCE)

The division of time into units of 60 has roots in ancient Babylonian sexagesimal (base-60) mathematics:

Why base-60?

  • Highly divisible: 60 has divisors 1, 2, 3, 4, 5, 6, 10, 12, 15, 20, 30, 60
  • Finger counting: Babylonians counted 12 finger segments (phalanges) on one hand using the thumb, repeated 5 times for the other hand (12 × 5 = 60)
  • Astronomical convenience: 360 days approximated the year (6 × 60), aligning with the 360-degree circle

Time divisions established:

  • 1 day = 24 hours (2 × 12)
  • 1 hour = 60 minutes
  • 1 minute = 60 seconds

This system spread through ancient Egypt, Greece, and Rome, persisting for over 4,000 years.

Medieval Development: Mechanical Clocks (1200s-1600s)

The word "second" derives from Medieval Latin "pars minuta secunda" meaning "second minute part" (the second division of the hour):

  • First division: Hour divided into 60 "pars minuta prima" (first minute parts) = minutes
  • Second division: Minute divided into 60 "pars minuta secunda" (second minute parts) = seconds

Early mechanical clocks (1200s-1300s):

  • Displayed only hours, no minute or second hands
  • Too imprecise to measure seconds accurately
  • Driven by falling weights and escapement mechanisms

Pendulum revolution (1656):

  • Christiaan Huygens invented the pendulum clock
  • First clocks accurate enough to measure seconds reliably
  • Pendulum period provided regular "tick" for second counting
  • Accuracy improved from 15 minutes/day to 15 seconds/day

Marine chronometers (1700s):

  • John Harrison developed precise clocks for navigation (1730s-1760s)
  • Accurate timekeeping enabled longitude determination at sea
  • Precision to within 1 second per day

Astronomical Definition: Mean Solar Second (1832-1967)

In 1832, the second was formally defined as 1/86,400 of a mean solar day:

  • Mean solar day: Average length of a solar day over a year (accounts for Earth's elliptical orbit)
  • 86,400 seconds: 24 hours × 60 minutes × 60 seconds

Problems with astronomical definition:

  1. Earth's rotation is irregular: Tidal friction gradually slows rotation (~2 milliseconds per century)
  2. Seasonal variations: Earth's orbit affects day length by milliseconds
  3. Unpredictable fluctuations: Earthquakes, atmospheric changes affect rotation
  4. Increasing demand for precision: Radio, telecommunications, science required better accuracy

By the 1950s, astronomical observations showed the "second" was not constant—the length varied by parts per million depending on the era.

Atomic Revolution: Caesium Standard (1955-1967)

1955 - First caesium atomic clock:

  • Louis Essen and Jack Parry at UK's National Physical Laboratory built the first caesium atomic clock
  • Demonstrated caesium-133 atoms oscillate at precisely 9,192,631,770 Hz
  • Accuracy: 1 second in 300 years (far exceeding astronomical clocks)

1967 - Official redefinition: The 13th General Conference on Weights and Measures (CGPM) redefined the second:

"The second is the duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the caesium-133 atom."

Why caesium-133?

  • Atomic property: Transition frequency is a fundamental constant of nature
  • Highly stable: Unaffected by temperature, pressure, or electromagnetic fields
  • Reproducible: Any caesium-133 atom behaves identically
  • Practical: Relatively easy to construct atomic clocks using caesium

Impact:

  • Timekeeping became independent of Earth's rotation
  • Precision improved from parts per million to parts per trillion
  • Enabled GPS, internet synchronization, telecommunications, and modern science

Modern Atomic Clocks (1990s-Present)

Caesium fountain clocks (1990s):

  • Atoms launched upward in "fountain" configuration
  • Gravity slows atoms, allowing longer measurement time
  • Accuracy: 1 second in 100 million years

Optical lattice clocks (2000s-2020s):

  • Use strontium or ytterbium atoms instead of caesium
  • Operate at optical frequencies (100,000× higher than caesium)
  • Accuracy: 1 second in 15 billion years (age of the universe!)
  • May redefine the second in future decades

Applications requiring atomic precision:

  • GPS satellites: Nanosecond errors cause position errors of ~1 foot
  • High-frequency trading: Microsecond timestamps for financial transactions
  • Telecommunications: Synchronizing cell towers and internet infrastructure
  • Science: Detecting gravitational waves, testing relativity, fundamental physics

Leap Seconds: Reconciling Atomic and Astronomical Time

The problem:

  • Atomic time (TAI): Runs at constant rate based on caesium clocks
  • Earth rotation (UT1): Slows gradually due to tidal friction
  • Difference: ~2 milliseconds per day (accumulates ~1 second every 18 months)

Solution: Leap seconds (since 1972):

  • Coordinated Universal Time (UTC) = atomic time adjusted to stay within 0.9 seconds of Earth rotation
  • Leap second: Extra second added (or removed) on June 30 or December 31
  • 27 leap seconds added between 1972-2016 (none since 2016)

Controversy:

  • Leap seconds cause problems for computer systems, GPS, networks
  • Debate ongoing about abolishing leap seconds in favor of pure atomic time
  • Possible change may occur in the 2030s

of the Day

Prehistoric Recognition (Before 3000 BCE)

The day-night cycle is the most fundamental observable pattern in nature, recognized by all human cultures and even animals:

Biological origins:

  • Circadian rhythms: Internal ~24-hour biological clock evolved in response to Earth's rotation
  • Found in bacteria, plants, animals, humans
  • Regulated by light/dark cycle
  • Predates human civilization by billions of years

Early human observation:

  • Stone Age: Organized activities by sun position (hunting at dawn, gathering by day)
  • Neolithic era: Agricultural cycles tied to day length (planting, harvesting)
  • Megalithic monuments: Stonehenge (c. 3000 BCE) aligned with solstice sunrise
  • Earliest "clocks": Shadows cast by objects (proto-sundials)

Ancient Egyptian Timekeeping (c. 3000 BCE)

Egyptians formalized day measurement:

  1. Shadow clocks and sundials (c. 1500 BCE):

    • Obelisks cast shadows indicating time of day
    • Divided daylight into 12 parts (seasonal hours)
    • Used horizontal bars with markings
  2. Water clocks (clepsydrae):

    • Used at night when sundials didn't work
    • Water dripped at constant rate through calibrated container
    • Divided night into 12 parts
  3. Decans (star clocks):

    • 36 groups of stars rising throughout year
    • Each decan rose ~40 minutes apart
    • Used to tell time at night

Egyptian day structure:

  • Day began at sunrise (variable time)
  • 12 hours daylight + 12 hours darkness = 24 hours
  • But "hours" varied by season (longer daytime hours in summer)

Babylonian Contributions (c. 2000 BCE)

Babylonians established key concepts:

  1. Seven-day week:

    • Based on seven visible celestial bodies (Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn)
    • Each day named after a planet/god
    • This system spread globally
  2. Day began at sunset:

    • Still used in Hebrew and Islamic calendars
    • Genesis 1:5: "And there was evening, and there was morning—the first day"
  3. Base-60 mathematics:

    • Eventually led to 24 hours, 60 minutes, 60 seconds
    • 360° circle (from ~360 days in year)

Greek and Roman Systems (500 BCE - 400 CE)

Greek astronomers:

  • Hipparchus (c. 150 BCE): Studied equation of time (variation in solar day length)
  • Recognized need for "mean solar day" as average

Roman timekeeping:

  • Day began at midnight (adopted by modern civil timekeeping)
  • Divided into:
    • Dies (daytime): Sunrise to sunset, 12 horae (hours)
    • Nox (nighttime): Sunset to sunrise, 4 vigiliae (watches) of ~3 hours each
  • Market day cycle: Nundinae (8-day week, superseded by 7-day week)

Roman calendar influence:

  • Julian Calendar (45 BCE): 365.25-day year, leap years
  • Day names from planets (still used): Sunday (Sun), Monday (Moon), Saturday (Saturn)

Medieval and Islamic Developments (600-1300 CE)

Islamic timekeeping:

  • Day begins at sunset (following Hebrew tradition)
  • Five daily prayers (salat) structured the day:
    • Fajr (dawn), Dhuhr (noon), Asr (afternoon), Maghrib (sunset), Isha (night)
  • Sophisticated astronomical tables calculated prayer times
  • "Islamic day" vs. "civil day" distinction in Muslim countries

Medieval Christian hours:

  • Canonical hours: Structured monastic life
    • Matins (midnight), Lauds (dawn), Prime (6 AM), Terce (9 AM)
    • Sext (noon), None (3 PM), Vespers (sunset), Compline (bedtime)
  • Church bells marked these hours, organizing community life

Mechanical Clocks and Equal Hours (1300s)

Transformation of daily time:

Before mechanical clocks:

  • "Hours" varied by season
  • Time was task-oriented ("work until sunset")
  • Imprecise coordination

After mechanical clocks (1300s-1400s):

  • 24 equal hours became standard
  • Clocks tick at constant rate regardless of season
  • "Clock time" replaced "sun time" for daily schedules
  • Enabled precise coordination of activities

Social impact:

  • Time discipline: Workers expected at specific times
  • Urban life required synchronization
  • "Punctuality" became a virtue
  • Transition from natural rhythms to mechanical rhythms

Scientific Definition (1800s)

Astronomical measurement:

  • 1832: Second officially defined as 1/86,400 of mean solar day
  • Astronomers recognized Earth's rotation not perfectly uniform
  • Tidal friction slowly increases day length (~1.7 milliseconds per century)

Problem discovered:

  • Earth's rotation varies:
    • Seasonal variations (atmosphere, ice melt)
    • Long-term slowing (tidal friction from Moon)
    • Irregular variations (core-mantle coupling, earthquakes)
  • "Day" based on Earth rotation became unreliable time standard

Atomic Era: Day Decoupled from Rotation (1967)

Atomic second (1967):

  • Second redefined based on caesium-133 atomic transitions
  • Day remains 86,400 seconds (by definition)
  • But now independent of Earth's actual rotation period

Consequence: Leap seconds

  • Earth's rotation gradually slowing
  • Atomic time (TAI) and Earth rotation time (UT1) drift apart
  • Leap seconds added to keep them synchronized:
    • 27 leap seconds added between 1972-2016
    • Last one: December 31, 2016 (23:59:60)
    • Makes that day 86,401 seconds long
  • Controversy: May abolish leap seconds in favor of "leap hours" every few centuries

Current system:

  • UTC (Coordinated Universal Time): Atomic time with leap seconds
  • Keeps within 0.9 seconds of Earth rotation (UT1)
  • Used for civil timekeeping worldwide

Calendar Evolution

Ancient calendars:

  • Lunar calendars: Based on moon phases (~29.5 days per month)
  • Solar calendars: Based on seasonal year (365.25 days)
  • Lunisolar calendars: Combine both (Hebrew, Chinese)

Gregorian Calendar (1582):

  • Reformed Julian calendar
  • Year = 365.2425 days (very close to true solar year: 365.2422 days)
  • Leap year rules:
    • Divisible by 4: Leap year (1600, 2000, 2004, 2024)
    • Divisible by 100: Not leap year (1700, 1800, 1900)
    • Divisible by 400: Leap year anyway (1600, 2000, 2400)
  • Now used in nearly all countries for civil purposes

Common Uses and Applications: seconds vs days

Explore the typical applications for both Second (imperial/US) and Day (imperial/US) to understand their common contexts.

Common Uses for seconds

The second is the universal foundation for all time measurement in modern civilization:

1. Timekeeping and Clocks

Everyday timekeeping:

  • Wristwatches and clocks display hours, minutes, seconds
  • Smartphones synchronize to atomic time via network
  • Wall clocks, alarm clocks, digital displays
  • Public time displays (train stations, airports, town squares)

Precision timekeeping:

  • Atomic clocks: Caesium, rubidium, hydrogen maser clocks
  • GPS satellites: Carry atomic clocks for navigation
  • Scientific facilities: National metrology institutes maintain primary time standards
  • Network Time Protocol (NTP): Synchronizes computer clocks to microsecond accuracy

2. Scientific Research and Experiments

Physics experiments:

  • Measuring particle lifetimes (nanoseconds to picoseconds)
  • Timing light pulses in lasers (femtoseconds)
  • Gravitational wave detection (millisecond timing precision)
  • Quantum mechanics experiments (Planck time: 10⁻⁴⁴ seconds)

Chemistry:

  • Reaction kinetics and rates
  • Spectroscopy (measuring light absorption/emission frequencies)
  • Femtochemistry (bond breaking/forming at femtosecond scale)

Biology:

  • Neural signal timing (milliseconds)
  • Cellular processes (seconds to hours)
  • Ecological cycles (days, seasons, years measured in seconds)

3. Computing and Digital Systems

Processor operations:

  • CPU clock speeds measured in GHz (billions of cycles/second)
  • Instruction execution times (nanoseconds)
  • Cache latency, memory access times

Software and programming:

  • Timestamps (Unix time: seconds since January 1, 1970)
  • Timeouts and delays
  • Animation frame rates (60 frames/second = 0.0167 s/frame)
  • Video frame rates (24, 30, 60 FPS)

Database and logging:

  • Transaction timestamps (millisecond or microsecond precision)
  • System logs with second-level granularity
  • Performance monitoring (operations/second)

4. Telecommunications and Networking

Network synchronization:

  • Cell towers synchronized to GPS time (nanosecond precision)
  • Internet infrastructure timing
  • 5G networks require nanosecond coordination
  • Precision Time Protocol (PTP) for industrial networks

Data transmission:

  • Bit rates measured in bits/second (Mbps, Gbps)
  • Latency measured in milliseconds
  • Packet timing and queuing

5. Navigation and GPS

Global Positioning System:

  • Atomic clocks on satellites (accuracy ~10 nanoseconds)
  • Signal travel time calculations
  • Position accuracy requires nanosecond precision
  • GNSS systems (GPS, GLONASS, Galileo, BeiDou)

Aviation:

  • Aircraft navigation timing
  • Air traffic control coordination
  • Flight duration measurements

6. Financial and Trading

High-frequency trading:

  • Microsecond timestamps on transactions
  • Trading algorithms execute in microseconds
  • Market data feeds timestamped to nanoseconds
  • Regulatory requirements for precise time-stamping

Banking:

  • Transaction timestamps
  • Interest calculations (per second for some instruments)
  • Automated trading systems

7. Sports and Athletics

Competition timing:

  • Track and field (0.01 second precision)
  • Swimming (0.01 second precision)
  • Skiing, bobsled (0.01 second precision)
  • Motor racing (0.001 second precision)

Training and performance:

  • Stopwatches for interval training
  • Heart rate monitors (beats/second)
  • Pace calculations (minutes per kilometer/mile)
  • Reaction time testing

8. Manufacturing and Industrial

Process control:

  • Machine cycle times (seconds)
  • Assembly line timing
  • Quality control measurements
  • Synchronization of robots and automation

Industrial timing:

  • Conveyor belt speeds
  • Injection molding cycle times (2-60 seconds typical)
  • 3D printing layer times
  • Chemical process durations

When to Use days

and Applications

1. Age and Lifespan Measurement

Human life measured in days:

  • Age calculation:

    • Newborn: Age in days (first month)
    • Infant: Days and weeks (first 12 months)
    • Adult: Years (365.25 days per year)
  • Life expectancy:

    • Global average: ~73 years = 26,645 days
    • US average: ~78 years = 28,470 days
    • Japan (highest): ~84 years = 30,660 days
  • Milestones:

    • 100 days: Traditional celebration in some cultures
    • 1,000 days: ~2.7 years (toddler milestone)
    • 10,000 days: ~27.4 years (young adult)
    • 20,000 days: ~54.8 years (mid-life)
    • 30,000 days: ~82.2 years (if reached, long life)
  • Historical figures:

    • "Lived 90 years" = 32,850 days
    • Queen Elizabeth II: 35,065 days (96 years, 140 days)
    • Oldest verified person: Jeanne Calment, 44,724 days (122 years, 164 days)

2. Project Management and Planning

Projects measured in days:

  • Timeline terminology:

    • "Day 0": Project start
    • "Elapsed days": Total calendar days
    • "Working days": Excluding weekends/holidays
    • "Man-days": One person working one day
  • Estimation:

    • "3-day task"
    • "2-week project" = 10 working days
    • "6-month project" = ~130 working days
  • Milestones:

    • "Deliverable due Day 30"
    • "Phase 1 complete Day 45"
    • "Final deadline Day 90"
  • Agile/Scrum:

    • Sprint: 14 days (2 weeks) typical
    • Daily standup: Every day, 15 minutes
    • Sprint review: End of 14-day sprint

3. Astronomy and Planetary Science

Planetary rotation periods measured in days:

  • Planetary "days" (rotation period):

    • Mercury: 58.6 Earth days
    • Venus: 243 Earth days (slower than its year!)
    • Earth: 1 day (23 hours 56 min sidereal)
    • Mars: 1.03 days (24 hours 37 min) - called a "sol"
    • Jupiter: 0.41 days (9 hours 56 min)
    • Saturn: 0.45 days (10 hours 33 min)
    • Uranus: 0.72 days (17 hours 14 min)
    • Neptune: 0.67 days (16 hours 6 min)
  • Orbital periods (years in days):

    • Mercury year: 88 Earth days
    • Venus year: 225 Earth days
    • Mars year: 687 Earth days
    • Earth year: 365.25 days
  • Mars missions:

    • Use "sols" (Mars days) for mission planning
    • Sol 1, Sol 2, Sol 3... (rovers like Curiosity, Perseverance)
    • Communication delay: 3-22 minutes (depends on planets' positions)
  • Astronomical events:

    • Lunar month: 29.53 days (new moon to new moon)
    • Eclipse cycles: Saros cycle = 6,585.3 days (18 years, 11 days)

4. Weather and Climate

Weather patterns measured in days:

  • Forecasting:

    • 1-day forecast: Very accurate (~90%)
    • 3-day forecast: Accurate (~80%)
    • 7-day forecast: Moderately accurate (~65%)
    • 10+ day forecast: Less reliable
  • Weather phenomena:

    • Heat wave: 3+ consecutive days above threshold
    • Cold snap: 2+ days below freezing
    • Drought: 15+ days without significant rain
  • Seasonal patterns:

    • Growing season: Number of frost-free days (150-200+ days)
    • Rainy season: 90-180 days (tropics)
    • Winter: Shortest day (winter solstice) vs. longest night
  • Degree days:

    • Heating degree days (HDD): Measure of cold
    • Cooling degree days (CDD): Measure of heat
    • Base 65°F: Sum of daily degrees below/above
  • Climate records:

    • "Hottest day on record"
    • "100 days above 90°F" (Phoenix averages 110+ days)
    • "Consecutive days of rain" (record: 331 days, Kauai)

5. Finance and Business

Financial operations measured in days:

  • Payment terms:

    • Net 30: Payment due 30 days after invoice
    • Net 60: Payment due 60 days after invoice
    • 2/10 Net 30: 2% discount if paid within 10 days, otherwise due in 30
  • Interest calculation:

    • Daily interest: Annual rate ÷ 365 days
    • Grace period: 21-25 days (credit cards)
    • Late fees: Applied after due date + grace period
  • Financial metrics:

    • Days sales outstanding (DSO): Average days to collect payment
    • Days payable outstanding (DPO): Average days to pay suppliers
    • Days inventory outstanding (DIO): Average days inventory held
  • Trading:

    • "Trading day": Stock market open day (weekdays, excluding holidays)
    • NYSE: ~252 trading days per year
    • Settlement: T+2 (trade day + 2 business days)
  • Bonds:

    • Accrued interest calculated by day
    • 30/360 day count convention (assumes 30-day months)
    • Actual/365: Uses actual calendar days

6. Data Storage and Computing

Digital retention measured in days:

  • Backups:

    • Daily backups: 7 days retained (1 week)
    • Weekly backups: 30 days retained (1 month)
    • Monthly backups: 365 days retained (1 year)
  • Logs:

    • Server logs: 30-90 days retention typical
    • Security logs: 90-365 days (compliance requirements)
    • Application logs: 14-30 days
  • Caching:

    • Browser cache: 30 days default
    • CDN cache: 1-30 days depending on content
    • DNS cache: 1 day (86,400 seconds TTL common)
  • Data retention policies:

    • GDPR: 30 days to fulfill deletion request
    • Email: Auto-delete after 90 days (some organizations)
    • Trash/recycle bin: 30 days before permanent deletion

7. Habits and Personal Development

Habit formation measured in days:

  • Popular beliefs:

    • "21 days to form a habit" (myth - actually varies widely)
    • "30-day challenge" (fitness, meditation, etc.)
    • "90-day transformation programs"
  • Research findings:

    • Average habit formation: 66 days (range: 18-254 days)
    • Simple habits: 18-30 days
    • Complex habits: 200+ days
  • Streaks:

    • "100-day streak" on language apps (Duolingo)
    • "30-day yoga challenge"
    • "365-day photo project" (one photo per day for a year)
  • Reading goals:

    • "Read every day for 30 days"
    • "One book per week" = finish in 7 days
    • "365 books in a year" = 1 per day

Additional Unit Information

About Second (s)

What is the base unit of time in the SI system?

The second (s) is the base unit of time in the International System of Units (SI). It's one of the seven SI base units, alongside meter (length), kilogram (mass), ampere (current), kelvin (temperature), mole (amount of substance), and candela (luminous intensity).

All other time units (minute, hour, day, year) are derived from the second.

Why is the second defined using atoms?

The atomic definition provides a much more stable and precise standard than relying on Earth's rotation, which fluctuates.

Problems with astronomical definition:

  • Earth's rotation slows by ~2 milliseconds per century (tidal friction)
  • Seasonal variations affect day length
  • Unpredictable fluctuations from earthquakes, atmospheric changes
  • Accuracy limited to ~1 part per million

Advantages of atomic definition:

  • Fundamental constant: Caesium-133 transition frequency is a property of nature
  • Reproducible: Any caesium-133 atom behaves identically
  • Stable: Unaffected by external conditions (temperature, pressure)
  • Precise: Modern atomic clocks accurate to 1 second in 100 million years

Result: GPS, telecommunications, science, and technology require nanosecond precision impossible with astronomical timekeeping.

How many seconds are in a minute?

There are exactly 60 seconds in 1 minute.

This derives from ancient Babylonian base-60 (sexagesimal) mathematics, which established 60 as the standard division for time over 4,000 years ago.

Conversions:

  • 1 minute = 60 seconds
  • 2 minutes = 120 seconds
  • 5 minutes = 300 seconds
  • 10 minutes = 600 seconds

How many seconds are in an hour?

There are exactly 3,600 seconds in 1 hour.

Calculation:

  • 1 hour = 60 minutes
  • 1 minute = 60 seconds
  • 1 hour = 60 × 60 = 3,600 seconds

Conversions:

  • 1 hour = 3,600 seconds
  • 2 hours = 7,200 seconds
  • 12 hours = 43,200 seconds
  • 24 hours (1 day) = 86,400 seconds

How many seconds are in a day?

There are 86,400 seconds in 1 day (24 hours).

Calculation:

  • 1 day = 24 hours
  • 1 hour = 3,600 seconds
  • 1 day = 24 × 3,600 = 86,400 seconds

Breakdown:

  • 24 hours × 60 minutes/hour × 60 seconds/minute = 86,400 seconds

Note: This assumes a standard 24-hour day. Due to Earth's rotation irregularities, actual solar days vary by milliseconds. Leap seconds are occasionally added to keep atomic time synchronized with Earth rotation.

How many seconds are in a year?

A standard 365-day year contains 31,536,000 seconds.

Calculation:

  • 365 days × 24 hours/day × 60 minutes/hour × 60 seconds/minute
  • = 365 × 86,400
  • = 31,536,000 seconds

Variations:

  • Leap year (366 days): 31,622,400 seconds
  • Julian year (365.25 days, average): 31,557,600 seconds
  • Tropical year (365.2422 days, Earth orbit): 31,556,925 seconds

Fun fact: The song "Seasons of Love" from Rent states "525,600 minutes" in a year, which equals 31,536,000 seconds (365 days).

What is a millisecond?

A millisecond (ms) is one-thousandth of a second: 0.001 seconds or 10⁻³ seconds.

Conversions:

  • 1 second = 1,000 milliseconds
  • 1 millisecond = 0.001 seconds
  • 1 minute = 60,000 milliseconds

Common uses:

  • Computer response times (1-100 ms)
  • Network ping times (1-300 ms typical)
  • Human reaction time (~200 ms)
  • Video frame duration (60 FPS = 16.67 ms/frame)
  • Stopwatch hundredths (0.01 s = 10 ms)

What is a nanosecond?

A nanosecond (ns) is one-billionth of a second: 0.000000001 seconds or 10⁻⁹ seconds.

Conversions:

  • 1 second = 1,000,000,000 nanoseconds (1 billion)
  • 1 millisecond = 1,000,000 nanoseconds (1 million)
  • 1 microsecond = 1,000 nanoseconds

Reference points:

  • Light travels 30 cm (1 foot) in 1 nanosecond
  • Computer processor operations: ~0.2-1 nanosecond
  • GPS timing precision: ~10 nanoseconds
  • RAM memory access: ~50-100 nanoseconds

Grace Hopper's demonstration: Computer pioneer Grace Hopper famously distributed 30cm lengths of wire to represent "one nanosecond" (distance light travels in 1 ns) to illustrate the importance of speed in computing.

Why are there 60 seconds in a minute instead of 100?

The 60-second minute derives from ancient Babylonian base-60 (sexagesimal) mathematics developed around 3000 BCE, over 1,000 years before the decimal system.

Reasons for base-60:

1. High divisibility: 60 has 12 divisors: 1, 2, 3, 4, 5, 6, 10, 12, 15, 20, 30, 60

  • Easy to divide into halves, thirds, quarters, fifths, sixths
  • 100 (decimal) has only 9 divisors: 1, 2, 4, 5, 10, 20, 25, 50, 100

2. Finger counting method:

  • Count 12 finger segments (phalanges) on one hand using thumb
  • Track count on other hand: 12 × 5 fingers = 60

3. Astronomical convenience:

  • ~360 days per year ≈ 6 × 60
  • Circle divided into 360 degrees (6 × 60)
  • Babylonian astronomy used these divisions

4. Historical persistence: The system spread through Egyptian, Greek, and Roman civilizations and became too entrenched to change. When mechanical clocks developed in medieval Europe, they adopted the existing Babylonian time divisions.

Attempts to decimalize time:

  • French Revolutionary Calendar (1793-1805): 10-hour day, 100-minute hour, 100-second minute
  • Failed: Too difficult to change clocks, conversion from traditional system
  • Result: We still use Babylonian base-60 for time, but base-10 (decimal) for most other measurements

How accurate are atomic clocks?

Modern atomic clocks are extraordinarily accurate:

Caesium atomic clocks (standard):

  • Accuracy: 1 second in 100 million years
  • Precision: Parts per trillion (10⁻¹²)
  • Used in GPS satellites, national time standards

Caesium fountain clocks (advanced):

  • Accuracy: 1 second in 300 million years
  • Precision: Better than 10⁻¹⁵
  • Used by metrology institutes (NIST, PTB, NPL)

Optical lattice clocks (state-of-the-art):

  • Accuracy: 1 second in 15-30 billion years
  • Precision: 10⁻¹⁸ to 10⁻¹⁹
  • Use strontium, ytterbium, or aluminum ions
  • So precise they detect gravitational time dilation across centimeters of height

Comparison:

  • Quartz watch: 1 second in 1-10 days (10⁻⁵ accuracy)
  • Mechanical watch: 1-10 seconds per day (10⁻⁴ to 10⁻⁵)
  • Sundial: Minutes per day (10⁻³)
  • Atomic clock: 1 second in 100 million years (10⁻¹⁶)

Why this matters: GPS requires 10-nanosecond precision; a 1-microsecond error causes 300-meter position errors.

What are leap seconds and why do we need them?

Leap seconds are occasional one-second adjustments added to Coordinated Universal Time (UTC) to keep it synchronized with Earth's rotation.

The problem:

  • Atomic time (TAI): Runs at constant rate based on caesium clocks, unchanging
  • Earth rotation (UT1): Slows gradually due to tidal friction (~2 milliseconds per day longer)
  • Discrepancy: Accumulates ~1 second every 18-24 months

Solution:

  • Add (or theoretically remove) 1 second on June 30 or December 31
  • Keeps UTC within 0.9 seconds of Earth rotation time (UT1)
  • 27 leap seconds added between 1972 and 2016
  • No leap seconds since 2016 (Earth rotation has been slightly faster recently)

How it works: Instead of 23:59:59 → 00:00:00, the sequence is: 23:59:59 → 23:59:60 → 00:00:00 (leap second inserted)

Controversy:

  • Problems: Computer systems, GPS, networks struggle with leap seconds (software bugs, crashes)
  • Proposed solution: Abolish leap seconds, let UTC and UT1 drift apart
  • Debate: Ongoing since 2000s; decision may be made in 2026-2030s

Current status: Leap seconds remain in use, but their future is uncertain.


About Day (d)

How many hours are in a day?

Exactly 24 hours in a standard civil day.

This is a defined constant: 1 day = 24 hours = 1,440 minutes = 86,400 seconds.

Exception: Daylight Saving Time transitions create days with 23 hours (spring forward) or 25 hours (fall back) in regions that observe DST.

How many seconds are in a day?

Exactly 86,400 seconds in a standard day.

Calculation: 24 hours × 60 minutes × 60 seconds = 86,400 seconds

Since 1967, this equals 793,927,920,332,800,000 caesium-133 oscillations (~794 quadrillion).

Exception: Days with leap seconds have 86,401 seconds (last occurred December 31, 2016).

Is every day exactly 24 hours long?

For civil timekeeping: Yes. The day is defined as exactly 24 hours (86,400 seconds).

For Earth's rotation: No. Earth's actual rotation period varies:

  • Gradually slowing (~1.7 milliseconds per century) due to tidal friction from Moon
  • Seasonal variations (±1 millisecond) from atmospheric/oceanic changes
  • Irregular variations from earthquakes, ice melt, core-mantle coupling

Solution: Leap seconds occasionally added to keep clock time synchronized with Earth's rotation (within 0.9 seconds).

What's the difference between a solar day and a sidereal day?

Solar day (24 hours):

  • Time from one solar noon to the next (sun at highest point)
  • What we use for civil timekeeping
  • Accounts for Earth's orbit around sun

Sidereal day (23 hours, 56 minutes, 4 seconds):

  • Time for Earth to rotate 360° relative to distant stars
  • Used in astronomy for telescope tracking
  • ~4 minutes shorter than solar day

Why the difference? After Earth rotates 360° (one sidereal day), it has moved ~1° along its orbit. It must rotate an additional ~1° (~4 minutes) for the sun to return to the same position in the sky.

Result: 365 solar days per year, but 366 sidereal days per year (one extra rotation due to orbit).

Why does February have 28 days?

Historical reasons:

  1. Roman calendar (753 BCE):

    • Originally 10 months, 304 days (March-December)
    • Winter was monthless period
  2. Numa Pompilius reform (c. 713 BCE):

    • Added January and February
    • Romans considered even numbers unlucky
    • Made most months 29 or 31 days
    • February got leftover days: 28 (occasionally 29)
  3. Julius Caesar (45 BCE):

    • Julian calendar: 365.25-day year
    • Added day to February every 4 years (leap year)
    • February remained shortest month
  4. Pope Gregory XIII (1582):

    • Gregorian calendar reform
    • Refined leap year rules
    • February kept 28/29-day structure

Why not fix it? Changing calendar would disrupt billions of systems worldwide (contracts, software, cultural traditions).

How many days are in a year?

Common year: 365 days Leap year: 366 days

Solar/tropical year (Earth's orbit): 365.2422 days (365 days, 5 hours, 48 minutes, 46 seconds)

Leap year rules (Gregorian calendar):

  • Divisible by 4: Leap year (2024, 2028)
  • Divisible by 100: Not leap year (2100, 2200)
  • Divisible by 400: Leap year (2000, 2400)

Average Gregorian year: 365.2425 days (very close to true solar year)

Other calendar systems:

  • Islamic calendar: 354 days (lunar)
  • Hebrew calendar: 353-385 days (lunisolar, variable)
  • Julian calendar: 365.25 days (old system, now obsolete)

What is a leap second?

A leap second is an extra second added to clocks to keep atomic time synchronized with Earth's rotation.

Why needed:

  • Earth's rotation gradually slowing (tidal friction)
  • Atomic clocks run at constant rate (86,400 seconds per day)
  • Without leap seconds, clock time would drift from solar time

How it works:

  • Added at end of June 30 or December 31
  • Clock reads 23:59:59 → 23:59:60 → 00:00:00 (next day)
  • That day has 86,401 seconds instead of 86,400

History:

  • 27 leap seconds added between 1972-2016
  • Last one: December 31, 2016
  • None added since (Earth's rotation has been speeding up slightly)

Controversy:

  • Causes problems for computer systems
  • Proposed to abolish in favor of letting atomic time drift (then add "leap hour" every few centuries)

How do different cultures define when a day starts?

Different traditions begin the day at different times:

Midnight (00:00) - Modern civil time:

  • Used by most countries for official purposes
  • Inherited from Roman tradition
  • Convenient for business (avoids confusion around midday)

Sunset - Jewish and Islamic tradition:

  • Hebrew calendar: Day begins at sunset
  • Islamic calendar: Day begins at sunset
  • Biblical: "And there was evening, and there was morning—the first day"
  • Makes sense for agricultural societies

Dawn/Sunrise - Ancient Egypt, Hinduism:

  • Egyptian day began at sunrise
  • Hindu day traditionally begins at sunrise
  • Natural marker of "beginning" of daylight

Noon - Ancient Babylonians (some periods):

  • Based on sun at highest point
  • Astronomical reference

Modern inconsistency:

  • Civil day: Midnight
  • Religious calendars: Often sunset
  • Common language: "Day" often means daylight hours only

How old am I in days?

Formula: Age in days = (Years × 365.25) + extra days since last birthday

Example:

  • Born January 1, 2000
  • Today is November 26, 2024
  • Age: 24 years, 329 days
  • Days: (24 × 365.25) + 329 ≈ 9,095 days

Online calculators:

  • Many websites calculate exact age in days
  • Account for actual leap years experienced
  • Can calculate down to hours/minutes/seconds

Milestones:

  • 1,000 days: ~2.7 years old
  • 10,000 days: ~27.4 years old ("10,000-day birthday")
  • 20,000 days: ~54.8 years old
  • 30,000 days: ~82.2 years old (if reached)

Why is a week 7 days?

Ancient origins:

  1. Babylonian astronomy (c. 2000 BCE):

    • Seven visible celestial bodies: Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn
    • Each "ruled" one day
    • 7-day planetary week
  2. Biblical/Jewish tradition:

    • Genesis creation story: God created world in 6 days, rested on 7th
    • Sabbath (7th day) holy day of rest
    • Commandment: "Remember the Sabbath day"
  3. Roman adoption:

    • Romans adopted 7-day week (1st-3rd century CE)
    • Named days after planets/gods
    • Spread throughout Roman Empire
  4. Global spread:

    • Christianity spread 7-day week with Sunday as holy day
    • Islam adopted 7-day week with Friday as holy day
    • Now universal worldwide

Why not 10 days?

  • French Revolution tried 10-day week (1793-1805) - failed
  • USSR tried 5-day and 6-day weeks (1929-1940) - abandoned
  • 7-day week too culturally embedded to change

Day names (English):

  • Sunday: Sun's day
  • Monday: Moon's day
  • Tuesday: Tiw's day (Norse god)
  • Wednesday: Woden's day (Odin)
  • Thursday: Thor's day
  • Friday: Frigg's day (Norse goddess)
  • Saturday: Saturn's day

Can a day ever be longer or shorter than 24 hours?

For civil timekeeping: Usually no. A day is defined as exactly 24 hours (86,400 seconds).

Exceptions:

  1. Leap seconds:

    • Day with leap second = 86,401 seconds (0.001% longer)
    • 27 instances between 1972-2016
    • Adds one second at end of June 30 or December 31
  2. Daylight Saving Time:

    • "Spring forward" day: 23 hours (lose 1 hour)
    • "Fall back" day: 25 hours (gain 1 hour)
    • Only in regions observing DST
  3. Time zone transitions:

    • Crossing International Date Line can skip or repeat a day
    • Country changing time zones can alter day length
  4. Earth's actual rotation:

    • Varies by ±1 millisecond seasonally
    • Gradually slowing (~1.7 ms per century)
    • But civil day remains fixed at 86,400 seconds

Historical:

  • Ancient "seasonal hours" made days vary by season
  • Equal 24-hour days standardized with mechanical clocks (1300s)

Conversion Table: Second to Day

Second (s)Day (d)
0.50
10
1.50
20
50
100
250
500.001
1000.001
2500.003
5000.006
1,0000.012

People Also Ask

How do I convert Second to Day?

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What is the conversion factor from Second to Day?

The conversion factor depends on the specific relationship between Second and Day. 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 Day back to Second?

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What are common uses for Second and Day?

Second and Day are both standard units used in time measurements. They are commonly used in various applications including engineering, construction, cooking, and scientific research. Browse our time converter for more conversion options.

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

All Time Conversions

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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 Time and Frequency

National Institute of Standards and TechnologyOfficial time standards and definitions

BIPM Second Definition

Bureau International des Poids et MesuresDefinition of the SI base unit for time

Last verified: December 3, 2025