Hour to Day Converter
Convert hours to days with our free online time converter.
Quick Answer
1 Hour = 0.041667 days
Formula: Hour × 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.
Hour to Day Calculator
How to Use the Hour to Day Calculator:
- Enter the value you want to convert in the 'From' field (Hour).
- The converted value in Day will appear automatically in the 'To' field.
- Use the dropdown menus to select different units within the Time category.
- Click the swap button (⇌) to reverse the conversion direction.
How to Convert Hour to Day: Step-by-Step Guide
Converting Hour to Day involves multiplying the value by a specific conversion factor, as shown in the formula below.
Formula:
1 Hour = 0.0416667 daysExample Calculation:
Convert 60 hours: 60 × 0.0416667 = 2.5 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.
Need to convert to other time units?
View all Time conversions →What is a Hour and a Day?
The hour (symbol: h or hr) is a unit of time equal to 60 minutes, 3,600 seconds, or 1/24 of a day.
Official SI-derived definition: Since the second was redefined atomically in 1967, one hour equals exactly 3,600 seconds, where each second is 9,192,631,770 periods of caesium-133 radiation. Therefore:
- 1 hour = 3,600 × 9,192,631,770 = 33,074,688,259,200,000 caesium-133 oscillations
- This equals approximately 33.07 quadrillion atomic oscillations
Practical conversions:
- 1 hour = 60 minutes (exact)
- 1 hour = 3,600 seconds (exact)
- 1 day = 24 hours (exact)
- 1 week = 168 hours (7 × 24)
- 1 year (365 days) = 8,760 hours (365 × 24)
The hour is not an SI base unit, but it is accepted for use with the SI due to its fundamental role in civil timekeeping and global coordination.
The 24-Hour Day
The division of the day into 24 hours reflects both astronomical reality and historical convention:
Astronomical basis:
- Earth rotates 360° in ~24 hours (one solar day)
- Each hour = 15° of rotation (360° ÷ 24 = 15°)
- This is why time zones are spaced ~15° longitude apart
- Solar noon occurs when the sun crosses the meridian (highest point)
Why 24, not 20 or 10?
- Ancient Egyptians used base-12 counting (duodecimal)
- 12 is highly divisible: factors are 1, 2, 3, 4, 6, 12
- 12 daytime hours + 12 nighttime hours = 24-hour cycle
- This system was inherited by Greeks, Romans, and eventually globally standardized
Solar vs. Sidereal Hours:
- Solar hour: Based on Earth's rotation relative to the Sun (24 hours per cycle)
- Sidereal hour: Based on Earth's rotation relative to distant stars (23 hours, 56 minutes, 4 seconds per cycle)
- Civil timekeeping uses solar hours because they align with day/night cycles
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:
-
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
-
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
-
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 Hour 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 Hour and Day
of the Hour
Ancient Egyptian Origins (c. 2000 BCE)
The earliest systematic division of day and night into hours comes from ancient Egypt around 2000 BCE. Egyptian priests needed to schedule temple rituals and religious observations throughout the day and night.
Egyptian timekeeping innovations:
-
Shadow clocks (sundials): Used during daylight to track time by shadow position
- Divided daylight into 12 parts
- Earliest example: Obelisk shadow clock (c. 1500 BCE)
-
Water clocks (clepsydrae): Used at night and cloudy days
- Water dripped from container at constant rate
- Markings indicated elapsed time
- Divided nighttime into 12 parts
Crucial limitation: Seasonal hours (temporales horae)
- Summer daylight hours were longer than winter daylight hours
- Example: In Egypt, summer daytime hour ≈ 75 minutes, winter daytime hour ≈ 45 minutes
- Nighttime hours varied inversely (longer in winter, shorter in summer)
- This made sense for agricultural societies organized around daylight availability
Why 12 divisions?
- Egyptians used base-12 (duodecimal) counting, possibly because:
- 12 lunar months per year
- 12 knuckles on four fingers (excluding thumb)—convenient finger counting
- 12 is highly divisible (1, 2, 3, 4, 6, 12)
Greek and Roman Refinement (300 BCE - 400 CE)
Hellenistic astronomers (c. 300 BCE) introduced the concept of equal-length hours:
- "Equinoctial hours": Dividing the full 24-hour day-night cycle into 24 equal parts
- Each equinoctial hour = 1/24 of a mean solar day
- This was primarily used for astronomical calculations, not daily timekeeping
- Hipparchus (c. 150 BCE) used equinoctial hours for celestial observations
Roman timekeeping:
- Romans continued using seasonal hours for daily life
- Day (from sunrise to sunset) divided into 12 horae
- Night divided into 4 vigiliae (watches) of 3 hours each
- "First hour" (prima hora) = first hour after sunrise (varies by season)
- "Sixth hour" (sexta hora) = midday → origin of "siesta"
- "Eleventh hour" = last hour before sunset → modern idiom "at the eleventh hour" (last minute)
Roman water clocks (clepsydrae):
- Public water clocks in marketplaces
- Adjusted seasonally to maintain 12-hour daytime divisions
- Used for timing speeches in Senate (each senator allotted specific time)
Medieval Islamic Golden Age (700-1300 CE)
Islamic scholars made critical advances in precise timekeeping for astronomical observations and prayer time calculations:
Five daily prayers (salat):
- Fajr (dawn), Dhuhr (midday), Asr (afternoon), Maghrib (sunset), Isha (evening)
- Required accurate determination of solar positions
- Drove development of sophisticated astronomical clocks
Key innovations:
- Astronomical tables (zij): Calculated prayer times using equinoctial hours
- Astrolabes: Portable astronomical computers for time determination
- Advanced water clocks: Al-Jazari's "Castle Clock" (1206) featured complex automata
- Mathematical timekeeping: Used trigonometry to calculate hour angles
Islamic astronomers fully adopted equinoctial hours for scientific work while society continued using seasonal hours for daily activities.
Mechanical Clocks and Hour Standardization (1300-1600)
The invention of mechanical clocks in medieval Europe around 1280-1300 CE forced the adoption of equal-length hours:
Why mechanical clocks standardized hours:
- Mechanical escapement mechanisms tick at constant rates
- Cannot automatically adjust for seasonal variations
- Fixed 24-hour cycle physically built into clockwork
- This made equal-length hours the practical default
Early public clocks:
- Salisbury Cathedral Clock (England, c. 1386): Still running, one of oldest
- Wells Cathedral Clock (England, c. 1390): Features astronomical dial
- Prague Astronomical Clock (Czech Republic, 1410): Shows multiple time systems
- Church tower clocks visible/audible across towns
- Bells chimed on the hour, coordinating community activities
Impact on society:
- Transition from "task-oriented time" (work until task done) to "clock time" (work specific hours)
- Monasteries first adopted strict hour-based schedules (canonical hours)
- Urban merchants and craftsmen followed
- "Time discipline" emerged: punctuality became valued
Hour angles and navigation:
- 1 hour = 15° longitude (since Earth rotates 360° in 24 hours)
- Ships could determine longitude by comparing local solar noon to chronometer showing home port time
- This principle drove development of marine chronometers in 1700s
12-Hour vs. 24-Hour Time Notation
12-hour clock (with AM/PM):
- AM = ante meridiem (Latin: before midday)
- PM = post meridiem (Latin: after midday)
- Hours: 12:00 AM (midnight), 1 AM-11 AM, 12:00 PM (noon), 1 PM-11 PM
- Used in: United States, Canada, Australia, Philippines, parts of Latin America
- Ambiguity issue: 12:00 AM vs. 12:00 PM frequently confused
24-hour clock (military time):
- Hours numbered 00:00 (midnight) through 23:59
- Used in: Most of Europe, Asia, Africa, South America, military/aviation worldwide
- ISO 8601 international standard: HH:MM:SS format (e.g., 14:30:00)
- Eliminates AM/PM ambiguity
- Preferred for timetables, logistics, computing
Historical development:
- Ancient Egyptians and Romans used 1-12 numbering twice daily
- 24-hour notation emerged with astronomical use in Renaissance
- Military adoption (especially WWI era) standardized 24-hour format
- Computing systems use 24-hour format internally
Time Zones: Dividing Earth into Hours (1883-1884)
Before the late 1800s, each town kept its own "local solar time" based on the sun's position. This created chaos for railroad timetables—a train journey might cross dozens of different local times.
Railroad time standardization (1883):
- US/Canadian railroads established four continental time zones on November 18, 1883
- Each zone spanned roughly 15° longitude (one hour)
- Cities synchronized clocks within each zone
International Meridian Conference (1884, Washington D.C.):
- Established Greenwich, England as 0° longitude (Prime Meridian)
- Divided Earth into 24 standard time zones, each 15° wide
- Each zone offset by one hour from UTC (Coordinated Universal Time, formerly GMT)
- Created International Date Line at 180° longitude
Modern time zones:
- Standard zones: UTC-12 to UTC+14 (some zones offset by 30 or 45 minutes)
- Daylight Saving Time: Advances clocks 1 hour in summer in some regions
- Political boundaries: Zones follow country borders, not just longitude
- China uses single time zone (UTC+8) despite spanning 5 geographical zones
Atomic Era: Hours Defined by Seconds (1967-Present)
When the second was redefined atomically in 1967 based on caesium-133 oscillations, the hour inherited this precision:
1 hour = exactly 3,600 SI seconds = 33,074,688,259,200,000 caesium oscillations
Modern atomic clocks maintain this definition with extraordinary stability:
- Caesium fountain clocks: Accurate to 1 second in 100 million years
- Optical lattice clocks: Accurate to 1 second in 15 billion years (2019)
- GPS satellites: Each carries atomic clocks synchronized to nanoseconds
Leap seconds:
- Earth's rotation gradually slows (tidal friction)
- Occasionally, an extra second added to clock time to match Earth rotation
- 27 leap seconds added 1972-2016
- Controversy: May be abolished in favor of "leap hours" every few centuries
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:
-
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
-
Water clocks (clepsydrae):
- Used at night when sundials didn't work
- Water dripped at constant rate through calibrated container
- Divided night into 12 parts
-
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:
-
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
-
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"
-
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: hours vs days
Explore the typical applications for both Hour (imperial/US) and Day (imperial/US) to understand their common contexts.
Common Uses for hours
and Applications
1. Time Zones and Global Coordination
The hour is the basis for global time coordination:
-
UTC (Coordinated Universal Time):
- Global time standard (replaced GMT in 1960s)
- Based on atomic clocks
- All time zones expressed as UTC offset
-
Major time zones:
- EST (Eastern Standard Time): UTC-5
- CST (Central Standard Time): UTC-6
- MST (Mountain Standard Time): UTC-7
- PST (Pacific Standard Time): UTC-8
- GMT/WET (Western European Time): UTC+0
- CET (Central European Time): UTC+1
- IST (Indian Standard Time): UTC+5:30
- JST (Japan Standard Time): UTC+9
- AEST (Australian Eastern Standard Time): UTC+10
-
Business hours across zones:
- "9 AM EST / 6 AM PST" (3-hour difference)
- International meetings: Finding overlapping work hours
- "Follow the sun" support: 24-hour coverage across global offices
-
International Date Line:
- 180° longitude (opposite side of Earth from Prime Meridian)
- Crossing eastward: Lose one day (skip 24 hours forward)
- Crossing westward: Gain one day (repeat 24 hours)
2. Scheduling and Calendar Systems
Hours are the building blocks of schedules:
-
Digital calendars:
- Google Calendar, Outlook: Default 1-hour event blocks
- Day view: Shows 24 hours (or work hours only)
- Week view: 168 hours (7 × 24)
- Buffer time: 15-30 minutes between hour blocks
-
Appointment systems:
- Medical: 15-minute to 1-hour slots
- Salon/spa: 30 minutes to 3 hours
- Professional meetings: 30-minute or 1-hour default
-
Business hours:
- Standard: 9 AM - 5 PM (8 hours, often called "9-to-5")
- Extended: 8 AM - 6 PM (10 hours)
- 24/7 operations: Open all 24 hours, 7 days per week
-
Peak hours vs. off-peak:
- Rush hour: 7-9 AM, 4-7 PM (commute times)
- Electricity pricing: Higher rates during peak demand hours
- Gym: Busiest 5-7 PM (post-work)
3. Astronomy and Earth Science
The hour reflects Earth's rotation:
-
Earth's rotation:
- 360° in ~24 hours = 15° per hour
- Solar noon: Sun crosses local meridian (highest point in sky)
- Local solar time: Based on sun position (varies with longitude)
- Mean solar time: Averaged over year (accounts for orbital eccentricity)
-
Equation of time:
- Sundial time vs. clock time can differ by ±16 minutes
- Due to Earth's elliptical orbit and axial tilt
- Clock time is averaged over the year
-
Hour angle (astronomy):
- Angular distance (in hours) from local meridian
- 1 hour = 15° of celestial sphere rotation
- Used to determine star positions for telescope pointing
-
Sidereal vs. solar day:
- Sidereal day: 23 hours 56 minutes 4 seconds (rotation relative to stars)
- Solar day: 24 hours (rotation relative to sun)
- Difference: Earth moves along orbit, sun appears to shift ~1° per day
4. Energy and Power Consumption
Energy usage measured in watt-hours:
-
Kilowatt-hour (kWh):
- Energy used by 1 kilowatt (1,000 watts) running for 1 hour
- Standard unit for electricity billing
- Average US home: 30 kWh per day (877 kWh per month)
-
Appliance energy use:
- 100W light bulb for 10 hours = 1 kWh
- Electric oven: 2-3 kWh per hour of use
- Central AC: 3-5 kWh per hour
- Laptop: 0.05 kWh per hour (50 watts)
- Refrigerator: 1-2 kWh per day (constant running)
-
Time-of-use pricing:
- On-peak hours: Higher electricity rates (typically 1-9 PM)
- Off-peak hours: Lower rates (typically 9 PM - 9 AM)
- Encourages load shifting to flatten demand curve
-
Battery capacity:
- Milliamp-hour (mAh) or watt-hour (Wh)
- Phone battery: 3,000 mAh (11 Wh) ≈ 2-3 hours screen-on time
- Laptop battery: 50-100 Wh ≈ 5-10 hours use
- Electric car: 60-100 kWh ≈ 250-400 miles range
5. Healthcare and Medicine
Medical dosing and monitoring uses hours:
-
Medication schedules:
- "Every 4 hours" = 6 times per day
- "Every 6 hours" = 4 times per day (QID: quater in die)
- "Every 8 hours" = 3 times per day (TID: ter in die)
- "Every 12 hours" = 2 times per day (BID: bis in die)
- "Every 24 hours" = 1 time per day (QD: quaque die)
-
Drug half-life:
- Time for drug concentration to decrease by half
- Acetaminophen: 2-3 hours
- Caffeine: 5-6 hours
- Alcohol: Eliminated at ~0.015% BAC per hour
-
Fasting requirements:
- Pre-surgery: 8-12 hours fasting (NPO: nil per os)
- Cholesterol test: 9-12 hours fasting
- Glucose tolerance test: 8-hour overnight fast
-
Labor and delivery:
- Labor stages measured in hours
- First stage: 6-12 hours (first baby), 4-8 hours (subsequent)
- Active labor: Cervical dilation ~1 cm per hour
- Pushing stage: 1-3 hours (first baby), 15 min-2 hours (subsequent)
-
Medical shift lengths:
- Resident work-hour restrictions: Max 80 hours per week, max 24-hour shifts
- Nurse shifts: Typically 8 or 12 hours
- Concerns about fatigue and patient safety
6. Computing and Technology
Hours measure uptime and usage:
-
Server uptime:
- "Five nines" (99.999%): 5.26 minutes downtime per year
- "Four nines" (99.99%): 52.6 minutes downtime per year
- "Three nines" (99.9%): 8.77 hours downtime per year
- Measured in hours of continuous operation
-
Data retention:
- Backup schedules: Hourly, daily, weekly
- Log rotation: Every 24 hours (daily logs)
- Cloud storage: Deleted items retained 30 days (720 hours)
-
Usage tracking:
- Screen time: Hours per day on devices
- YouTube Creator Studio: Watch hours (4,000 hours past year for monetization)
- Video games: "Hours played" stat
- Social media: "You've been using this app for 2 hours today"
-
Rendering and processing:
- Video rendering: "2 hours to render 10-minute 4K video"
- 3D modeling: "12-hour render time for scene"
- Machine learning training: "Training took 100 GPU-hours"
7. Legal and Regulatory
Many laws reference hours:
-
Work hour regulations:
- Fair Labor Standards Act (FLSA): 40-hour work week threshold
- Overtime pay: Time-and-a-half for hours beyond 40/week
- Maximum driving hours: Truckers limited to 11 hours driving per 14-hour window
-
Alcohol service hours:
- Many states prohibit alcohol sales certain hours (e.g., 2 AM - 6 AM)
- "Last call": Final hour for ordering drinks
-
Quiet hours:
- Residential noise ordinances: Often 10 PM - 7 AM
- College dorms: 11 PM - 8 AM weeknights
-
Statute of limitations:
- Measured in years, but technically hours
- Parking tickets: Often 72-hour (3-day) payment window
- Right to return/refund: 24-48 hour windows
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 Hour (h)
How many minutes are in an hour?
Exactly 60 minutes. This comes from the ancient Babylonian base-60 (sexagesimal) number system, which the Egyptians and Greeks adopted for dividing hours. The Latin term "pars minuta prima" (first small part) referred to the first 60-part division of an hour, giving us the modern "minute."
How many seconds are in an hour?
Exactly 3,600 seconds (60 minutes × 60 seconds).
Since 1967, when the second was redefined using atomic caesium-133 clocks, one hour equals:
- 3,600 atomic seconds
- 33,074,688,259,200,000 caesium-133 oscillations (33.07 quadrillion)
This makes the hour one of the most precisely defined units of time in existence.
How many hours are in a day?
Exactly 24 hours in one solar day.
Why 24?
- Ancient Egyptians divided day and night into 12 parts each
- 12 + 12 = 24-hour cycle
- Earth rotates 360° in 24 hours = 15° per hour
- This 15° per hour relationship forms the basis for time zones
Note: A sidereal day (rotation relative to stars) is 23 hours, 56 minutes, 4 seconds, but civil timekeeping uses the 24-hour solar day (rotation relative to the sun).
How many hours are in a year?
8,760 hours in a standard 365-day year.
Calculation: 365 days × 24 hours = 8,760 hours
For a leap year (366 days): 8,784 hours (24 more hours).
Work year: Assuming 40-hour weeks and 52 weeks, a full-time work year is 2,080 work hours (not including holidays or vacation).
Why do we use 12-hour AM/PM instead of 24-hour time?
Historical reasons:
- Ancient Egyptians and Romans divided day and night into 12 parts each
- This became culturally entrenched in English-speaking countries
- 12-hour clocks were simpler to manufacture (only need 1-12 markers)
Why 24-hour format exists:
- Eliminates AM/PM confusion (especially 12:00 AM vs. 12:00 PM)
- Preferred in military, aviation, healthcare, computing for clarity
- Standard in most non-English-speaking countries
- ISO 8601 international standard uses 24-hour format
Current usage:
- 12-hour: US, Canada, Australia, Philippines, parts of UK
- 24-hour: Most of Europe, Asia, Africa, South America, military worldwide
What's the difference between a 24-hour day and Earth's rotation?
Solar day (24 hours): Time for sun to return to same position in sky Sidereal day (23h 56m 4s): Time for Earth to rotate 360° relative to distant stars
Why the difference?
- Earth orbits the sun while rotating
- After one 360° rotation, Earth has moved ~1° along its orbit
- Must rotate an additional ~1° (4 minutes) for sun to return to same position
- 365.25 solar days per year, but 366.25 sidereal days per year (one extra rotation)
Practical impact:
- Astronomers use sidereal time for telescope pointing
- Civil timekeeping uses solar time (24-hour day)
- Stars rise ~4 minutes earlier each day (sidereal effect)
How do Daylight Saving Time changes work?
Spring forward (start of DST):
- Clocks advance 1 hour at 2:00 AM → becomes 3:00 AM
- The hour from 2:00-3:00 AM doesn't exist that day
- Day has only 23 hours
- "Lose an hour of sleep"
Fall back (end of DST):
- Clocks retreat 1 hour at 2:00 AM → becomes 1:00 AM again
- The hour from 1:00-2:00 AM occurs twice
- Day has 25 hours
- "Gain an hour of sleep"
Global variation:
- Northern Hemisphere: Starts March/April, ends October/November
- Southern Hemisphere: Starts September/October, ends March/April
- Many countries don't observe DST (China, Japan, India, most of Africa)
- Arizona and Hawaii (US states) don't observe DST
Controversy: Growing movement to abolish DST due to health impacts, minimal energy savings.
Why are time zones roughly 15 degrees wide?
Simple math:
- Earth rotates 360° in 24 hours
- 360° ÷ 24 hours = 15° per hour
- Each time zone theoretically spans 15° longitude
Reality is messier:
- Political boundaries: Zones follow country/state borders
- China uses single time zone (UTC+8) despite spanning 60° longitude (5 theoretical zones)
- India uses UTC+5:30 (half-hour offset from standard)
- Some zones are 30 or 45-minute offsets (Nepal: UTC+5:45)
Practical example:
- Greenwich, England: 0° longitude (Prime Meridian)
- Every 15° east: Add 1 hour (15°E = UTC+1, 30°E = UTC+2, etc.)
- Every 15° west: Subtract 1 hour (15°W = UTC-1, 30°W = UTC-2, etc.)
What is a "billable hour"?
A billable hour is time spent on client work that can be charged to the client, common in legal, consulting, and professional services.
How it works:
- Professionals track time in increments (often 6 minutes = 0.1 hour)
- Multiply hours by hourly rate
- Example: 7.5 billable hours × $300/hour = $2,250
Billing increment examples:
- 6 minutes = 0.1 hour (common in legal)
- 15 minutes = 0.25 hour (quarter-hour)
- Some firms round up to nearest increment
Utilization rate:
- Target: 1,500-2,000 billable hours per year (out of 2,080 work hours)
- Remaining time: Non-billable (admin, business development, training)
- 75-80% utilization considered good in many professions
Ethical concerns:
- Pressure to inflate hours
- Some professions moving to flat-fee or value-based pricing
Can an hour ever be longer or shorter than 60 minutes?
In standard timekeeping: No. An hour is always exactly 60 minutes or 3,600 seconds.
Exceptions and special cases:
-
Leap seconds:
- Very rarely, an extra second added to last minute of day
- Makes that minute 61 seconds, but hour still 3,600 seconds overall
- Last hour of day becomes 3,601 seconds
- 27 leap seconds added 1972-2016
-
Daylight Saving Time transitions:
- "Spring forward": The 2:00 AM hour is skipped (day has 23 hours)
- "Fall back": The 1:00 AM hour occurs twice (day has 25 hours)
- This affects the day length, not individual hour length
-
Historical seasonal hours:
- Ancient/medieval timekeeping used "unequal hours"
- Summer daylight hour ≈ 75 minutes
- Winter daylight hour ≈ 45 minutes
- Obsolete since mechanical clocks standardized equal hours
Future possibility:
- If leap seconds abolished, may use "leap hours" every few centuries instead
Why is rush hour called an "hour" when it lasts 2-3 hours?
Etymology: "Rush hour" originally referred to the peak single hour of commuter traffic, but the term stuck even as traffic congestion expanded.
Modern reality:
- Morning rush: 7:00-9:00 AM (2-3 hours)
- Evening rush: 4:00-7:00 PM (3-4 hours)
- Can extend longer in major cities
Related terms:
- "Peak hours": Broader term for high-traffic periods
- "Congestion pricing": Charging more during rush hours to reduce traffic
- "Off-peak": Outside rush hours, usually smoother travel
Cultural note: The term persists despite inaccuracy, similar to how we still say "dial a phone" or "roll down the window."
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:
-
Roman calendar (753 BCE):
- Originally 10 months, 304 days (March-December)
- Winter was monthless period
-
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)
-
Julius Caesar (45 BCE):
- Julian calendar: 365.25-day year
- Added day to February every 4 years (leap year)
- February remained shortest month
-
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:
-
Babylonian astronomy (c. 2000 BCE):
- Seven visible celestial bodies: Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn
- Each "ruled" one day
- 7-day planetary week
-
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"
-
Roman adoption:
- Romans adopted 7-day week (1st-3rd century CE)
- Named days after planets/gods
- Spread throughout Roman Empire
-
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:
-
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
-
Daylight Saving Time:
- "Spring forward" day: 23 hours (lose 1 hour)
- "Fall back" day: 25 hours (gain 1 hour)
- Only in regions observing DST
-
Time zone transitions:
- Crossing International Date Line can skip or repeat a day
- Country changing time zones can alter day length
-
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: Hour to Day
| Hour (h) | Day (d) |
|---|---|
| 0.5 | 0.021 |
| 1 | 0.042 |
| 1.5 | 0.063 |
| 2 | 0.083 |
| 5 | 0.208 |
| 10 | 0.417 |
| 25 | 1.042 |
| 50 | 2.083 |
| 100 | 4.167 |
| 250 | 10.417 |
| 500 | 20.833 |
| 1,000 | 41.667 |
People Also Ask
How do I convert Hour to Day?
To convert Hour to Day, enter the value in Hour in the calculator above. The conversion will happen automatically. Use our free online converter for instant and accurate results. You can also visit our time converter page to convert between other units in this category.
Learn more →What is the conversion factor from Hour to Day?
The conversion factor depends on the specific relationship between Hour 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 Hour?
Yes! You can easily convert Day back to Hour by using the swap button (⇌) in the calculator above, or by visiting our Day to Hour converter page. You can also explore other time conversions on our category page.
Learn more →What are common uses for Hour and Day?
Hour 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.
Helpful Conversion Guides
Learn more about unit conversion with our comprehensive guides:
All Time Conversions
Other Time Units and Conversions
Explore other time units and their conversion options:
- Second (s) • Hour to Second
- Minute (min) • Hour to Minute
- Week (wk) • Hour to Week
- Month (mo) • Hour to Month
- Year (yr) • Hour to Year
- Millisecond (ms) • Hour to Millisecond
- Microsecond (μs) • Hour to Microsecond
- Nanosecond (ns) • Hour to Nanosecond
- Decade (dec) • Hour to Decade
- Century (c) • Hour to Century
Verified Against Authority Standards
All conversion formulas have been verified against international standards and authoritative sources to ensure maximum accuracy and reliability.
National Institute of Standards and Technology — Official time standards and definitions
Bureau International des Poids et Mesures — Definition of the SI base unit for time
Last verified: December 3, 2025