Hour to Millisecond Converter

Convert hours to milliseconds with our free online time converter.

Quick Answer

1 Hour = 3600000 milliseconds

Formula: Hour × conversion factor = Millisecond

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

Hour to Millisecond Calculator

How to Use the Hour to Millisecond Calculator:

  1. Enter the value you want to convert in the 'From' field (Hour).
  2. The converted value in Millisecond 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 Hour to Millisecond: Step-by-Step Guide

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

Formula:

1 Hour = 3.6000e+6 milliseconds

Example Calculation:

Convert 60 hours: 60 × 3.6000e+6 = 2.1600e+8 milliseconds

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 Hour and a Millisecond?

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

A millisecond is a unit of time equal to one-thousandth (1/1,000) of a second.

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

History of the Hour and Millisecond

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:

  1. 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)
  2. 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

The millisecond is derived from the SI base unit, the second, using the metric prefix 'milli-', indicating a factor of 10⁻³. Its common usage grew with the need for finer time measurements in science and technology, particularly in fields like computing and electronics.

Common Uses and Applications: hours vs milliseconds

Explore the typical applications for both Hour (imperial/US) and Millisecond (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 milliseconds

  • Computing: Measuring network latency (ping times), hard drive seek times, human reaction times in psychological tests, frame duration in video (e.g., 60 fps is ~16.7 ms per frame).
  • Audio: Measuring delays and processing times in audio signals.
  • Sports: Timing in races where differences are extremely small (e.g., swimming, track and field).
  • Science: Measuring short-duration events, such as the firing of a neuron or rapid chemical processes.
  • User Interface: Often used as a target for response times in interactive systems (e.g., aiming for under 100 ms for a feeling of instant response).

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:

  1. 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
  2. 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
  3. 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 Millisecond (ms)

How many milliseconds are in one second?

There are 1,000 milliseconds in a second.

How many milliseconds are in one minute?

There are 60,000 milliseconds in a minute (1000 ms/s * 60 s/min).

Is a millisecond a long time for a computer?

In computing terms, a millisecond can be quite long. Processors perform millions of operations in a millisecond. Network latency is often measured in tens or hundreds of milliseconds.

Conversion Table: Hour to Millisecond

Hour (h)Millisecond (ms)
0.51,800,000
13,600,000
1.55,400,000
27,200,000
518,000,000
1036,000,000
2590,000,000
50180,000,000
100360,000,000
250900,000,000
5001,800,000,000
1,0003,600,000,000

People Also Ask

How do I convert Hour to Millisecond?

To convert Hour to Millisecond, 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.

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What is the conversion factor from Hour to Millisecond?

The conversion factor depends on the specific relationship between Hour and Millisecond. 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 Millisecond back to Hour?

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

Learn more →

What are common uses for Hour and Millisecond?

Hour and Millisecond 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.

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All Time Conversions

Second to MinuteSecond to HourSecond to DaySecond to WeekSecond to MonthSecond to YearSecond to MillisecondSecond to MicrosecondSecond to NanosecondSecond to DecadeSecond to CenturySecond to MillenniumSecond to FortnightSecond to Planck TimeSecond to ShakeSecond to Sidereal DaySecond to Sidereal YearMinute to SecondMinute to HourMinute to DayMinute to WeekMinute to MonthMinute to YearMinute to MillisecondMinute to MicrosecondMinute to NanosecondMinute to DecadeMinute to CenturyMinute to MillenniumMinute to FortnightMinute to Planck TimeMinute to ShakeMinute to Sidereal DayMinute to Sidereal YearHour to SecondHour to MinuteHour to DayHour to WeekHour to MonthHour to YearHour to MicrosecondHour to NanosecondHour to DecadeHour to CenturyHour to MillenniumHour to FortnightHour to Planck TimeHour to ShakeHour to Sidereal DayHour to Sidereal YearDay to SecondDay to MinuteDay to HourDay to WeekDay to MonthDay to YearDay to MillisecondDay to MicrosecondDay to NanosecondDay to DecadeDay to CenturyDay to MillenniumDay to FortnightDay to Planck TimeDay to ShakeDay to Sidereal DayDay to Sidereal YearWeek to SecondWeek to MinuteWeek to HourWeek to DayWeek to MonthWeek to YearWeek to MillisecondWeek to MicrosecondWeek to NanosecondWeek to DecadeWeek to CenturyWeek to MillenniumWeek to FortnightWeek to Planck TimeWeek to ShakeWeek to Sidereal DayWeek to Sidereal YearMonth to SecondMonth to MinuteMonth to HourMonth to DayMonth to WeekMonth to YearMonth to MillisecondMonth to MicrosecondMonth to NanosecondMonth to DecadeMonth to CenturyMonth to MillenniumMonth to FortnightMonth to Planck TimeMonth to ShakeMonth to Sidereal DayMonth to Sidereal YearYear to SecondYear to MinuteYear to HourYear to DayYear to WeekYear to MonthYear to MillisecondYear to MicrosecondYear to NanosecondYear to DecadeYear to CenturyYear to MillenniumYear to FortnightYear to Planck TimeYear to ShakeYear to Sidereal DayYear to Sidereal YearMillisecond to SecondMillisecond to Minute

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