Exploring Our Cosmic Calendar: How Long is a Year on Each Planet?

The shortest year in our solar system is Mercury at 88 Earth days. The longest is Neptune at 165 Earth years. 

The planets in our solar system. Credit: WikiMedia Commons.

Our solar system is a bustling celestial neighborhood, with planets whirling around the Sun in a mesmerizing dance. Each planet follows its own timetable, spinning on its axis and orbiting the Sun at its unique pace. Let's take a fascinating journey through our solar system and explore the duration of a year on each planet, measured in Earth days:

  • Mercury– 88 Earth days
  • Venus– 225 Earth days
  • Earth– 365 days
  • Mars– 687 Earth days
  • Jupiter– 4,331 Earth days or 12 Earth years
  • Saturn- 10,747 Earth days or 29.4 Earth years
  • Uranus– 30,589 Earth days or 84 Earth years
  • Neptune– 59,800 Earth days or 165 Earth years

Rotation and revolution

On planets other than Earth, we use Earth's tropical year as a measuring stick, about 365 solar days long. A solar day is the time it takes the Earth to complete one full revolution on its axis, marked by the Sun's position in the sky. Meanwhile, a year is defined by a planet's orbit around the sun, called a revolution.

Interestingly, all the celestial bodies in our solar system move in the same pattern, but at different speeds. Gas giants like Jupiter and Saturn, along with the ice giants Uranus and Neptune, rotate faster than rocky planets like Earth, Mars, Venus and Mercury. Each planet's rotation rate is influenced by its formation from the protoplanetary disk orbiting our young Sun. However, the reason for the remarkably fast rotation of the giant planets still remains a mystery.

Laws of motion

Kepler's third law of motion unravels the complex relationship between a planet's orbital period and its distance from our brightest star. Planets farther from the Sun begin long journeys, orbiting at slower speeds due to the gravitational pull from the distant Sun. In contrast, those closer to the Sun zip faster, under the grip of its powerful gravity.

For example, Mercury, the Sun's nearest neighbor, completes one revolution in just 88 days. At the opposite end of the solar system, Neptune resides on the far side, leisurely orbiting every 165 years.

Moreover, the motion of the planets is not uniform in their orbital paths. Orbits, similar to flat circles or ellipses, produce variations in speed. Kepler's second law of motion uncovers this phenomenon: As a planet moves closer to the Sun in its orbit, it speeds up, simply because it is moving farther away from our star's bright embrace


Mercury, the swift-footed messenger of the cosmos, exhibits a strange dance in the heavens. While its rotation on its axis is relaxed, taking 59 Earth days to complete one rotation, its journey around the Sun is unusually fast. Every 88 Earth days, Mercury completes one full orbit, tracing a path that prevents its slow rotation.

Yet, the speed of the Sun across Mercury's sky is the same. As Mercury accelerates along its elliptical orbit, its speed fluctuates, causing the Sun to perform a complex ballet. This celestial spectacle means that one solar day, which encompasses a full cycle of day and night, spans about 176 Earth days on Mercury's scorched surface.


Venus, where a year is about 225 days. Credit: NASA/JPL-Caltech

Venus, the sizzling jewel of the solar system, dances to its own rhythm. It takes approximately 225 Earth days for Venus to complete a single orbit around the Sun. However, its mesmerizing spin paints a unique picture in the cosmic tapestry. Unlike most planets, which gracefully pirouette counterclockwise as they orbit, Venus performs a mesmerizing retrograde waltz, twirling in a clockwise direction. This distinctive motion means that Venus takes a leisurely 243 Earth days to complete just one rotation on its axis.


Earth, in an image taken from the International Space Station on March 9, 2015. Credit: NASA

Earth, our cosmic home, begins a mesmerizing journey around the Sun, completing a full orbit in exactly 365.25 days. Meanwhile, Earth's graceful rotation on its axis traces the daily celestial ballet, rotating once every 23.9 hours.


The Red Planet shows off its distinct color, as well as one bright polar cap. Credit: NASA

A Martian year spans 687 Earth days or 1.88 Earth years, a testament to the Red Planet's longer orbital journey around the Sun. Martians mark time in sols, where a year translates to 669.6 sols. Despite the stark contrast in year length, Mars mirrors Earth's rotation rhythm, completing one spin on its axis every 24.6 hours.


Jupiter, as imaged by the Hubble Space Telescope. Credit: NASA, ESA, A. Simon (Goddard Space Flight Center) and M.H. Wong (University of California, Berkeley)

Jupiter, the colossal gas giant, whirls through its days at a dizzying pace, completing a full rotation in under 10 hours. Despite its speedy spin, Jupiter's immense distance from the Sun extends its orbit, requiring a whopping 12 Earth years to complete a single jovian year. Light, racing across the cosmos, takes approximately 43 minutes to reach Jupiter's lofty atmosphere, a stark contrast to the mere 8 minutes it takes to illuminate our home planet Earth.


Saturn as it appeared June 8, 2017, through a Celestron 8-inch Schmidt-Cassegrain telescope. Credit: Molly Wakeling

Trailing closely behind Jupiter, Saturn boasts the second-shortest day among the planets, completing one rotation every 10.7 Earth hours. However, Saturn's spectacular orbit around the Sun extends at a more leisurely pace, requiring 10,756 Earth days or 29.4 Earth years to complete. Saturn's axial tilt of 26.7° adds a fascinating dynamism to its appearance, allowing us to see its spectacular rings change over time. As Saturn glides gracefully through space, we observe different perspectives of its rings - from their northern flanks, to their fringes, and finally to their southern flanks. Anticipation is building for the next ring flyover, scheduled for 2025, when Saturn's rings will once again be visible on edge, treating observers to a celestial spectacle.


Uranus gets its blue-green color from methane gas, which absorbs red wavelengths of light. Credit: JPL / NASA

A journey around the Sun on Uranus is truly an odyssey, spanning roughly 84 Earth years – a lifetime in itself! Despite its leisurely orbit, time flies on the ice giant, with a day passing in a mere 17.2 hours. Adding to its enigmatic allure, Uranus seems to dance to its own rhythm, rotating retrograde, or counterclockwise, like Venus. What's more, Uranus showcases a peculiar tilt, seemingly lounging on its side at an angle of 97.8°, an astronomical feat that sets it apart in the cosmic ballet.


It takes big optics and perfect seeing (or adaptive optics) to catch cloud features on the distant ice giant Neptune. The best time to see it is at opposition. Credit: ESO/P. Weilbacher (AIP)

A day on Neptune slips by in just 16 Earth hours, a fleeting passage of time amidst the swirling winds of this distant ice giant. Yet, Neptune's grand circuit around the Sun extends over 165 Earth years, encompassing a staggering 59,800 Earth days. Despite its vast orbit, Neptune experiences the subtle rhythms of seasons, owing to its axial tilt of 28.3°. However, the planet's lengthy year stretches each of its four seasons to over 40 Earth years, a testament to the majestic scale of time on this distant world.

Honorable mention: Pluto

The distant, icy dwarf planet Pluto was first imaged in detail by the New Horizons spacecraft as it flew past in July 2015. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Alex Parker

For 76 years, from 1930 to 2006, Pluto held the esteemed title of the solar system's ninth planet. However, in 2006, the International Astronomical Union made the landmark decision to reclassify Pluto as a dwarf planet. Currently, there are five recognized dwarf planets in our cosmic neighborhood. A year on Pluto spans an astonishing 248 Earth years, while a single day on this distant world stretches over 153.3 Earth hours, equivalent to just over 6 Earth days.

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