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Nereid - NASA/JPL

Nereid

The Wild Orbit Moon

A moon with the most eccentric orbit of any major moon - its distance from Neptune varies by 7 million kilometers!

Orbital Period
360.14 days
Tidal Locking
No
Rotates freely
Planet Rotations
536.0×
per orbit
Atmosphere
No

🌙 Mind-Blowing Fact

Nereid has the WILDEST orbit of any major moon! Its distance from Neptune varies from 1.4 million km to 9.6 million km. That's a 6.8x difference! It's probably a captured Kuiper Belt object that got too close to Neptune!

What is Time on Nereid?

What is Time on Nereid?

Nereid is Neptune's third-largest moon, but by far its strangest. With the most eccentric orbit of any major moon, Nereid is probably a captured Kuiper Belt object.

The 360-Day Orbit

  • One orbit = 360 Earth days - Nearly a full year!
  • Longest orbital period of any inner system moon
  • NOT tidally locked - Rotates every 10.8 hours!
  • Neptune rotates 536 times per orbit - Watch it spin wildly

The Eccentric Orbit

Nereid's orbit is EXTREMELY eccentric:

  • Periapsis (closest): 1.4 million km
  • Apoapsis (farthest): 9.6 million km
  • Eccentricity: 0.75 (most eccentric of large moons!)
  • Distance varies by 6.8x during each orbit

Not Tidally Locked!

Unlike almost all major moons, Nereid rotates independently:

  • Rotation: 10.8 hours
  • Orbit: 360 days
  • Result: Experiences ~800 days per orbit!
  • Neptune appears different sizes throughout year

Probably a Capture

Nereid's weird orbit suggests:

  • Originally a Kuiper Belt object
  • Captured by Neptune during migration
  • Never circularized orbit
  • Never tidally locked due to distance
  • Will likely escape or collide eventually (billions of years)

The Variable View

From Nereid, Neptune's appearance changes dramatically:

  • At periapsis: 0.96° across (2 full moons)
  • At apoapsis: 0.14° across (smaller than Venus from Earth!)
  • Distance changes create "Neptune seasons"
  • But these seasons take 360 days!

A Day in the Life

The Captured Wanderer

You orbit Nereid at apoapsis - the farthest point from Neptune. You check the distance: 9.6 million kilometers. Neptune is barely visible - a blue-green dot only 0.14 degrees across, hardly larger than Venus appears from Earth.

"Six months ago, we were at periapsis," your companion says, checking logs. "1.4 million km away. Neptune filled the sky - nearly a full degree across. Now look at it. A dot."

You watch Nereid rotate below - a lumpy, irregular moon completing a rotation every 10.8 hours. Unlike most moons, Nereid isn't tidally locked. It spins freely, like an asteroid. Because that's probably what it once was - a Kuiper Belt object that wandered too close to Neptune and got captured.

"How long until we start falling back?" you ask.

"We're already falling," the companion replies. "We passed apoapsis three days ago. Now begins the long fall back toward Neptune. In 180 days, we'll reach periapsis again. Neptune will grow from a dot to a disk filling the sky. And then we'll swing back out, spending another 180 days reaching this point again."

You look at the distant Neptune, its blue color barely visible. Somewhere on that planet, a year passes while Nereid completes one orbit. On Neptune's surface (if it had one), you'd see 536 sunrises. But out here, on captured Nereid, you experience time differently. Wild swings in distance. 800 ten-hour days per orbital year. Neptune growing and shrinking like breathing.

"Time is a circle for most moons," you say. "But for Nereid, time is an ellipse. A long, stretched-out ellipse."

"An ellipse that proves Nereid doesn't belong here," the companion adds. "It was captured. And someday - in a billion years, or ten billion - it will either escape or collide. Nereid's time at Neptune is temporary. Geological temporary. But temporary nonetheless."

You watch the small blue dot that is Neptune, and wonder what Nereid saw when it was still in the Kuiper Belt, before it was captured, when its time was its own.

Thought Experiments

Why isn't Nereid tidally locked like other moons?

Distance! Tidal locking happens when a moon orbits close enough for tidal forces to gradually slow its rotation until it matches its orbit. Nereid's average distance (5.5 million km) is too far for strong tidal forces. Plus, its eccentric orbit means tidal forces vary wildly - strong at periapsis, weak at apoapsis. This prevents tidal locking. Nereid has probably kept its original 10.8-hour rotation since capture!

Will Nereid's orbit ever circularize?

Eventually, but it would take hundreds of billions of years - longer than the Sun will live! Tidal forces slowly circularize orbits, but the process is slow for distant, low-mass moons. Nereid's orbit is SO eccentric and SO distant that it would take an incredibly long time. More likely, Nereid will be ejected by gravitational interactions with Triton or other planets before its orbit circularizes.

The Science of Time on Nereid

The Science of Eccentric Orbits

Nereid's eccentricity (e = 0.75) is extreme for a major moon:

Comparison:

- Moon (Earth): e = 0.055

- Io (Jupiter): e = 0.004

- Triton (Neptune): e = 0.000016

- Nereid: e = 0.75 (13x more than most comets!)

Orbital mechanics:

- At periapsis: Velocity = 2.6 km/s

- At apoapsis: Velocity = 0.4 km/s

- Speed varies by 6.5x!

- Orbital energy constant, but kinetic/potential trade off

Origin theories:

1. Capture from Kuiper Belt (most likely)

2. Scattered by Triton when Triton was captured

3. Original irregular moon that avoided tidal circularization

Evidence favors capture - no native moon would have such an eccentric orbit.