Why explore Neptune

Neptune, our outermost planet, is a windy blue world with exotic ice, raging storms, rings, and a moon that could have a subsurface ocean.

Neptune in natural color from the Voyager 2 spacecraft. Credits: NASA,  JPL-Caltech, Justin Cowart

Why study Neptune

Neptune, along with its cousin Uranus, is the least-explored planet in our solar system, having been visited by a spacecraft only once. Yet we’ve found more Neptune-sized worlds orbiting other stars than any other type of planet.  In order to understand other solar systems and figure out whether our own is unique, we need to learn more about the windy blue world in our own backyard.

Like Jupiter and Saturn, Neptune’s atmosphere consists mostly of hydrogen and helium, but it also has methane that absorbs red light, giving it a deep blue hue. Beneath the atmosphere lies an ocean of water, ammonia, and methane, squeezed by intense pressures into a semi-solid state. For this reason we call Neptune an ice giant, though the ice isn’t anything like what you’d find in your freezer, with temperatures likely reaching thousands of degrees! Electric currents flowing through this icy-hot ocean may be responsible for powering Neptune’s strong and unusually complex magnetic field.

Earth compared to Uranus and Neptune. Credits: NASA, JPL-Caltech, Björn Jónsson, Justin Cowart

Where Neptune formed and how it got its water isn’t clear. The disk of dust and gas that formed our solar system probably didn’t contain enough material to form Neptune at its current location, 30 times farther from the Sun than Earth. Like the other outer planets, it was probably born closer to the Sun before moving outward, though the Sun would have evaporated its water had Neptune been too close. By figuring out where Neptune was born and how the planet evolved, scientists learn what conditions in the early solar system were like, around the time life arose on Earth.

Neptune has 14 known moons, half of which were likely captured by the planet’s gravity rather than forming in place. Only one moon, Triton, is big enough to be spherical. It has planet-like characteristics similar to Pluto such as a complex icy surface and thin nitrogen atmosphere, and may have started off as a free-roaming dwarf planet. Geysers of nitrogen erupt from Triton’s surface that may be coming from a subsurface water ocean. Future missions would help confirm whether the ocean exists, and whether it might be habitable to life as we know it.

Just like Saturn, Neptune has a set of rings shepherded by small moons and made up of cold, icy particles. But its outermost ring is not complete, comprising five distinct arcs. Scientists think the planet’s moon Galatea prevents particles in these arcs from spreading out to complete the ring but no one knows for sure.

As Voyager 2 receded from Neptune, it observed the two outermost thin rings in glancing sunlight (at a phase angle of 135°). Three bright arcs in the outermost rings are visible. Credits: NASA, JPL-Caltech

That one time we explored Neptune

It takes a spacecraft a long time to reach Neptune, and we’ve only done it once. NASA launched the nuclear-powered Voyager 2 spacecraft in 1977 to fly past every giant planet in the outer solar system, taking advantage of a rare planetary alignment that only happens every 175 years. Voyager 2 passed Neptune in August 1989.

Its instruments measured an atmospheric temperature of -220 degrees Celsius, with wind speeds as high as 2,100 kilometers per hour, possibly driven from heat radiating deep within the planet. Voyager 2 also made the definitive observations of the planet’s rings and saw storms raging across the face of the planet, the largest being an Earth-sized anticyclone similar to Jupiter’s famous Great Red Spot.

Just like at Uranus, Voyager 2 found that Neptune’s magnetic field doesn’t cleanly intersect the planet’s core and is tilted significantly away from the north and south poles. No other planet in our solar system has such complex magnetic fields as the ice giants.

Voyager 2 also revealed Triton’s relatively young, crater-free surface, indicating geologic processes at work. Further attesting this were fractures, ridges, and lava plains in the north, as well as kilometers-high nitrogen geysers in the south that hinted at a possible subsurface ocean.

Voyager 2 acquired the images for this high-resolution mosaic of Triton on 25 August 1989. Visible in the south are dark splotches formed by nitrogen geysers that could be linked to a subsurface ocean. Credits: NASA, JPL, Ted Stryk

The road ahead

With no new space missions to Neptune since Voyager 2, scientists have relied on the Hubble Space Telescope and large ground-based telescopes to regularly observe the planet. The observations have discovered more moons, monitored seasonal storms, and even detected gases in Triton’s thin atmosphere.

Infrared images of Neptune taken by the Hubble Space Telescope in 2005. Bright belts and spots show sign of atmospheric activity. Credit: NASA, ESA, E. Karkoschka, H.B. Hammel

A Neptune orbiter would help us better understand ice giants by measuring the planet’s magnetic field, mapping gravity variations and atmospheric wobbles to understand the core, and observing how heat is radiated on the planet’s night side. A probe dropped into Neptune’s frigid atmosphere could precisely measure the composition of gases, helping scientists figure out where Neptune formed and how it evolved.

China is considering a Voyager-like mission interstellar space that would launch in 2024 and make a Neptune flyby in 2038. The spacecraft would include an atmospheric probe. NASA is considering a low-cost Neptune mission called TRIDENT that would perform a single flyby of Triton, mapping the moon’s surface and exploring whether it has a subsurface ocean. The existence of such an ocean would open up possibilities for habitable worlds very distant from their stars.

The agency is also considering a flagship mission to either Uranus or Neptune as part of the decadal survey, a report produced by the U.S. scientific community every 10 years to guide future NASA missions. The last decadal survey favored a Uranus mission to lower costs.

This image of Neptune and Triton was captured by Voyager 2 as it departed the Neptune system on 31 August 1989. South is at bottom; Voyager 2’s flyby over Neptune’s northern hemisphere bent the spacecraft’s trajectory downwards out of our solar system’s orbital plane. Credit: NASA / JPL-Caltech / Justin Cowart

Originally published at The Planetary Society.

Like my work?
I don’t display ads, support me and get exclusive benefits in return. 🚀

2 thoughts on “Why explore Neptune”