We've only been to Pluto once, and it's so hard to get there we'll probably never go again.

We've only been to Pluto once, and it's so hard to get there we'll probably never go again.

Planetary Science Limits

Ever wonder why we've only visited Pluto once? Space seems empty, but getting there involves solving puzzles that would make Einstein scratch his head. One slight miscalculation early on becomes a mission-ending disaster years later.

Pluto's Discovery

In 1930, young astronomer Clyde Tombaugh was methodically examining photographic plates at Lowell Observatory when he spotted something extraordinary. It was a tiny, moving speck. By 1989, robotic spacecraft had visited all known planets from Mercury to Neptune, leaving only distant Pluto unexplored. 

File:Clyde W. Tombaugh.jpegUnknown authorUnknown author, Wikimedia Commons

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Pluto's Discovery (Cont.)

What Tombaugh couldn't have imagined was that he'd discovered the first member of an entire population of icy worlds beyond Neptune, making Pluto not just remote, but part of a vast, debris-filled region that would challenge every aspect of spacecraft design.

File:Pluto.jpgC m handler, Wikimedia Commons

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New Horizons

After nearly 20 years of political battles, budget cuts, and outright cancellations, New Horizons finally launched on January 19, 2006, becoming humanity's first and only successful mission to Pluto. It was cancelled at least six times between 1990 and 2005, with politicians dismissing it as too expensive.

File:15-011a-NewHorizons-PlutoFlyby-ArtistConcept-14July2015-20150115.jpgJohns Hopkins University Applied Physics Laboratory/Southwest Research Institute, Wikimedia Commons

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Distance Challenge

Pluto's distance, approximately 3 billion miles (5 billion km) from Earth, presented power difficulties for the New Horizons designers, as the sun's rays at that distance are too weak to produce power. New Horizons took 9 years and 5 months to get to Pluto.

File:Pluto Charon Moon Earth Comparison.pngYucatan, Wikimedia Commons

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Distance Challenge (Cont.)

At a distance of approximately 39 AU from the Sun and traveling at an average speed of 4.1 AU per year, sunlight at Pluto's distance is nearly 1,000 times weaker than on Earth. This makes every engineering decision exponentially more complex.

File:Pluto-Charon system.jpgESO, Wikimedia Commons

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Mass Limitation

Every gram matters when you're heading to the edge of the solar system. Even using the Lockheed Martin Atlas V rocket, one of the most powerful in the US fleet, New Horizons had to weigh approximately 1,050 pounds. 

File:MRO Liftoff.jpegCraigboy, Wikimedia Commons

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Mass Limitation (Cont.)

The chosen version of the Atlas V utilized five strap-on solid rocket boosters, higher than any other launch, plus a powerful Centaur upper stage, and even that wasn't enough. Engineers had to add a third stage, a Boeing Delta II upper stage.

File:CFT Atlas V Booster LVOS (KSC-20240221-PH-FMX01 0048).jpgNASA Kennedy Space Center / NASA/Frank Michaux, Wikimedia Commons

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Gravity Wells

To reach Pluto in 9.5 years, the spacecraft must travel extremely quickly, reaching speeds of approximately 58,500 kilometers per hour. But here's the catch: to get into orbit, operators would have to cut down that speed by over 90%.

File:PIA23922-MarsPerseveranceRover-RocketLaunch-ArtistConcept-20200617.jpgNASA/JPL-Caltech, Wikimedia Commons

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Launch Windows

The physics of interplanetary travel creates narrow launch windows that occur infrequently, and missing one means waiting years for the next opportunity. Mission planners must coordinate launch dates with planetary positions, as planets must be in the correct positions for gravity assists to be effective. 

File:Juno's Atlas V 551 at liftoff.jpgPhoto credit: NASA/Tony Gray and Tim Powers, Wikimedia Commons

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Planetary Alignment

Sometimes the universe gives you a cosmic gift, and sometimes it doesn't. The concept of the Grand Tour started in 1964, when Gary Flandro noted that an alignment of Jupiter, Saturn, Uranus, and Neptune in the 1970s would allow a single spacecraft to visit all outer planets.

File:Gary Flandro.jpgNASA/Aubrey Gemignani, Wikimedia Commons

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Planetary Alignment (Cont.)

This particular alignment occurs once every 175 years, and the next opportunity won't come until around 2151–2154. While New Horizons didn't need this complete alignment, even partial alignments for single gravity assists are rare and must be precisely timed, making mission planning a decades-long commitment.

File:Solar System true color.jpgCactiStaccingCrane, Wikimedia Commons

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Escape Velocity

Breaking free from Earth's gravitational pull is just the first hurdle in an epic journey. New Horizons was launched with a speed of about 16.26 km/s (36,400 mph). It was the fastest spacecraft to leave Earth. It passed the Moon's orbit in just nine hours.

File:New Horizons (ann21001a).jpgJ. Olmsted (STScI), Wikimedia Commons

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Escape Velocity (Cont.)

This was nearly 10 times faster than the Apollo astronauts. Even at this record-breaking speed, the spacecraft still needed additional boosts to reach Pluto in a reasonable timeframe. The energy requirements are so extreme that chemical rockets are pushed to their theoretical limits.

File:New Horizons (15771242233).jpgKevin Gill from Nashua, NH, United States, Wikimedia Commons

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Trajectory Precision

The flyby presents challenges because MU69 is so faint that no ground-based telescope has ever seen it; only Hubble has, and it's too faint for New Horizons to detect until about 100 days before the flyby. Mission planners must calculate trajectories years in advance.

File:Orbits of 2014 MU69, Pluto, Neptune, and New Horizons.pngNASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Alex Parker, Wikimedia Commons

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Jupiter Assist

Jupiter became New Horizons' cosmic stepping stone, but this celestial slingshot required split-second timing and nerves of steel. The spacecraft flew by Jupiter on Feb. 28, 2007, with the encounter increasing its velocity by 9,000 miles per hour (14,400 kilometers per hour).

File:PIA22946-Jupiter-RedSpot-JunoSpacecraft-20190212.jpgNASA/JPL-Caltech/SwRI/MSSS/Kevin M. Gill, Wikimedia Commons

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Power Requirements

When you're billions of miles from the Sun, solar panels become about as useful as an umbrella in a hurricane. Solar panels are worthless when traveling as far from the sun as New Horizons did, hence a radioisotope thermoelectric generator (RTG) is needed.

File:Multi-Mission Radioisotope Thermoelectric Generator for Curiosity.jpgKim Shiflett, Wikimedia Commons

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Solar Distance

At Pluto's distance, about 39 times farther than the Earth-Sun distance, sunlight becomes a mere whisper of its former self. The sun's rays at Pluto are too weak to generate meaningful power. This creates "extreme" conditions where spacecraft and instruments must have extraordinarily long lifetimes.

File:Solar sys.jpgHarman Smith and Laura Generosa (nee Berwin), graphic artists and contractors to NASA's Jet Propulsion Laboratory., Wikimedia Commons

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RTG Necessity

The RTG on New Horizons uses an array of thermocouples to produce electricity from the heat released by decaying plutonium, generating about 4,000 watts of thermal power at launch. Of that, only about 250 watts becomes usable electricity, with the remaining heat used to warm the spacecraft. 

File:MMRTG unloading.jpgNASA/Frankie Martin, Wikimedia Commons

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Communication Delays

When New Horizons reached Pluto, it took 4.5 hours for a one-way message to travel between Earth and the spacecraft. This communication delay means that real-time control is impossible. The spacecraft must be programmed to operate autonomously during critical phases. 

File:New Horizons over Pluto (17620333413).jpgKevin Gill from Nashua, NH, United States, Wikimedia Commons

Data Transmission

Getting data back from Pluto is like trying to download a movie through a drinking straw. The spacecraft could only transmit about 1–2 kilobits of data per second due to the enormous distance, and there were about 6.25 gigabytes of data collected during the Pluto encounter.

File:New horizons (NASA).jpgNASA, Wikimedia Commons

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Debris Hazards

The Kuiper Belt is a cosmic shooting gallery filled with potentially deadly debris. Mission planners discovered the new Pluto moons, Kerberos and Styx, during New Horizons' journey, raising concerns about debris or dust around Pluto that could potentially destroy the spacecraft at 31,000 mph. 

File:Kuiper belt diagram.pngWilyD, Wikimedia Commons

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Atmospheric Changes

Pluto's atmosphere consists mainly of nitrogen with minor amounts of methane and carbon monoxide, all vaporized from surface ices. It was thought that during aphelion, the atmosphere would largely freeze out and fall to the surface, but more elaborate models predict that Pluto maintains a significant atmosphere year-round. 

File:Pluto-01 Stern 03 Pluto Color TXT.jpgNASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute, Wikimedia Commons

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Seasonal Variations

The dwarf planet's 248-year orbit combined with its extreme axial tilt of 122.5 degrees creates seasonal changes that last decades or centuries. Pluto's last passage through perihelion was September 5, 1989, and it's currently moving away from the Sun with decreasing surface illumination.

Pluto on a black backgroundNASA, Unsplash

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Temperature Extremes

Welcome to one of the coldest neighborhoods in the solar system, where the temperature makes Antarctica seem tropical. Pluto's surface temperature ranges from -375 to -400 degrees Fahrenheit, cold enough that water behaves like a rock. At such extreme temperatures, most materials become brittle.

File:Pluto-Charon-v2-10-1-15.jpgNASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute, Wikimedia Commons

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Mission Duration

Deep-space missions can take up to 10 years from development to launch, and for New Horizons, it took close to 20 years from initial concept to actually reaching its destination. The spacecraft had to remain functional for over nine years of interplanetary cruise.

File:New Horizons 1.jpgNASA, Wikimedia Commons

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Funding Challenges

By the way, NASA effectively canceled Pluto missions at least six times between 1990 and 2005, with projected costs surpassing $1 billion by 2000. The Planetary Society organized massive postcard-writing campaigns, and advocates like Alan Stern spent nearly 20 years lobbying for funding.

File:La NASA en la Embajada (34142640202).jpgEmbajada de los Estados Unidos en Uruguay from Montevideo, Uruguay, Wikimedia Commons

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