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Lucy

Exploring the Fossils of Planet Formation

NASA’s Lucy spacecraft performing a close flyby of a rocky asteroid, demonstrating its mission to study Jupiter Trojan asteroids and early Solar System formation.

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Attribute Details
Mission Name Lucy
Mission Type Solar System exploration mission
Operating Agency NASA
Launch Date 16 October 2021
Primary Targets Jupiter Trojan asteroids (L4 & L5 groups)
Secondary Targets Main-belt asteroid + multiple Trojan binaries
Mission Duration ~12 years (planned)
Power Source Solar arrays (largest ever used beyond Mars)
Flyby Method High-speed close encounters
First Target Flyby Asteroid 52246 Donaldjohanson (2025)
Trojan Flyby Period 2027–2033
Mission Status Active

Key Highlights

  • First mission dedicated exclusively to Jupiter Trojan asteroids
  • Explores both L4 (Greek) and L5 (Trojan) swarms
  • Visits more asteroids than any previous space mission
  • Studies objects that preserve pristine early Solar System conditions
  • Named after the fossil that revolutionized understanding of human origins

Introduction — Why the Lucy Mission Matters

The early Solar System was chaotic, crowded, and violent.
Most of the evidence from that era has been erased—melted, reprocessed, or reshaped by billions of years of planetary evolution.

The Lucy mission was designed to study what remains.

Jupiter’s Trojan asteroids are often described as time capsules—primitive bodies trapped in stable orbits since the Solar System’s infancy. By visiting them directly, Lucy aims to answer a fundamental question:

How did the planets form, and why does the Solar System look the way it does today?

What Are Jupiter Trojans?

Jupiter Trojans are asteroids that share Jupiter’s orbit around the Sun, clustered around two stable regions known as Lagrange points:

  • L4 — leading Jupiter by 60° (Greek camp)

  • L5 — trailing Jupiter by 60° (Trojan camp)

These regions are gravitationally stable, allowing objects to remain there for billions of years.

Key characteristics:

  • Highly primitive composition

  • Diverse surface colors and densities

  • Likely formed across multiple regions of the early Solar System

Lucy is the first spacecraft ever sent to explore them up close.

Mission Name — Why “Lucy”?

The mission is named after Lucy, the famous 3.2-million-year-old hominin fossil discovered in Ethiopia.

The analogy is intentional:

  • The fossil Lucy revealed human evolutionary origins

  • The spacecraft Lucy aims to reveal planetary evolutionary origins

Just as the fossil rewrote our understanding of humanity’s past, the Lucy mission is expected to reshape theories of Solar System formation.

Mission Architecture — A Grand Tour Without Orbiting

Lucy is not an orbiter.
Instead, it performs a complex sequence of gravity assists and flybys, allowing it to visit many targets efficiently.

Key design features:

  • Multiple Earth gravity assists

  • Repeated crossings of the asteroid belt

  • High-speed encounters optimized for imaging and spectroscopy

  • A trajectory spanning billions of kilometers

This makes Lucy one of the most dynamically ambitious missions ever flown.

Lucy’s Target List — A Diverse Family of Asteroids

Lucy’s targets were chosen to represent the full diversity of Trojan populations.

Planned encounters include:

  • 3548 Eurybates (binary system)

  • 15094 Polymele

  • 11351 Leucus

  • 21900 Orus

  • 617 Patroclus–Menoetius (equal-mass binary)

Each target offers clues about:

  • Composition differences

  • Collisional history

  • Internal structure

  • Formation environment

Together, they form a comparative dataset unmatched in asteroid science.

Scientific Goals of the Lucy Mission

Lucy’s core objectives include:

  • Determining Trojan surface compositions

  • Measuring mass and density

  • Studying cratering and geology

  • Investigating binary asteroid formation

  • Testing models of planetary migration

These goals directly address leading theories such as the Nice Model, which proposes that the giant planets migrated early in Solar System history.

Why Trojans Hold the Key to Planetary Migration

Modern models suggest that:

  • Jupiter did not form where it currently orbits

  • Giant planets moved significantly during early epochs

  • Small bodies were scattered and captured during this migration

Jupiter Trojans may be:

  • Captured remnants from multiple regions

  • Survivors of planetary reshuffling

  • Direct evidence of early gravitational chaos

Lucy’s observations will either validate or challenge these ideas.

Engineering Challenge — Solar Power Near Jupiter

Operating near Jupiter presents a major challenge: low sunlight.

Lucy solves this by using:

  • Two massive circular solar arrays

  • Ultra-efficient power management

  • Lightweight composite materials

These arrays are the largest solar panels ever flown for a deep-space mission, proving solar power is viable far beyond Mars.

Why Lucy Is a Landmark Mission

Lucy is important because it:

  • Explores a completely unvisited population

  • Links asteroid science with planet formation theory

  • Tests long-standing migration models

  • Expands deep-space solar-powered exploration

  • Creates a new framework for comparative asteroid studies

It is not just a mission to asteroids—it is a mission to the Solar System’s memory.

Lucy’s Scientific Payload — Seeing, Measuring, Understanding

Lucy carries a focused but powerful suite of instruments designed for fast, high-precision flybys. Every instrument is optimized to extract maximum science in the short encounter windows.

L’LORRI — High-Resolution Imaging System

  • Narrow-angle visible-light camera

  • Derived from New Horizons’ LORRI

  • Resolves surface features, craters, and boulders

  • Tracks rotation, shape, and geology

L’LORRI provides the detailed imagery needed to interpret each asteroid’s surface history.


L’Ralph — Color and Composition Mapper

L’Ralph combines two instruments:

  • MVIC (Multispectral Visible Imaging Camera)

  • LEISA (Infrared imaging spectrometer)

Together, they:

  • Map surface colors and compositional variations

  • Detect ices, organics, and minerals

  • Identify space-weathering effects

This instrument is central to solving the Trojan color diversity mystery.


L’TES — Thermal Emission Spectrometer

  • Measures surface temperature

  • Determines thermal inertia

  • Constrains grain size and regolith properties

Thermal data helps reveal whether Trojans are fluffy rubble piles or compact bodies.

Binary Trojans — A Unique Scientific Opportunity

One of Lucy’s most important targets is 617 Patroclus–Menoetius, a rare equal-mass binary system.

Why Binary Systems Matter

Binary Trojans allow scientists to:

  • Measure mass directly through orbital motion

  • Calculate bulk density accurately

  • Infer internal structure

Patroclus–Menoetius is thought to be:

  • Extremely low density

  • Possibly ice-rich

  • Formed gently, not by violent collision

This supports formation in the cold outer Solar System.

The Trojan Color Mystery

Jupiter Trojans fall into two broad color groups:

  • Red Trojans

  • Less-red (neutral) Trojans

Key questions Lucy addresses:

  • Are these groups compositionally different?

  • Did they form in different regions of the Solar System?

  • Are surface colors primordial or altered by space weathering?

Lucy’s multi-target design allows direct comparison under identical instrumentation—something telescopes alone cannot achieve.

Lucy and the Nice Model — Putting Theory to the Test

The Nice Model predicts that:

  • Jupiter migrated inward and outward

  • Small bodies were scattered across the Solar System

  • Some were captured at Lagrange points

Lucy tests this by checking whether:

  • Trojan compositions are diverse

  • Binary systems survived gentle capture

  • Objects resemble Kuiper Belt bodies

If Trojans show mixed origins, it strongly supports large-scale planetary migration.

Comparison with Other Asteroid Missions

Lucy complements, rather than duplicates, other missions.

Mission Primary Focus Key Difference
NEAR Shoemaker Single asteroid Orbital study
OSIRIS-REx Carbonaceous NEO Sample return
Hayabusa2 Rubble-pile asteroid Sample return
Psyche Metal-rich asteroid Unique composition
Lucy Trojan population Multi-target flybys

Lucy’s strength lies in comparative diversity, not prolonged study of a single body.

Encounter Strategy — High Speed, High Precision

Lucy flybys occur at velocities up to 9 km/s.

This requires:

  • Extremely accurate navigation

  • Pre-planned imaging sequences

  • Autonomous pointing corrections

Despite brief encounters, Lucy can collect:

  • Global shape models

  • Detailed regional imagery

  • Complete spectral datasets

The mission proves that flyby science, when done correctly, can rival orbital missions in impact.

Trojan Geology — What Lucy Is Looking For

Key surface features of interest include:

  • Crater populations and ages

  • Fractures and ridges

  • Boulder distributions

  • Surface layering

These features help reconstruct:

  • Collisional history

  • Internal strength

  • Thermal evolution

Even subtle geological differences between Trojans can reveal vastly different origins.

Why Lucy Is Scientifically Risky — and Powerful

Lucy is bold because:

  • Trojans are faint and distant

  • Targets are poorly characterized

  • Flybys offer no second chances

But this risk is precisely why the mission is transformative. Lucy explores a population that has remained untouched because it is difficult, not because it is unimportant.

Lucy’s Role in Planetary Science

Lucy sits at the intersection of:

  • Asteroid science

  • Planetary migration theory

  • Solar System origin studies

Its findings will influence:

  • Models of giant planet formation

  • Interpretation of exoplanet systems

  • Future mission planning

Lucy does not just study asteroids—it studies how planetary systems assemble.

Lucy’s Long Trajectory — A Mission Measured in Decades

Lucy’s flight path is one of the most intricate ever designed for a planetary mission.

Rather than heading directly to Jupiter, Lucy follows a looping, energy-efficient route shaped by gravity assists.

Key milestones:

  • 2021 — Launch from Earth

  • 2022–2025 — Earth gravity assists and asteroid belt crossing

  • 2025 — Flyby of main-belt asteroid 52246 Donaldjohanson

  • 2027–2028 — First encounters with L4 (Greek camp) Trojans

  • 2031–2033 — Encounters with L5 (Trojan camp), including Patroclus–Menoetius

This trajectory allows Lucy to visit both Trojan swarms—something no other mission has ever attempted.

What Success Looks Like for the Lucy Mission

Lucy’s success is not defined by a single discovery, but by the pattern that emerges across many targets.

The mission will be considered transformative if it can:

  • Demonstrate compositional diversity among Trojans

  • Confirm whether Trojans formed in multiple Solar System regions

  • Accurately measure densities and internal structures

  • Link Trojan properties to planetary migration models

Even null results—such as unexpected uniformity—would be scientifically powerful, forcing a reevaluation of long-standing theories.

Will Lucy Answer All Questions?

No—and that is by design.

Lucy is a pathfinder mission. Its role is to:

  • Identify trends

  • Expose anomalies

  • Highlight new questions

Its findings will likely inspire:

  • Follow-up orbiters

  • Sample-return mission concepts

  • Expanded Trojan surveys

Lucy opens the door—it does not close the book.

Frequently Asked Questions (FAQ)

Why hasn’t anyone visited Jupiter Trojans before?

They are distant, faint, and widely spread, making missions technically challenging and costly.

Does Lucy orbit any asteroid?

No. All encounters are high-speed flybys.

Why use solar power so far from the Sun?

Advances in solar panel efficiency make it lighter and more reliable than nuclear alternatives for this mission class.

Is Lucy related to the Lucy fossil directly?

Only symbolically. Both represent discoveries about origins—biological and planetary.

Could Trojans contain ice?

Yes. Density and spectral data suggest some may be ice-rich beneath a dusty surface.

Lucy’s Broader Impact on Planetary Science

Lucy’s influence extends beyond Jupiter.

Its results will affect:

  • Models of early Solar System instability

  • Interpretation of Kuiper Belt objects

  • Understanding of exoplanetary debris disks

  • Future deep-space mission design

By studying stable small bodies, Lucy helps explain why planetary systems do not self-destruct during formation.

Lucy in the Universe Map Context

Within Universe Map, Lucy connects naturally to:

  • Jupiter Trojans

  • Lagrange points (L4 and L5)

  • Planetary migration models

  • The Nice Model

  • Oort Cloud and Kuiper Belt comparisons

Together, these topics reveal the architecture behind planetary order.

Final Perspective

Lucy is a mission about memory.

The Jupiter Trojans are not random debris—they are survivors from the Solar System’s most turbulent epoch. By visiting them, Lucy reads a record written before planets finished forming.

Just as the fossil Lucy changed how we understand human origins, the Lucy spacecraft may change how we understand planetary origins—showing that stability often hides a violent past.