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Mr. Brown's Science Labs
Earth & Space Science · Astronomy Unit · Lab 07

What happened to Pluto?

In 2006, astronomers stripped Pluto of its title. Was it the right call? You decide.

35 Minutes 21 Points ESRT Page 15 Regents Aligned

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pluto · dwarf-planet · IAU · planet-definition · Mr-Brown-science-labs · Earth-Space-Regents · ESRT-page-15 · astronomy
vocabulary · planet · dwarf-planet · IAU · Kuiper-Belt · hydrostatic-equilibrium · asteroid-belt · 8-second-timer
Step One

Vocabulary cards

Tap a card to flip it. Each card stays open for 8 seconds. You may reopen any card as often as you like.

Practice — Match each term to its definition

Tap a term, then tap the matching definition. Correct pairs lock in green.

Terms

Definitions

reading-one · Clyde-Tombaugh · 1930-discovery · Lowell-Observatory · Planet-X · sentence-stem · hochman
Step Two · Reading One

The story so far

Clyde's Ninth Planet

On a cold winter night, a 24-year-old Kansas farmer named Clyde Tombaugh discovered a new world. Working at the Lowell Observatory, he had been comparing photographic plates of the night sky, hunting for a "Planet X" that astronomers believed was tugging on Neptune's orbit. After months of patient searching, he found a small dot that shifted between two photographs taken six days apart.

The new world was named Pluto, after the Roman god of the underworld. For 76 years, every textbook taught that our solar system had nine planets. Pluto was the smallest, the coldest, and the most distant — a tiny icy world taking 248 Earth years to orbit the Sun once.

But Pluto was always strange. Its orbit is tilted at 17 degrees from the path of the other planets. It is so eccentric that for 20 years of every orbit, Pluto is actually closer to the Sun than Neptune. And it is unbelievably tiny — smaller, in fact, than Earth's own Moon. By the 1990s, astronomers were beginning to whisper a question nobody wanted to ask: was Pluto really a planet at all?

Question 1 · 1 pt

Pluto was discovered in 1930 because

Question 2 · 1 pt

Pluto's orbit is unusual, but

reading-two · Eris-Mike-Brown · IAU-Prague-2006 · three-rules-of-planethood · sentence-scrambler · sentence-expansion
Step Three · Reading Two

The vote that demoted Pluto

Eris Changes Everything

In 2005, astronomer Mike Brown and his team at Caltech announced the discovery of a new world far beyond Pluto. They named it Eris, after the Greek goddess of discord — and discord is exactly what it caused. Early measurements suggested Eris was even larger than Pluto.

Suddenly astronomers had a problem. If Pluto was a planet, then Eris had to be the tenth. And what about all the other large icy objects being found in a region called the Kuiper Belt? Were there going to be twenty planets? Fifty?

In August 2006, the International Astronomical Union met in Prague and voted on a new definition. To be a planet, an object must do three things: orbit the Sun, be massive enough that its own gravity pulls it into a round shape, and have "cleared the neighborhood" around its orbit. Pluto passes the first two tests. But it shares its space with thousands of Kuiper Belt objects, so it fails the third. By a show of hands, Pluto was reclassified as a dwarf planet. Mike Brown himself wrote a book titled How I Killed Pluto and Why It Had It Coming.

Question 3 · 1 pt

Pluto failed the third rule, so

Question 4 · 1 pt · Unscramble the sentence

Tap a word in the bank, then tap a numbered slot to place it. Correctly placed words turn green.

Question 5 · 1 pt · Unscramble the sentence
Question 6 · 1 pt · Sentence Expansion

Astronomers studied Pluto.

Rewrite the sentence so it answers all three prompts:

When / WhereWhyHow
simulation · animated-orbit · Kuiper-Belt · cleared-neighborhood · Pluto-vs-Earth · interactive · canvas-animation
Step Five · Watch the Rule in Action

Did Pluto clear its neighborhood?

This simulation shows Pluto orbiting the Sun inside the Kuiper Belt — a region packed with thousands of icy objects. Use the toggle to compare it to Earth's "clean" orbital path.

Tracking: Pluto
Sun Pluto Neptune Kuiper Belt Objects (60+)
Question 7 · 1 pt

After watching the simulation, I can see Pluto failed the third rule of planethood because

data-table · ESRT-page-15 · Solar-System-Data · classification · 4-points · Eris-Pluto-Earth-Jupiter-Moon
Step Five · Data Analysis

Six worlds, three classifications

Before you classify, look at the worlds you are about to compare. Each body is drawn to scale relative to the others. The Sun is not to scale — it would be hundreds of times wider than Jupiter.

SUN · NOT TO SCALE Mercury 4,879 km Earth + Moon 12,756 km · 3,476 km Jupiter 142,984 km Pluto 2,376 km Eris 2,326 km OBJECTS TO SCALE · 1 PX ≈ 953 KM

Find the dashed rings — that's where Pluto, Eris, and the Moon are. They really are that small.

ESRT — page 15 · Solar System Data. The eight planets and their orbital characteristics are listed there. Pluto and Eris are not on the ESRT — that's the lesson.
Scale Drawing · Each Body Proportional to the Others
SUN · NOT TO SCALE Mercury · 4,879 km Moon · 3,476 km Earth · 12,756 km Jupiter · 142,984 km Pluto · 2,376 km Eris · 2,326 km 20,000 km
Body diameters are drawn to scale relative to each other (1 px ≈ 1,430 km). Sun and orbital distances are not to scale. Notice how tiny Pluto and Eris are compared to even Earth's Moon.
Object Diameter (km) Mass (×10²² kg) Distance from Sun (AU) Orbital Eccentricity Classification
Mercury 4,879 33 0.39 0.206 PLANET (example)
Earth 12,756 597 1.00 0.017
Jupiter 142,984 189,800 5.20 0.048
Earth's Moon 3,476 7.35 — (orbits Earth)
Pluto 2,376 1.30 39.48 0.244
Eris 2,326 1.66 67.78 0.441
Worth 4 points · Click "Check" when finished
bar-graph · mass-comparison · Earth-Pluto-Eris-Moon · log-scale · graph-interpretation
Step Five · Visualize the Data

How big is Pluto, really?

The graph below shows the mass of four solar system bodies. Because Earth is so much more massive than the others, the y-axis uses a logarithmic scale — each step is ten times bigger than the one below it.

10²¹ 10²² 10²³ 10²⁴ 10²⁵ Mass (kilograms) 1.30×10²² Pluto 1.66×10²² Eris 7.35×10²² Earth's Moon 5.97×10²⁴ Earth LOG SCALE · EACH GRIDLINE = ×10
Mass of four solar system bodies (kg)
Graph Question 1 · 1 pt

Based on the bar graph, which statement is best supported?

Graph Question 2 · 1 pt

Approximately how many times more massive is Earth than Pluto?

sorter · drag-drop · classification · Ceres-Haumea-Makemake-Vesta-Europa · IAU-three-rules
Step Six · Apply the Rules

Sort the solar system

Tap an object in the word bank to select it (it will turn red), then tap the category zone where it belongs. Tap a placed object to send it back to the bank.

Planet
Dwarf Planet
Asteroid
Moon
Worth 2 points · all 10 must be placed
regents-style · multiple-choice · ESRT-lookup · IAU-criteria · 6-questions-from-bank-of-12 · exam-prep
Step Seven · Regents-Style Questions

Six questions, one point each

Style mimics the NYS Earth & Space Science Regents (Jan 2026, June 2025). Use ESRT page 15 where helpful.

final-grade · score-breakdown · print-to-PDF · letter-grade · Mr-Brown-science-labs
Lab Complete

Your final grade

— / 20 points

Below you can print the entire lab to PDF — including your readings, data table, graph, and every answer you submitted.