Planets
Search out every planet and the features that make each one different.
Find these words
- neptune
- satellite
- giant
- ring system
- distant
- frozen
- terrestrial
- gaseous
- windy
- habitable zone
- molten
- dwarf planet
- rocky
- spin
- magnetic field
- cloudy
Nicely done.
You found these. Now read about them
More science word searches
Sixteen words for eight very different worlds
No two planets in this solar system are built the same way. Some are rock and metal small enough to walk across in a few years; others are gas so deep that “surface” barely means anything. This puzzle’s vocabulary is about comparing those worlds directly, in size, composition and distance from the sun.
What the words mean
The two planet families
Terrestrial planets are the four closest to the sun, Mercury, Venus, Earth and Mars, and they share a solid, rocky surface built mostly from metal and silicate rock. Gas giants are the four beyond them, Jupiter, Saturn, Uranus and Neptune, built mostly from hydrogen and helium with no solid surface to land on at all. The split is not just size; it is composition, and it lines up almost exactly with distance from the sun, since the early solar system was too hot near the sun for light gases to stick around, leaving only rock and metal behind to form planets there.
Size and scale
The size range across the eight planets is enormous. Jupiter alone contains more mass than all the other planets combined, while Mercury is barely larger than Earth’s moon. This rundown of the eight planets puts the numbers side by side, diameter, mass and distance from the sun, which makes the family resemblance within each group, terrestrial or gas giant, much easier to see than it is from pictures alone.
Moons
Moons are natural satellites, bodies that orbit a planet rather than the sun directly, and they are distributed very unevenly. Mercury and Venus have none at all. Mars has two small, irregularly shaped ones, likely captured asteroids rather than moons that formed alongside the planet. The gas giants, by contrast, each carry dozens, including Jupiter’s Europa and Saturn’s Titan, moons large and interesting enough that some are studied as places life might exist elsewhere in the solar system.
Comparing across the family
These examples of planets lay out defining features for all eight in one place, useful for spotting a pattern the definitions above only hint at: temperature does not fall in a straight line with distance from the sun. Venus, the second planet out, is hotter than Mercury, the closest one, because a thick carbon dioxide atmosphere traps heat far more effectively than Mercury’s almost nonexistent one does. Surface gravity follows its own separate pattern too: it depends on both mass and diameter together, which is why Saturn, despite being the second most massive planet, has surface gravity barely stronger than Earth’s, spread as it is across a far larger sphere.
Using this in a classroom
The three sheets carry the same sixteen words in different grids, which works well for a first attempt in class and a retest or homework version later. The puzzle and the answer key print on separate pages, so the key does not have to go out with the puzzle. This set fits grades 3 through 7, roughly the range where students first learn the planets individually rather than just in order. A useful extension: after solving, have students sort the sixteen words into “terrestrial” and “gas giant” columns, then justify any word that does not obviously belong to a planet at all.
For a shorter daily warm-up, the science word search hub offers a new sixteen-word grid on a different science topic each day.
Where “planet” stops meaning what it used to
Pluto is the classic case, but the more useful mix-up to teach is the boundary between a planet and something that only resembles one. The difference between a dwarf planet and a planet comes down to one rule: a full planet has cleared other debris out of its orbital path through its own gravity, and a dwarf planet has not, no matter how round or massive it otherwise is. At the other end of the size scale, a brown dwarf gets confused with a giant planet for the opposite reason: it is far more massive than any planet, sitting in a gap between the largest gas giants and the smallest true stars, massive enough to fuse a little deuterium but not enough to sustain the hydrogen fusion that makes something a star. Knowing both boundaries, planet versus dwarf planet at the small end and planet versus brown dwarf at the large end, is what separates a real definition of “planet” from a rough sense of what one looks like.