Planets

8 CATALOGUED

A planet is a body that orbits the Sun, is massive enough that its own gravity has pulled it round, and has cleared other bodies out of its orbital path. Eight qualify, and they fall into two families: four small rocky worlds close in, and four giants of gas and ice further out. The dividing line is where the young Sun's warmth fell low enough for water to freeze, so the outer bodies had far more solid material to build from.

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THE FAMOUS ONES

] 8 ENTRIES

8 OBJECTS

[

THE SCIENCE OF PLANETS

] 3 CARDS
Rocky · rock and metal, with a surfaceGas giant · hydrogen and helium, no surfaceIce giant · water, ammonia and methane
TO SCALE WITH EACH OTHER AND WITH NOTHING ELSE · DIAMETERS FROM EACH PLANET’S OWN STORED RADIUS, IN ORBITAL ORDER · MERCURY IS 4879 KM ACROSS AGAINST JUPITER’S 139 822, A FACTOR OF 29 · EACH DISC IS DRAWN BY THE SAME CODE AS THAT PLANET’S OWN PAGE, FROM ITS STORED CLASS, DENSITY AND ALBEDO · THE GAPS BETWEEN THEM ARE NOT DISTANCES

Rock inside, gas outside

Mercury, Venus, Earth and Mars are rock and metal, small, and have few moons between them. Jupiter and Saturn are overwhelmingly hydrogen and helium; Uranus and Neptune hold more water, ammonia and methane and are usually called ice giants. None of the four giants has a surface to stand on — the atmosphere thickens continuously until it stops being a gas. The split shows in the sizes alone: the four rocky worlds together would fit inside Neptune with room to spare.

Why the orbits are nearly flat

Every planet orbits within a few degrees of the same plane and all of them go the same way round, because they condensed from one rotating disc of gas and dust about 4.6 billion years ago. Collisions in a cloud cancel out sideways motion and leave the shared spin, which is why a flattened disc is what forming systems look like wherever they are observed.

See where all eight are right now →

DISTANCE FROM THE SUN, LOGARITHMIC, FROM EACH PLANET’S OWN STORED SEMI-MAJOR AXIS · A LOG AXIS IS THE ONLY ONE THAT HOLDS ALL EIGHT, AND IT FLATTERS THE OUTER SOLAR SYSTEM: ON A LINEAR AXIS OF THIS WIDTH THE INNER FOUR WOULD SHARE THE FIRST 5 PER CENT OF IT AND THE OTHER FOUR WOULD HAVE THE REST · AND AT THE SIZE THE DISCS ABOVE ARE DRAWN — 896 KM TO THE PIXEL — NEPTUNE WOULD BE 1.3 KILOMETRES AWAY, WHICH IS WHY THE TWO FIGURES ARE TWO FIGURES

Distances nothing prepares you for

The planets are tiny against the gaps between them. On a scale where the Earth is a millimetre across, the Sun is a ten-centimetre ball twelve metres away and Neptune is a third of a kilometre out. Every diagram that shows the planets side by side is compressing that gap by a factor of thousands, which is worth remembering when one appears to sit beside another. The axis above is logarithmic for exactly that reason, and it says what a straight one would have done instead.

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COMMON QUESTIONS

] 9 ANSWERED
What counts as a planet?
Three tests, set by the IAU in 2006: it orbits the Sun, its own gravity has pulled it round, and it has cleared other bodies out of its orbital neighbourhood. Pluto passes the first two and fails the third.
Why are there two kinds?
Distance from the young Sun. Close in it was too warm for ice, so only rock and metal were available and the planets stayed small; beyond the line where water ice could survive there was far more material, and four cores grew heavy enough to hold on to hydrogen and helium.
How far apart are they really?
Much further than any diagram shows. If the Earth sat one metre from the Sun, Neptune would be thirty metres away, the Sun would be a bead nine millimetres across, and the Earth would be smaller than a grain of sand.
How were the outer ones found?
Uranus by accident in 1781, at the eyepiece. Neptune by arithmetic in 1846: Uranus was not where Newton's laws said it should be, two astronomers independently worked out where an unseen eighth planet would have to be to explain the discrepancy, and it was found within a degree of the prediction.
What is a day and a year on another planet?
A year is one trip around the Sun and a day is one turn on the axis, and the two have nothing to do with each other. Venus turns once every 243 Earth days, backwards, and completes an orbit in 225 — so its day is longer than its year.
Why is Pluto not a planet?
It meets two of the three conditions the IAU set in 2006 — it orbits the Sun and it is round — and fails the third, because it shares its region with a great many similar bodies in the Kuiper Belt. The decision followed the discovery of comparable objects out there: either Pluto was reclassified, or the count of planets became open-ended. It is a dwarf planet, which is a category rather than a demotion.
Which planet is hottest?
Venus, at about 464 °C at the surface, though Mercury is closer to the Sun. A carbon dioxide atmosphere ninety times the pressure of Earth's traps heat so effectively that Venus is hotter day and night than Mercury ever gets, and hot enough to melt lead.
Can you see planets without a telescope?
Five of them, easily: Mercury, Venus, Mars, Jupiter and Saturn have been known since antiquity for exactly that reason. They look like bright stars that do not twinkle and that move against the fixed pattern from night to night — which is what "planet" originally meant, a wanderer. Uranus is borderline under perfect conditions, and Neptune needs optics.
Is there a Planet Nine?
It is a hypothesis, not a discovery. Several distant Kuiper Belt objects have orbits that cluster in a way that would be explained by an unseen body of several Earth masses far beyond Neptune. Surveys have not found it, and the clustering may also be a selection effect in how those objects were discovered.