Comets

4076 TRACKED

A comet is a body of ice, dust and rock on an orbit that carries it close to the Sun and then far away again. For most of its orbit it is a dark, inert nucleus a few kilometres across; approaching the Sun, the ice turns straight to gas and drags out the coma and the tails that make it visible. They are among the least altered material in the Solar System, which is why so much effort goes into reaching them.

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THE FAMOUS ONES

] 8 ENTRIES
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THE SCIENCE OF COMETS

] 3 CARDS
THE SUNBOTH TAILS POINT ALONG THIS LINE, AWAY FROM THE SUNDIRECTION OF TRAVEL →
a few kilometres of ice and dust
gas and dust off the nucleus, larger than a planet
straight, swept back by the solar wind
curved, each grain on its own orbit
NOT TO SCALE, AND IT CANNOT BE · WITH THE COMA DRAWN AT A TYPICAL 100 THOUSAND KM ACROSS, THE 68.5 KM-RADIUS NUCLEUS THIS CATALOGUE HOLDS FOR C/2014 UN271 (BERNARDINELLI-BERNSTEIN) WOULD BE AN EIGHTIETH OF THE DOT DRAWN HERE · THAT COMET COMES WITHIN 11 AU OF THE SUN ON AN ORBIT OF ECCENTRICITY 0.999 · THE ONE THING DRAWN TRUE IS THE GEOMETRY: THE ION TAIL LIES ON THE LINE FROM THE SUN THROUGH THE NUCLEUS WHICHEVER WAY THE COMET IS MOVING, AND THE DUST FALLS BEHIND IT

Anatomy

The nucleus is the solid part — typically a few kilometres of ice and dust, and very dark. The coma is the cloud of gas and dust released from it, which can grow larger than a planet. There are usually two tails: a dust tail that curves along the orbit, and a straight bluish ion tail of charged gas swept back by the solar wind. Only the nucleus is permanent; everything else in a picture of a comet is material leaving it for good.

Why the tail points away from the Sun

It is not trailing behind the motion like smoke. Radiation pressure and the solar wind push the released material directly away from the Sun, so the tail lies on the anti-solar side regardless of which way the comet is going. An outbound comet therefore flies tail-first. The ion tails held a further clue: they lie a few degrees off the anti-solar line, tipped by the comet's own motion, and in 1951 Ludwig Biermann showed that sunlight alone could not do that — the Sun had to be streaming charged particles outward. The solar wind was found in comet tails a decade before a spacecraft could measure it directly.

927 orbits · back inside about 20 years · from a disc beyond Neptune
Halley-type133 orbits · back in 20 to 200 years · steeper, and some of them backwards
1710 orbits · one pass in recorded history · from a shell around everything
Sungrazers1306 orbits · one comet that broke up, counted a thousand times
0°45°90°135°180°
HOW FAR EACH COMET’S ORBIT IS TILTED OUT OF THE PLANE THE PLANETS ORBIT IN, IN TEN-DEGREE BINS, FROM THIS CATALOGUE’S OWN ELEMENTS · EACH ROW IS SCALED TO ITS OWN TALLEST BIN, BECAUSE THE FAMILIES DIFFER IN SIZE BY MORE THAN TEN TO ONE AND THE SHAPE IS WHAT IS BEING COMPARED · PAST 90° THE COMET GOES ROUND THE SUN BACKWARDS · THE SHORT-PERIOD COMETS HUG THE PLANE BECAUSE THEY COME FROM A DISC; THE LONG-PERIOD ONES ARRIVE AT EVERY ANGLE BECAUSE THEY FALL FROM A SHELL · THE DISC IS SEEN ONLY IN ITS LARGEST MEMBERS AND THE SHELL NOT AT ALL, SO THESE TILTS ARE MOST OF THE EVIDENCE FOR BOTH · THE SUNGRAZERS ARE ON THEIR OWN ROW BECAUSE THEY ARE ONE OBJECT’S DEBRIS AND WOULD OTHERWISE READ AS A DIRECTION THE SHELL PREFERS

Two reservoirs

Short-period comets, which return in under about 200 years, come mostly from the Kuiper Belt and its scattered disc beyond Neptune, and orbit near the plane of the planets. Long-period comets arrive from the Oort Cloud, a roughly spherical shell reaching perhaps a quarter of the way to the nearest star, and can come in from any direction at all. A comet's orbit is therefore evidence about where it has been stored. The Kuiper Belt is seen directly only in its largest members — a comet-sized body there is far too faint to detect — and the Oort Cloud has never been observed at all, so the tilts of these orbits are most of the case for both.

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COMMON QUESTIONS

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What happens when one approaches the Sun?
The ice begins turning straight to gas and drags dust out with it. The nucleus grows a coma — a temporary atmosphere that can be wider than the Sun — and behind that the tails. Far from the Sun there is nothing to see but a dark few kilometres of ice.
How long is a comet's orbit?
From a few years to millions, and for some there is no answer at all. Short-period comets come from the Kuiper belt beyond Neptune and return within about two centuries; the long-period ones fall in from the Oort cloud, and one of their orbits can take millions of years. A few hundred here are on paths that never close, most of them the Sun's own comets flung outward by a close pass with a planet — and two that were never the Sun's to begin with. The third interstellar visitor found so far, 1I/'Oumuamua, passed through without ever growing a coma, so it is filed with the asteroids.
How bright will a new comet get?
Almost nobody can say in advance. Brightness depends on how much volatile material is left near the surface, which cannot be measured from Earth, so predictions made a year out have been wrong by several magnitudes in both directions.
Where do meteor showers come from?
Almost always from comets. A comet leaves a stream of dust along its orbit, and when the Earth crosses that stream the grains burn up in the atmosphere. The Perseids come from Swift-Tuttle; the Orionids and the Eta Aquariids are both Halley. The December Geminids are the exception: their parent, Phaethon, is catalogued as an asteroid — either a dead comet or a rock that sheds dust when the Sun bakes it.
What is a comet made of?
Water ice mostly, with carbon monoxide and dioxide, ammonia and methane, a great deal of dust, and complex organic molecules. Rosetta found that the water on comet 67P carries a different deuterium ratio from the Earth's oceans, which argues that comets did not deliver most of our water.
How often is a comet visible without a telescope?
Roughly one a decade becomes genuinely striking, though several a year are within reach of binoculars. Predicting brightness is notoriously unreliable, because it depends on how much ice a particular nucleus still has and how it behaves when heated — comets have both fizzled and outperformed forecasts by large factors.
What is the difference between a comet and an asteroid?
Composition and behaviour rather than a hard line. A comet holds enough volatile ice to produce a coma when heated; an asteroid does not. The boundary is genuinely blurred — some objects have been reclassified after unexpectedly growing a tail, and some comets appear to have exhausted their ice and now look like asteroids.
When does Halley's Comet come back?
In 2061. It has a period of about 76 years and last passed close to the Sun in 1986; it is currently beyond Neptune's distance and heading back in. Its returns have been recorded for more than two thousand years, and it was the first comet shown to be a repeat visitor rather than a one-off.
Do comets run out?
Yes. Every close pass strips away some of the ice, so a short-period comet has a limited number of returns before it goes dormant or breaks up. Several have been observed disintegrating. The debris streams they leave behind are what the Earth runs through each year as a meteor shower.