Image copyright ESA/ROSETTA/NAVCAM Image caption The new report answers one of the big questions of the Rosetta mission

The rubber duck-shaped comet being followed by Europe's Rosetta probe used to be two separate objects.

Scientists say pictures of 67P show its two lobes to have "onion skin" layers that intersect in a way that can only be the result of two different bodies having collided and stuck together.

Ever since Rosetta arrived at the comet, the origin of its bizarre form has been one of the major puzzles.

The solution is now due to be published in the journal Nature.

Mission team members have also held a media conference to give further details, at the European Planetary Science Congress in Nantes, France.

Rosetta first spied the duck shape on approach to 67P/Churyumov-Gerasimenko in July 2014.

The idea that it was a "contact binary" - two conjoined comets - was a popular explanation from the word go.

But proving it has not been straightforward. An alternative possibility is simply that the icy dirt ball has been sculpted this way.

Every time it comes around the Sun, 67P's ices warm and it throws off gas and dust, and it could have been that this process has dominated in just one region to produce the distinctive appearance.

The Osiris camera on Rosetta can now settle the debate.

It reveals layers up to 650m thick in the body of the duck that are independent of similar strata detected in its head.

Image copyright ESA/ROSETTA/MPS FOR OSIRIS TEAM Image caption The deep pit at bottom-right shows the internal layering on the duck's body

Additional measurements taken by Rosetta of variations in the local tug of gravity across the lobes also support this two-body origin.

The direction of the tugging is more closely aligned with the independent layering than with a centre of mass associated with a single object.

Union of onions

Scientists say that to collide and stick together, the impact must have been a very low velocity one - perhaps just a few metres per second. Any faster and the primary objects would have done enormous damage to each other.

"I would say it's a quite beautiful love story," Matteo Massironi, from the Osiris team, said at Monday's press briefing.

He added that a key piece of evidence was a series of cross-sections of the comet, which the team were able to construct by extending the layers glimpsed on the surface into a 3D model of 67P's interior. These cross-sections painted a clear picture of two distinct sets of layers, reminiscent of a pair of onions.

"You don't know the structure of an onion until you cut across it," Dr Massironi said. "What we have seen is that this stratification is really continuous - and that [the one in the tail] doesn't match that of the head."

The discovery's consequences for what we understand about comet formation could be quite profound, says team member Stephen Lowry from Kent University, UK.

"It shows that comets were forming into large sizes and that they were then still colliding in this grown form to make even larger comets. So, it's not simply a case of independent comets completely forming out of centimetre- or metre-sized planetesimals, to make the comets we see today. And that's really quite fascinating, because it could be quite a ubiquitous process."

Image copyright ESA/ROSETTA/MPS FOR OSIRIS TEAM Image caption The local gravity field supports the idea that 67P was once two separate objects rather than a single formation

Other comets seen at relatively close quarters also display lobed shapes, including comets Halley, Borrelly and Hartley-2. Could they also be the result of low-velocity bump-and-stick events?

The tantalising prospect now is whether what was once two objects could split into two again. Could the constant erosion of gas and dust result in the duck losing its head? And will Rosetta be on hand to witness it?

The European Space Agency (Esa) probe has pictured a crack in the neck region of 67P, says Dr Lowry.

"If a comet is going to split, it's most likely to break along the interface between the two lobes. But I haven't seen any evidence yet that the crack is getting longer or wider. That's a strong indicator to me that perhaps 67P won't split on this orbit of the Sun."

Image copyright NASA Image caption Comets Borrelly and Hartley-2 have lobed shapes. Were they also made in low velocity collisions between objects

The comet takes just over six years to orbit the Sun and the Rosetta mission, after receiving a 10-month extension, will nonetheless end in September 2016.

At that point the spacecraft will spiral gradually closer and land yet again on 67P, said Esa project scientist Matt Taylor at the press conference - making a reference to the Philae lander's bumpy touchdown in November 2014.

He added that although the comet had passed its "perihelion" (its closest approach to the Sun), the mission was really only just beginning. "The papers are starting to flow."

Comet 67P - "Space duck" in numbers

A full rotation of the body takes just over 12.4 hours

The axis of rotation runs through the "neck" region

Its larger lobe ("body") is about 4.1 × 3.3 × 1.8 km

The smaller lobe ("head") is about 2.6 × 2.3 × 1.8 km

Gravity measurements give a mass of 10 billion tonnes

Mapping estimates the volume to be about 21.4 cubic km

The density works out at about 470kg per cubic metre

This would imply that Comet 67P is highly porous

It is 70-80% empty space, but are there big voids inside?

Daytime surface temperatures range from -93C to -43C

Amount of incident light reflected (albedo) is just 6%

Jonathan.Amos-INTERNET@bbc.co.uk and follow me on Twitter: @BBCAmos