Keep your eyes on the heavens at the turn of the year, say astronomers - you might spot streaking Quadrantids.

The meteor shower has lit up the early January skies since at least 1825. Now astronomer Peter Jenniskens of the SETI Institute in Mountain View, California, may have tracked down the source of the shooting stars.

The Quadrantids could be debris from a celestial body called 2003 EH1, Jenniskens says. 2003 EH1, which was discovered in March, was previously thought to be an asteroid on an orbit that brings it close to Earth.

Jennisken believes that 2003 EH1 may in fact be a washed-up comet1. It broke up about 500 years ago, he suggests, releasing a scattering of dusty grains that hit Earth's atmosphere and burn up to create the Quadrantids' light-show.

Most other meteor showers, such as the November Leonids, are also sparked when Earth periodically passes through a comet's dusty debris. The dust trail is replenished each time it returns to the inner solar system, and so the annual meteor showers become more spectacular.

Light show

The Quadrantids, which are generally rather faint, seem to emanate from the constellation of Boötes, close to the Big Dipper. The best view is obtained in the Northern Hemisphere from about 11 pm GMT. The show is typically at its most spectacular around 2-4 January.

Astronomers have long known that these meteors originated from some 'parent body', but were unable to agree on what it was. By looking at the meteor trajectories, Jenniskens calculated the orbit that this parent body would now be following and found that it closely fits the path of 2003 EH1.

Astronomers suspect that 2003 EH1 may itself be the remnant of a larger parent comet called C1490 Y1. In 1979, Japanese astronomer Ishiro Hasegawa discovered that the path of the Quadrantids seemed to be similar to that of C1490 Y1, which is mentioned in East Asian historical records from around 1490 and broke up roughly a century later.

Jenniskens teamed up with Brian Marsden of the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, to see whether they could match the predicted orbit of EH1 to that of C1490 Y1 at around the time that it broke up. This is tricky, because the orbits of C1490 Y1 and 2003 EH1 could have been shifted by close flybys of Earth or Jupiter.

The researchers conclude that 2003 EH1 might be the ancient core of C1490 Y1 - but the evidence is scant. They need better observations of the path currently followed by 2003 EH1. But if the once-obscure 2003 EH1 does turn out to be the heart of an extinct comet, it would make an enticing target for future space missions.