Over the last 15 years, astronomers¹ have detected nearly 500 planets orbiting stars in our cosmic neighbourhood, but none outside our Milky² Way has been confirmed. Now, however, a planet with a minimum mass 1.25 times that of Jupiter has been discovered orbiting a star of extragalactic（银河系外的） origin, even though the star now finds itself within our own galaxy³. It is part of the so-called Helmi stream — a group of stars that originally belonged to a dwarf⁴ galaxy that was devoured⁵ by our galaxy, the Milky Way, in an act of galactic cannibalism⁶（吞食，同类相食） about six to nine billion years ago. The results are published today in Science Express. "This discovery is very exciting," says Rainer Klement of the Max-Planck-Institut für Astronomie (MPIA), who was responsible for the selection of the target stars for this study. "For the first time, astronomers have detected a planetary system in a stellar stream of extragalactic origin. Because of the great distances involved, there are no confirmed detections of planets in other galaxies⁷. But this cosmic merger⁸ has brought an extragalactic planet within our reach."

The star is known as HIP⁹ 13044, and it lies about 2000 light-years from Earth in the southern constellation¹⁰（星座） of Fornax (the Furnace). The astronomers detected the planet, called HIP 13044 b, by looking for the tiny telltale（迹象） wobbles of the star caused by the gravitational tug¹¹ of an orbiting companion. For these precise observations, the team used the high-resolution spectrograph FEROS attached to the 2.2-metre MPG/ESO telescope at ESO's La Silla Observatory¹² in Chile.

Adding to its claim to fame, HIP 13044 b is also one of the few exoplanets（外部行星） known to have survived the period when its host star expanded massively after exhausting the hydrogen fuel supply in its core — the red giant phase of stellar evolution. The star has now contracted again and is burning helium in its core. Until now, these so-called horizontal branch stars have remained largely uncharted territory for planet-hunters.

"This discovery is part of a study where we are systematically¹³ searching for exoplanets that orbit stars nearing the end of their lives," says Johny Setiawan, also from MPIA, who led the research. "This discovery is particularly intriguing¹⁴（有趣的，迷人的） when we consider the distant future of our own planetary system, as the Sun is also expected to become a red giant in about five billion years."

HIP 13044 b is near to its host star. At the closest point in its elliptical（椭圆的） orbit, it is less than one stellar diameter from the surface of the star (or 0.055 times the Sun-Earth distance). It completes an orbit in only 16.2 days. Setiawan and his colleagues hypothesise that the planet's orbit might initially¹⁵ have been much larger, but that it moved inwards during the red giant phase.

Any closer-in planets may not have been so lucky. "The star is rotating relatively¹⁶ quickly for an horizontal branch star," says Setiawan. "One explanation is that HIP 13044 swallowed its inner planets during the red giant phase, which would make the star spin more quickly."

Although HIP 13044 b has escaped the fate of these inner planets so far, the star will expand again in the next stage of its evolution. HIP 13044 b may therefore be about to be engulfed¹⁷ by the star, meaning that it is doomed¹⁸ after all. This could also foretell¹⁹ the demise²⁰（死亡，终止） of our outer planets — such as Jupiter — when the Sun approaches the end of its life.

The star also poses interesting questions about how giant planets form, as it appears to contain very few elements heavier than hydrogen and helium — fewer than any other star known to host planets. "It is a puzzle for the widely accepted model of planet formation to explain how such a star, which contains hardly any heavy elements at all, could have formed a planet. Planets around stars like this must probably form in a different way," adds Setiawan.