'Jets' are long outflows of fast-moving gas found near many objects in the Universe, such as around young stars, or coming from black holes, neutron stars, and planetary nebulae, for example. The NASA/ESA Hubble Space Telescope has imaged the young planetary nebula Henize 3-1475 and its bizarre jet. Astronomers have nicknamed it the 'Garden-sprinkler' Nebula.

The origin of jets in the Universe is unclear, but they appear to originate in small regions of space where even Hubble's sharp vision cannot penetrate. To produce a jet, you require some sort of nozzle mechanism. So far, these theoretical 'nozzles' remain hidden by dust that obscures our view of the centres of planetary nebulae.

Despite decades of intense effort, there is no single example of a jet whose origin is clearly understood. The curious S-shape and extreme high speed of its gaseous outflow gives Henize 3-1475 a special place in the study of planetary nebulae.

Henize 3-1475 is located in the constellation of Sagittarius around 18 000 light-years away from us. The central star is more than 12 000 times as luminous as our Sun and weighs three to five times as much. With a velocity of around 4 million kilometres per hour, the jets are the fastest ever discovered. Scientists are also intrigued by the converging, funnel-shaped structures that connect the innermost 'knots' and the core region.

A group of international astronomers led by Angels Riera from Universitat Politècnica de Catalunya, Barcelona, Spain, have combined observations from Hubble's Wide Field and Planetary Camera 2, the Space Telescope Imaging Spectrograph and ground-based telescopes. Their work suggests that the nebula's S-shape and hypervelocity outflow is created by a central source that ejects streams of gas in opposite directions and precesses once every 1500 years. It is like an enormous, slowly rotating garden sprinkler.

The flow is not smooth, but rather episodic with an interval of about 100 years, creating clumps of gas moving away at velocities up to 4 million kilometres per hour. The reason for these intermittent ejections of gas is not known. It may be due to either cyclic magnetic processes in the central star (similar to the Sun's 22-year magnetic cycle), or to interactions with a companion star.

# # # Notes for editors
For broadcasters, animations of Henize 3-1475 are available from telescope.org/video/releases.html">http://www.spacetelescope.org/video/releases.html

The colour image is composed of five different exposures with Hubble's Wide Field and Planetary Camera 2 through the following filters: a wide blue filter (500 seconds), oxygen (800 seconds) shown in green, hydrogen-alpha (830 seconds) shown in yellow-orange, a singly ionised sulphur filter (1200 seconds) shown in orange-red and a wide red filter shown in red.

Image credit: European Space Agency, A. Riera (Universitat Politècnica de Catalunya, Spain) and P. García-Lario (European Space Agency ISO Data Centre, Spain)

The composite image was constructed with data from the ESO/ST-ECF Science Archive. The original Hubble exposures were obtained by J. Borkowski, (North Carolina State University, USA), J. Harrington, (University of Maryland, USA), J. Blondin (North Carolina State University, USA), M. Bobrowsky (Challenger Center for Space Science, USA), M. Meixner (Space Telescope Science Institute, USA), and Skinner (Space Telescope Science Institute, USA).

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

For more information, please contact:

Angels Riera
Universitat Politècnica de Catalunya, Barcelona, Spain
Tel. +34 93 896 77 39 (Monday, Wednesday, Thursday)
Tel. +34 93 402 11 27 (Tuesday and Friday)
E-mail: angels.riera@upc.es

Pedro García-Lario
European Space Agency ISO Data Centre, Villafranca, Spain
Phone: +34 91 813 1389
E-mail: pedro.garcia.lario@esa.int

Lars Lindberg Christensen
Hubble European Space Agency Information Centre, Garching, Germany
Tel: +49 89 3200 6306 (089 within Germany)
Cellular (24 hr): +49 173 3872 621 (0173 within Germany)
E-mail: lars@eso.org

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