News Release

Hubble captures strobe flashes from a young star

Peer-Reviewed Publication

ESA/Hubble Information Centre

Hubble Image of LRLL 54361 and its Surroundings

image: This infrared image from the NASA/ESA Hubble Space Telescope shows an image of protostellar object LRLL 54361 and its rich cosmic neighbourhood, a region called IC 348. The protostar, which is the bright object with fan-like beams of light coming from it, located towards the right of the image, is letting off flashes of light every 25.3 days. view more 

Credit: NASA, ESA, and J. Muzerolle (STScI)

The cause of the fireworks seen in this Hubble image and video is hidden behind a dense disc and envelope of dust. However, astronomers think that the strobe effect is due to periodic interactions between two newly-formed stars that are gravitationally bound to each other.

These two stars drag material inwards from a surrounding disc of gas and dust. Astronomers propose that the light flashes seen in this video are due to this material suddenly being dumped onto the growing stars as they near one another in their orbits, unleashing a blast of radiation.

"The protostar has such large brightness variations with a precise period that it is very difficult to explain," says James Muzerolle of the Space Telescope Science Institute in Baltimore, USA, who has recently studied this fascinating object using Hubble and NASA's Spitzer Space Telescope. Spitzer made repeated observations over seven years, before Hubble was pointed towards the object to make detailed observations over the period of one pulse event.

The Hubble observations uncover a spectacular movement of light away from the centre of the system, an optical illusion known as a light echo. While it might look like eruptions of gas are coming out of the protostar, these pulses are actually flashes of light propagating through the surrounding dust and gas and reflecting towards the observer: there is no substantial physical motion within the cloud over these timescales.

Flashing double star systems like this one are rare, because close binaries account for only a few percent of our galaxy's stellar population. Moreover, the pulsing light is likely to be a brief phenomenon in the early life of a star.

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Notes

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

Image credit: NASA, ESA, J. Muzerolle (STScI)

Links

* Images of Hubble: http://www.spacetelescope.org/images/archive/category/spacecraft/

* A press release from NASA, with more information about scientific research into LRLL 54361 is available here: http://hubblesite.org/news/2013/04

Contacts

Oli Usher
Hubble/ESA
Garching, Germany
Tel: +49-89-3200-6855
Email: ousher@eso.org

James Muzerolle
Space Telescope Science Institute
Baltimore, USA
Tel: +1-410-338-4719
Email: muzerol@stsci.edu

Ray Villard
Space Telescope Science Institute
Baltimore, USA
Tel: +1-410-338-4514
Email: villard@stsci.edu


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