Fledgling stars flicker in the heart of Orion
Astronomers were surprised to see the brightness of the young objects varying by more than 20 percent over just a few weeks.
By
ESA, Noordwijk, Netherlands —
Published:
March 1, 2012 Baby stars in Orion Nebula. Credit: ESA/PACS/NASA/JPL-Caltech/IRAM
Images from Herschel’s far-infrared instrument and two of Spitzer’s instruments working at shorter wavelengths give scientists a more detailed picture of stars growing in the heart of one of the most famous objects in the night sky.
The Orion Nebula is 1,350 light-years from Earth and appears prominently in the winter skies for Northern Hemisphere observers.
Sometimes referred to as Orion’s Sword, the nebula lies below the three stars that form the belt of Orion the Hunter, one of the most easily recognized constellations. It is one of the few nebulae visible to the naked eye and is a popular target for amateur astronomers.
The nebula contains the nearest site of massive star formation, with intense ultraviolet light from hot young stars causing gas and dust in the region to glow. Inside that dust — hidden at visible wavelengths — is a host of even younger stars still growing in their earliest phase of evolution.
This new combined far- and mid-infrared image cuts through the obscuring dust and reveals these embryonic stars.
A star forms when a dense cloud of gas and dust coalesces and then collapses under its own gravity, creating a central warm protostar surrounded by a swirling disk and a larger envelope.
Much of this material will spiral in and collect onto the protostar over hundreds of thousands of years before nuclear fusion is triggered at the core and it becomes a fully-fledged star. Some of the remnant gas and dust in the disk may go on to form a planetary system — as happened with our solar system.
A team of astronomers led by Nicolas Billot of the Institut de Radioastronomie Millimétrique, in Granada, Spain, used Herschel to image the Orion Nebula region once a week for six weeks in the late winter and spring last year. Herschel’s PACS Photodetector Array Camera and Spectrometer detected cold dust particles in disks around the youngest protostars at far-infrared wavelengths. This was combined with archival Spitzer images taken at shorter, mid-infrared wavelengths, which show older, hotter objects.
Astronomers were surprised to see the brightness of the young objects varying by more than 20 percent over just these few weeks, since the accretion process should take years or even centuries. They now have to explain why this is happening.
One possibility is that lumpy filaments of gas are funneling from the outer disk towards central regions near the star, temporarily warming the inner disk and leading it to brighten. Another scenario is that cold material is piling up at the inner edge and casting shadows on the outer disk, causing it to darken temporarily. In either case, it is clear that the gestation of baby stars is anything but a smooth, uniform process.
“Yet again, Herschel observations surprise us and provide more interesting insights into what happens during the very earliest phases of stars and planet formation,” said Göran Pilbratt from ESA.
It is only through the unprecedented far-infrared sensitivity and resolution of the Herschel Space Observatory, combined with the shorter-wavelength data from Spitzer, that astronomers are able to witness and fully discover the physical processes of star birth.
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