eso1546 — Science Release

Aging StaròÀÙs Weight Loss Secret Revealed

Giant star caught in the act of slimming down

25 November 2015

A team of astronomers using ESOòÀÙs Very Large Telescope (VLT) has captured the most detailed images ever of the hypergiant star VY Canis Majoris. These observations show how the unexpectedly large size of the particles of dust surrounding the star enable it to lose an enormous amount of mass as it begins to die. This process, understood now for the first time, is necessary to prepare such gigantic stars to meet explosive demises as supernovae.

VY Canis Majoris is a stellar goliath, a red hypergiant, one of the largest known stars in the Milky Way. It is 30òÀÓ40 times the mass of the Sun and 300 000 times more luminous. In its current state, the star would encompass the orbit of Jupiter, having expanded tremendously as it enters the final stages of its life.

The new observations of the star used the SPHERE instrument on the VLT. The adaptive optics system of this instrument corrects images to a higher degree than earlier adaptive optics systems. This allows features very close to bright sources of light to be seen in great detail [1]. SPHERE clearly revealed how the brilliant light of VY Canis Majoris was lighting up clouds of material surrounding it.

And by using the ZIMPOL mode of SPHERE, the team could not only peer deeper into the heart of this cloud of gas and dust around the star, but they could also see how the starlight was scattered and polarised by the surrounding material. These measurements were key to discovering the elusive properties of the dust.

Careful analysis of the polarisation results revealed these grains of dust to be comparatively large particles, 0.5 micrometres across, which may seem small, but grains of this size are about 50 times larger than the dust normally found in interstellar space.

Throughout their expansion, massive stars shed large amounts of material òÀÔ every year, VY Canis Majoris sees 30 times the mass of the Earth expelled from its surface in the form of dust and gas. This cloud of material is pushed outwards before the star explodes, at which point some of the dust is destroyed, and the rest cast out into interstellar space. This material is then used, along with the heavier elements created during the supernova explosion, by the next generation of stars, which may make use of the material for planets.

Until now, it had remained mysterious how the material in these giant starsòÀÙ upper atmospheres is pushed away into space before the host explodes. The most likely driver has always seemed to be radiation pressure, the force that starlight exerts. As this pressure is very weak, the process relies on large grains of dust, to ensure a broad enough surface area to have an appreciable effect [2].

òÀÜMassive stars live short lives,òÀÝ says lead author of the paper, Peter Scicluna, of the Academia Sinica Institute for Astronomy and Astrophysics, Taiwan. òÀÜWhen they near their final days, they lose a lot of mass. In the past, we could only theorise about how this happened. But now, with the new SPHERE data, we have found large grains of dust around this hypergiant. These are big enough to be pushed away by the staròÀÙs intense radiation pressure, which explains the staròÀÙs rapid mass loss.òÀÝ

The large grains of dust observed so close to the star mean that the cloud can effectively scatter the staròÀÙs visible light and be pushed by the radiation pressure from the star. The size of the dust grains also means much of it is likely to survive the radiation produced by VY Canis MajorisòÀÙ inevitable dramatic demise as a supernova [3]. This dust then contributes to the surrounding interstellar medium, feeding future generations of stars and encouraging them to form planets.

Notes

[1] SPHERE/ZIMPOL uses extreme adaptive optics to create diffraction-limited images, which come a lot closer than previous adaptive optics instruments to achieving the theoretical limit of the telescope if there were no atmosphere. Extreme adaptive optics also allows much fainter objects to be seen very close to a bright star.

The images in the new study are also taken in visible light òÀÔ shorter wavelengths than the near-infrared regime, where most earlier adaptive optics imaging was performed. These two factors result in significantly sharper images than earlier VLT images. Even higher spatial resolution has been achieved with the VLTI, but the interferometer does not create images directly.

[2] The dust particles must be large enough to ensure the starlight can push it, but not so large that it simply sinks. Too small and the starlight would effectively pass through the dust; too large and the dust would be too heavy to push. The dust the team observed about VY Canis Majoris was precisely the right size to be most effectively propelled outwards by the starlight.

[3] The explosion will be soon by astronomical standards, but there is no cause for alarm, as this dramatic event is not likely for hundreds of thousands of years. It will be spectacular as seen from Earth òÀÔ perhaps as bright as the Moon òÀÔ but not a hazard to life here.

More information

This research was presented in a paper entitled òÀÜLarge dust grains in the wind of VY Canis MajorisòÀÝ, by P. Scicluna et al., to appear in the journal Astronomy & Astrophysics.

The team is composed of P. Scicluna (Academia Sinica Institute for Astronomy and Astrophysics, Taiwan), R. Siebenmorgen (ESO, Garching, Germany), J. Blommaert (Vrije Universiteit, Brussels, Belgium), M. Kasper (ESO, Garching, Germany), N.V. Voshchinnikov (St. Petersburg University, St. Petersburg, Russia), R. Wesson (ESO, Santiago, Chile) and S. Wolf (Kiel University, Kiel, Germany).

ESO is the foremost intergovernmental astronomy organisation in Europe and the worldòÀÙs most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the worldòÀÙs most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the worldòÀÙs largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is a major partner in ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre European Extremely Large Telescope, the E-ELT, which will become òÀÜthe worldòÀÙs biggest eye on the skyòÀÝ.

Links

• Research paper
• Link to ESOcast about polarimetry
• Photos of the VLT

Contacts

Peter Scicluna
Academia Sinica Institute for Astronomy and Astrophysics
Taiwan
Tel: +886 (02) 2366 5420
Email: peterscicluna@asiaa.sinica.edu.tw

Richard Hook
ESO Public Information Officer
Garching bei M†®nchen, Germany
Tel: +49 89 3200 6655
Cell: +49 151 1537 3591
Email: rhook@eso.org

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