SRON Netherlands Institute for Space Research

Our mission is to bring about breakthroughs in international space research

SEE MORE

SRON Netherlands Institute for Space Research

SRON Netherlands Institute for Space Research

SRON Netherlands Institute for Space Research

Our mission is to bring about breakthroughs in international space research

SEE MORE

SRON Netherlands Institute for Space Research

BOTH SRON BUILDINGS, IN GRONINGEN AND UTRECHT, ARE CLOSED UNTIL FURTHER NOTICE

LATEST NEWS

A team of scientists from six European countries reported today they have finalized a thirty years long investigation of a hypergiant star that crossed the Yellow Evolutionary Void. In that period the star’s surface temperature quickly rose from five to eight thousand degrees. With this discovery a crucial 'missing link' in the evolution of hypergiant stars has been found. 

Hyperreus_8752_1.jpg
Artist's rendition of the hypergiant HR 8752 traversing the Yellow Evolutionary Void. The graph plots the star's surface temperature (log Teff) observed over a century. It increased from ~5000 to ~8000 C between 1985 and 2005, while the hypergiant's radius decreased from 750 to 400 times the radius of the Sun (A. Lobel ROB).
The hypergiants are the most luminous stars currently known in the Universe. The particular star they investigated for thirty years is called HR 8752 and can be observed with binoculars in the Northern constellation of Cassiopeia. HR 8752 is about 250 thousand times as luminous as our Sun. The Yellow Evolutionary Void is the surface temperature range from about five to twelve thousand degrees. It appears that this range is void of hypergiants, while one would expect in that temperature range at least a few hypergiants slowly heating up during the late part of their evolution.

The team of astronomers found that the atmospheres of hypergiants are unstable inside the Evolutionary Void because the outward directed forces in their atmospheres equalize or become even stronger than the inward gravitational pull. The instability of their atmospheres causes the gargantuan stars to lose tremendous amounts of mass and to traverse the Void in a cosmologically very short timespan. The team has discovered that the Void actually consists of two areas where the atmosphere of hypergiants become unstable, associated with the ionization of hydrogen and helium gas respectively, with a narrow stability strip around eight thousand degrees where the atmospheres are slightly more stable.

Three decades
While an analysis of earlier photometric observations showed that, at least from ~1900  to ~1980, HR 8752 stayed at a nearly constant surface temperature of five thousand degrees, the team had some indications that around 1985 this remarkable star was fairly close to or even beyond the low-temperature boundary of the Void. Wondering what would happen, the scientists decided to embark on a long and systematic program of spectroscopic observations that lasted for three decades. These have now shown that in the twenty years period from 1985 to 2005 the star’s surface temperature quickly rose from five to eight thousand degrees, while going through a series of events with very strong loss of mass. During the twenty years the radius of HR 8752 has shrunk from 750 to 400 times the radius of the Sun.

Hans Nieuwenhuijzen, former SRON researcher: “Our team made a tremendous effort to combine these observations of HR 8752 and we are delighted to see this marvellous result after so many years. We knew this was the hypergiant to watch and it payed off”.

Publication
The observations show the hypergiant star to traverse (part of) the Yellow Evolutionary Void. “They are in fact strong confirmation of the theoretical research on the area of the Void” said team member and former SRON director prof. Kees de Jager, an eminent researcher of the hypergiants. The team published the results last week in Astronomy and Astrophysics, entitled The hypergiant HR 8752 evolving through the Yellow Evolutionary Void.

The team is stepping up new research on hypergiants with the new findings on HR 8752. Other hypergiants may reveal similar spectacular properties with large changes in surface temperature on human time-scales. A number of candidate stars was selected for spectroscopic monitoring and the search for these unusually large temperature changes is on.

The science team mentioned in this news release consists of Dr. H. Nieuwenhuijzen (SRON Laboratory for Space Research, Netherlands), Prof. Dr. C. de Jager (NIOZ Royal Netherlands Institute for Sea Research, Netherlands), Dr. I. Kolka (Tartu Observatory, Estonia), Dr. G. Israelian (Instituto de Astrofisica de Canarias, Spain), Dr. A. Lobel (Royal Observatory of Belgium), Dr. E. Zsoldos (Konkoly Observatory, Hungary), Dr. A. Maeder (Observatoire de Genève, Switzerland), and Dr. G. Meynet (Observatoire de Genève, Switzerland).

This bilingual news release is also to be found on Kees de Jager's website.

Images
Download High-resolution image (jpg image format).
Download Low-resolution image (jpg image format).

More information
For more information please contact Hans Nieuwenhuijzen, This email address is being protected from spambots. You need JavaScript enabled to view it.; This email address is being protected from spambots. You need JavaScript enabled to view it. or Kees de Jager, This email address is being protected from spambots. You need JavaScript enabled to view it., phone +31 222 320816 / +31 6 20420611. Web: http://www.cdejager.com.

RESEARCH

SRON has four programme lines, Astrophysics, ExoplanetsEarth, and Technology, with science groups attached, and two expertise groups, Instrument science and Engineering.

ASTROPHYSICS

The Astrophysics programme at SRON is dedicated to unraveling the history of the universe, from the first stars and black holes to large-scale structure.

Read more

EXOPLANETS

The Exoplanets programme is dedicated to atmospheres of planets beyond our solar system and is an in-between of SRON's Astrophysics and Earth programmes.

Read more

EARTH

The Earth programme is aimed at the climate and air quality of planet Earth, with focus on the global carbon cycle and aerosols.

Read more

ENGINEERING

The Engineering group covers SRON's skills and know-how with regard to product assurance, quality assurance, configuration control, design engineering – electronic & mechanical – and parts procurement. It is an expertise group that provides resources for all SRON instrument projects.

Read more

INSTRUMENT SCIENCE

The Instrument science group covers SRON's skills and know-how with regard to instrument physics, system engineering (up to full-instrument level) and project management. It is an expertise group that provides resources for all SRON instrument projects.

Read more

TECHNOLOGY

The Technology programme is SRON's backbone for the development of enabling technology.

Read more

Annual report

New housing

Canon 50 jaar

SRON’s mission is to bring about breakthroughs in international space research 

Therefore the institute develops pioneering technology and advanced space instruments, and uses them to pursue fundamental astrophysical research, Earth science and exoplanetary research. As national expertise institute SRON gives counsel to the Dutch government and coordinates - from a science standpoint - national contributions to international space missions. SRON stimulates the implementation of space science in our society.



SCROLL TO TOP