First high-resolution image of the young binary star Theta 1 Orionis C

The results show the fascinating new possibilities of high-resolution stellar imaging achievable with infrared interferometry.Provided by the Max Planck Institute, Garching, Germany
By | Published: April 2, 2009 | Last updated on May 18, 2023
Theta 1 Ori C
Zooming in the center of the Orion star-forming region with the four bright Trapezium stars (Theta 1 Ori A-D). The dominant star is Theta 1 Ori C, which was imaged with unprecedented resolution with the VLT interferometer (lower right).
April 2, 2009
A team of astronomers, led by Stefan Kraus and Gerd Weigelt from the Max Planck Institute for Radio Astronomy (MPIfR) in Bonn, Germany, used European Southern Observatory’s (ESO) Very Large Telescope Interferometer (VLTI) to obtain the sharpest image of the young double star Theta 1 Orionis C in the Orion Trapezium Cluster. It is the most massive star in the nearest high-mass star-forming region. The new image clearly separates the two massive young stars of this system. The observations have a spatial resolution of about 2 milliarcseconds, corresponding to the size of a car on the surface of the Moon. The team was able to derive the properties of the orbit of this binary system, including the masses of the two stars — 38 and 9 solar masses — and their distance from us — 1,350 light-years. The results show the fascinating new possibilities of high-resolution stellar imaging achievable with infrared interferometry.

A particularly promising way to increase the angular resolution of conventional optical telescopes is the method of interferometry. This technique allows astronomers to combine the light from several telescopes, forming a huge virtual telescope with a resolving power corresponding to that of a single telescope with 656 feet (200 meters) diameter. The VLTI now offers this revolutionary technique to European astronomers and allows them to directly reconstruct images from the interferometric infrared data. A team of European astronomers utilized the VLTI and its near-infrared beam-combination instrument AMBER to demonstrate the imaging capabilities of this unique facility and to study the intriguing massive young star Theta 1 Ori C in unprecedented detail.

Theta 1 Ori C is the dominant and most luminous star in the Orion star-forming region. Located at a distance of only about 1,300 light years, the Orion region is the nearest region where massive stars are born, and it provides a unique laboratory to study the formation process of high-mass stars in detail. The intense radiation of Theta 1 Ori C is ionizing the whole Orion Nebula. With its strong wind, the star also shapes the famous Orion proplyds, young stars still surrounded by their protoplanetary dust disks.

Although Theta 1 Ori C appeared to be a single star, both with conventional telescopes and the Hubble Space Telescope, the team discovered the existence of a close companion. “VLTI interferometry with the AMBER instrument allowed us to obtain an image of this system with the spectacular angular resolution of only 2 milliarcseconds,” Kraus said. “This corresponds to the resolving power of a space telescope with a mirror diameter of 427 feet (130 meters).” The VLTI image reveals that in March 2008 the angular distance between the two stars was only about 20 milliarcseconds.

The collection of measurements shows that the two massive stars are on a very eccentric orbit with a period of 11 years. Using Kepler’s third law, the masses of the two stars were derived to be 38 and 9 solar masses. Furthermore, the measurements allow a trigonometric determination of the distance to Theta 1 Ori C and to the very center of the Orion star-forming region. The resulting distance of 1,350 light-years is in agreement with the work of another research group led by Karl Menten, also from MPIfR, who measured trigonometric parallaxes of the nonthermal radio emission of Orion Nebula stars using the Very Long Baseline Array. These results are important for studies of the Orion region as well as the improvement of theoretical models of high-mass star formation.

Since 1609, when Galileo Galilei first pointed a telescope toward the sky, the field of observational astronomy has strongly evolved in both spectral coverage and angular resolution. “Our observations demonstrate the fascinating new imaging capabilities of the VLTI,” Weigelt said. “This infrared interferometry technique will certainly lead to many fundamental new discoveries.”