The ultimate RAVE: final data release published | WPN World People News

The RAdial Velocity Experiment RAVE is a spectroscopic survey of stars in the southern hemisphere. RAVE was designed to get a representative census of the movements and of the atmospheric properties of stars in the wider neighbourhood of the Sun. By means of spectroscopy, the light of a star is decomposed into its rainbow colours. By analysing the spectra, the radial velocity of a star – the movement of the stars in the direction of the observer's view, can be determined. Furthermore, stellar spectra also enable scientists to determine stellar parameters like temperatures, surface gravities, and composition. In order to trace the structure and shape of our galaxy, RAVE successfully measured 518,387 spectra for 451,783 Milky Way stars.

RAVE observed nearly half a million stars of our Galaxy. The Sun is located at the centre of the coordinate system. Credit: AIP/K. Riebe, the RAVE Collaboration; Milky Way image (background): R. Hurt (SSC); NASA/JPL-Caltech

Astronomers are not only used to think in long time scales – their projects also are often many-year endeavours. RAVE observed the sky for almost every clear night between 2003 and 2013 at the 1.2-metre UK Schmidt telescope of the Anglo-Australian Observatory in Siding Spring, Australia. RAVE utilized a dedicated fibre-optical setup to simultaneously take spectra of up to 150 stars in a single observation. Only with this massive multiplexing such a large number of targets was achievable – the largest spectroscopic survey before RAVE featured only some 14000 targets. In this way the survey obtained a representative sample of the stars around our Sun that are located roughly in a volume 15000 light years across.

RAVE observed nearly half a million stars of our Galaxy. The Sun is located at the centre of the coordinate system. The colours represent radial velocities: red are receding stars and stars depicted in blue are approaching. Credit: AIP/K. Riebe, the RAVE Collaboration; Milky Way image (background): R. Hurt (SSC); NASA/JPL-Caltech

Over the past 15 years, an increasing number of stars and refined data products have been released. The final RAVE data release not only provides for the first time the spectra of all stars in the RAVE sample; the stars were also matched with stars from the DR2 catalogue of the satellite mission Gaia. Thanks to the exquisite distances and proper motions measured by Gaia, considerably improved stellar temperatures, surface gravities and the chemical composition of the stellar atmospheres could be derived.

Map of the night sky centered on the Milky Way, with stars observed by RAVE. More than 6000 observation fields mainly from the southern sky (below the celestial equator, red line) with about half a million stars have been observed. Credit: AIP/K. Riebe, the RAVE Collaboration; Milky-Way image (background): ESO/S. Brunier
The stars observed by RAVE are from the southern celestial hemisphere, since the UK-Schmidt telescope is located in Australia. There are only a few observation fields in the area of the Milky Way disk (central part), because in this crowded area it is much harder to collect and analyse individual stars.

“The RAVE data releases have provided new insights into the motion of stars and chemical structure of our Milky Way,” says Matthias Steinmetz, leader of the RAVE collaboration and scientific chairman of the Leibniz Institute for Astrophysics Potsdam (AIP). “The final data release concludes one of the first systematic spectroscopic Galactic Archaeology surveys. It’s really exciting to think about finishing this 15-year project. Thanks to RAVE, we have gained new insights into the structure and composition of our Milky Way."

The stars observed by RAVE are from the southern celestial hemisphere, since the UK-Schmidt telescope is located in Australia. There are only a few observation fields in the area of the Milky Way disk (central part), because in this crowded area it is much harder to collect and analyse individual stars. Credit: AIP/K. Riebe, the RAVE Collaboration

Some of the key results of RAVE include the determination of the minimum speed needed for a star to escape the gravitational pull of the Milky Way. The results confirmed that dark matter, an invisible component of the Universe of yet unknown nature, dominates the mass of our Galaxy. With RAVE it could be shown that the Milky Way disk is asymmetric and wobbles owing to the interaction with spiral arms and the infall of satellite galaxies. RAVE also allowed for the identification of stellar streams in the solar environment. These streams of stars are the residues of torn apart old dwarf galaxies that have merged into our Milky Way in the past. The chemical element abundances of the observed stars hold important clues to the chemical composition and the subsequent metal enrichment of the interstellar medium traced by stars of different ages and metallicities. With RAVE, astronomers efficiently searched for the very first stars, which are very metal-poor and give clues about the earliest epochs of star formation and the chemical evolution in the Milky Way.

The RAVE collaboration consists of researchers from over 20 institutions around the world and is coordinated by the AIP. More than 100 refereed scientific articles based on RAVE data were published since the first data release.

Source: Leibniz Institute for Astrophysics Potsdam