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I provide a summary of the ESA space astrometry mission Gaia regarding its main objectives and current status following the 2nd data release (Gaia DR2) in April 2018. The Gaia achievements in astrometry are assessed with a historical…

天体物理仪器与方法 · 物理学 2019-06-24 F. Mignard

Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original interferometric concept was changed to a direct-imaging…

天体物理仪器与方法 · 物理学 2016-09-15 Gaia Collaboration

The final astrometric data from the Gaia mission will transform our view of the stellar content of the Galaxy, particularly when complemented with spectroscopic surveys providing stellar parameters, line-of-sight kinematics and elemental…

星系天体物理 · 物理学 2018-06-13 Rosemary F. G. Wyse

The Gaia satellite, planned for launch by the European Space Agency (ESA) in 2013, is the next generation astrometry mission following Hipparcos. While mapping the whole sky, the Gaia space mission is expected to discover thousands of Solar…

地球与行星天体物理 · 物理学 2012-12-04 M. Todd , P. Tanga , D. M. Coward , M. G. Zadnik

ESA and NASA are studying projects having a tremendous return on variable star research. Other national space agencies are also studying or developing projects of smaller costs but with impressive returns. The projects range from global…

天体物理学 · 物理学 2007-05-23 Laurent Eyer

Stellar multiplicity is among the oldest and richest problems in astrophysics. Binary stars are a cornerstone of stellar mass and radius measurements that underpin modern stellar evolutionary models. Binaries are the progenitors of many of…

太阳与恒星天体物理 · 物理学 2024-05-15 Kareem El-Badry

In this concluding article I recall the early history of the Gaia mission, showing that the original science case and expectations of wide community interest in Gaia data have been met. The quarter-century long partnership involving some…

天体物理仪器与方法 · 物理学 2018-06-13 Gerard Gilmore

The scientific community needs to be prepared to analyse the data from Gaia, one of the most ambitious ESA space missions, to be launched in 2012. The purpose of this paper is to provide data and tools in order to predict in advance how…

天体物理仪器与方法 · 物理学 2015-05-19 C. Jordi , M. Gebran , J. M. Carrasco , J. de Bruijne , H. Voss , C. Fabricius , J. Knude , A. Vallenari , R. Kohley , A. Mora

We present the results of realistic end-to-end simulations of observations of nearby stars with the proposed global astrometry mission GAIA, recently recommended within the context of ESA's Horizon 2000 Plus long-term scientific program. We…

天体物理学 · 物理学 2016-08-30 M. G. Lattanzi , A. Spagna , A. Sozzetti , S. Casertano

In this article we present an overview of the ESA Gaia mission and of the unprecedented impact that Gaia will have on the field of variable star research. We summarise the contents and impact of the first Gaia data release on the…

Gaia will provide parallaxes and proper motions with accuracy ranging from 10 to 1000 microarcsecond on up to one billion stars. Most of these will be disk stars: for an unreddened K giant at 6 kpc, it will measure the distance accurate to…

天体物理学 · 物理学 2015-05-13 C. A. L. Bailer-Jones

Near-future data from ESA's Gaia mission will provide precise, full phase-space information for hundreds of millions of stars out to heliocentric distances of ~10 kpc. This "horizon" for full phase-space measurements is imposed by the Gaia…

宇宙学与河外天体物理 · 物理学 2013-11-12 Adrian M. Price-Whelan , Kathryn V. Johnston

Stellar variability studies are now reaching a completely new level thanks to ESA's Gaia mission, which enables us to locate many variable stars in the Hertzsprung-Russell diagram and determine the various instability strips/bands.…

We describe the preliminary results of a ground-based observing campaign aimed at building a grid of approximately 200 spectro-photometric standard stars (SPSS), with an internal $\simeq 1$\% accuracy (and sub-percent precision), tied to…

太阳与恒星天体物理 · 物理学 2020-12-23 Nicoletta Sanna , Elena Pancino , Giuseppe Altavilla , Silvia Marinoni , Monica Rainer

The era of high-precision astrometry has dawned upon us. The potential of Gaia $\mu$as-level precision in positional measurements is about to be unleashed in the field of extrasolar planetary systems. The Gaia data hold the promise for much…

地球与行星天体物理 · 物理学 2015-02-13 A. Sozzetti

The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representative samples of the stellar populations in the Galaxy, and a…

太阳与恒星天体物理 · 物理学 2022-10-19 G. Gilmore , S. Randich , C. C. Worley , A. Hourihane , A. Gonneau , G. G. Sacco , J. R. Lewis , L. Magrini , P. Francois , R. D. Jeffries , S. E. Koposov , A. Bragaglia , E. J. Alfaro , C. Allende Prieto , R. Blomme , A. J. Korn , A. C. Lanzafame , E. Pancino , A. Recio-Blanco , R. Smiljanic , S. Van Eck , T. Zwitter , T. Bensby , E. Flaccomio , M. J. Irwin , E. Franciosini , L. Morbidelli , F. Damiani , R. Bonito , E. D. Friel , J. S. Vink , L. Prisinzano , U. Abbas , D. Hatzidimitriou , E. V. Held , C. Jordi , E. Paunzen , A. Spagna , R. J. Jackson , J. Maiz Apellaniz , M. Asplund , P. Bonifacio , S. Feltzing , J. Binney , J. Drew , A. M. N. Ferguson , G. Micela , I. Negueruela , T. Prusti , H. -W. Rix , A. Vallenari , M. Bergemann , A. R. Casey , P. de Laverny , A. Frasca , V. Hill , K. Lind , L. Sbordone , S. G. Sousa , V. Adibekyan , E. Caffau , S. Daflon , D. K. Feuillet , M. Gebran , J. I. Gonzalez Hernandez , G. Guiglion , A. Herrero , A. Lobel , T. Merle , S. Mikolaitis , D. Montes , T. Morel , G. Ruchti , C. Soubiran , H. M. Tabernero , G. Tautvaisiene , G. Traven , M. Valentini , M. Van der Swaelmen , S. Villanova , C. Viscasillas Vazquez , A. Bayo , K. Biazzo , G. Carraro , B. Edvardsson , U. Heiter , P. Jofre , G. Marconi , C. Martayan , T. Masseron , L. Monaco , N. A. Walton , S. Zaggia , V. Aguirre Borsen-Koch , J. Alves , L. Balaguer-Nunez , P. S. Barklem , D. Barrado , M. Bellazzini , S. R. Berlanas , A. S. Binks , A. Bressan , R. Capuzzo-Dolcetta , L. Casagrande , L. Casamiquela , R. S. Collins , V. D'Orazi , M. L. L. Dantas , V. P. Debattista , E. Delgado-Mena , P. Di Marcantonio , A. Drazdauskas , N. W. Evans , B. Famaey , M. Franchini , Y. Fremat , X. Fu , D. Geisler , O. Gerhard , E. A. Gonzalez Solares , E. K. Grebel , M. L. Gutierrez Albarran , F. Jimenez-Esteban , H. Jonsson , T. Khachaturyants , G. Kordopatis , J. Kos , N. Lagarde , H. -G. Ludwig , L. Mahy , M. Mapelli , E. Marfil , S. L. Martell , S. Messina , A. Miglio , I. Minchev , A. Moitinho , J. Montalban , M. J. P. F. G. Monteiro , C. Morossi , N. Mowlavi , A. Mucciarelli , D. N. A. Murphy , N. Nardetto , S. Ortolani , F. Paletou , J. Palous , J. C. Pickering , A. Quirrenbach , P. Re Fiorentin , J. I. Read , D. Romano , N. Ryde , N. Sanna , W. Santos , G. M. Seabroke , L. Spina , M. Steinmetz , E. Stonkute , E. Sutorius , F. Thevenin , M. Tosi , M. Tsantaki , N. Wright , R. F. G. Wyse , M. Zoccali , J. Zorec , D. B. Zucker

The sheer size of high-accuracy, multi-band photometry, spectroscopy, astrometry and seismic data that space missions like Kepler, Gaia, PLATO, TESS, JWST and ground-based facilities under development such as MOONS, WEAVE and the LSST will…

太阳与恒星天体物理 · 物理学 2020-01-08 Gisella Clementini , Marcella Marconi , Alessia Garofalo

At the heart of a successful theory of galaxy formation must be a detailed physical understanding of the dissipational processes which form spiral galaxies. To what extent can we unravel the events that produced the Galaxy as we see it…

天体物理学 · 物理学 2011-03-10 J. Bland-Hawthorn

GAIA (originally the acronym for Global Astrometric Interferometer for Astrophysics) is a mission of the European Space Agency (ESA) which will make the largest, most precise three dimensional map of our Galaxy by an unparalleled survey of…

科普物理 · 物理学 2021-06-10 Priya Hasan

On the 19th of December 2013, the Gaia spacecraft was successfully launched by a Soyuz rocket from French Guiana and started its amazing journey to map and characterise one billion celestial objects with its one billion pixel camera. In…