Image of the Week

 

10 years of Gaia science operations

 

Figure 1. Some impressive numbers from the Gaia mission. The numbers are based on the predicted spacecraft ephemeris and the data accumulated by the science Data Integrity and Accountability Checks service. These numbers are updated multiple times per day and published on this page, which contains also more information on the exact meaning of each type of measurement taken. The numbers above represent 10 years of Gaia science operations. Credits: ESA/Gaia/DPAC - CC BY-SA 3.0 IGO.

 

Today Gaia celebrates 10 years of science operations. The above image shows some impressive numbers on the current status of the Gaia mission. Since the start of Gaia's science operations phase on 25 July 2014, Gaia has scanned across more than 256 billion objects. The typical star flow in the focal plane is about 3400 stars per second. It is good to realize that this is the typical star flow, not the maximum nor the minimum! It makes a big difference whether Gaia scans over the Galactic plane, an area bursting with stars, or over the Galactic anticentre, a less crowded area in the sky. Some areas are so crowded that Gaia adds a different type of observation because its regular way of observing objects cannot cope with the large amount of stars in view, and special engineering images are stored to allow capturing even more stars per second. A story discussing Gaia's observation of a crowded area was published along with Gaia's Focused Product Release: "Omega Centauri, a globular cluster bursting with stars - Gaia's additional data from engineering images taken in crowded regions".

When Gaia scans objects, the objects transit across the CCDs in the focal plane. The Gaia focal plane consists of two columns of Sky-Mapper CCDs, 9 columns of astrometric CCDs, 1 column each for the red-photometer and blue-photometer CCDs, and finally also 3 columns (with reduced amount of rows) of radial-velocity-spectrograph CCDs, as illustrated in the figure below. Full details on the focal plane can be found here and also from the Gaia Data Release 3 Documentation. A whopping amount of over 2.5 trillion astrometric CCD measurements were taken by now, along with over 500 billion photometric CCD measurements and close to 50 billion spectroscopic CCD measurements (see Figure 1).

Figure 2. Gaia focal plane as published here. Image credit: ESA. Acknowledgement: Alex Short.

 

So far the Gaia Collaboration has published new data 5 times already: Gaia Data Release 1 in September 2016, Gaia Data Release 2 in April 2018, Gaia Early Data Release 3 in December 2020, and Gaia's full Data Release 3 in June 2022 (which together form one complete data set). The last data release was focused on 5 specific data products: Gaia's Focused Product Release, as available since October 2023. Gaia's Data Release 4 is planned not before mid-2026 and will contain for the first time all data products planned for the nominal mission, a huge catalogue which is expected to amount to more than 500 TB of data.

Gaia's data releases have brought a wealth of star data, on stars in our Milky Way and beyond. But Gaia adds many other data products on top of its star data. The Gaia catalogues contain information on Solar system objects as well as on galaxies and quasars. The Gaia data releases are prepared by the Gaia Data Processing and Analysis Consortium in collaboration with the ESA Gaia teams. About 450 people from 25 countries contribute to the Gaia data processing! A story on the people behind the scenes was published with Gaia's Data Release 3: "Who produced the data? The people behind the scenes!".

 

Figure 3. Infographic on Gaia's 10 years in space, as published here and as created in view of Gaia's 10th launch anniversary. Credits: ESA, CC BY-SA 3.0 IGO.

 

The data sets released so far have been used heavily by astronomers across the world. In the figure below the yearly amount of peer-reviewed papers using Gaia data can be found. Currently, on average, about 5 Gaia-related papers are published per day. A full library with all Gaia-related papers can be found from the Gaia ADS libary. Stories discussing the science results from the mission are published here on Gaia Cosmos, as well as on esa.int/gaia. An archive of stories is also available from the ESA science and technology website. Several of these stories give an extensive overview on the advances made with the Gaia mission. For example the stories published with the Gaia launch anniversary: 10 Science topics to celebrate Gaia's 10 years in space and Gaia's decade of discoveries: unravelling the intricacies of our galaxy.

 


Figure 4. Overview of Gaia-related peer-reviewed publications. Credits: ESA/Gaia/DPAC - CC BY-SA 3.0 IGO.

 

Below some iconic visuals are shown highlighting the advances made with Gaia. First of all, our knowledge of our home galaxy has improved a lot. An updated view of the Milky Way top-down view was published along with Gaia's data release 3 and Gaia's launch anniversary. While detailed images exist of many external galaxies, our own galaxy requires extensive mapping from within to observe the structures that together give shape to the Milky Way. Even though Gaia has mapped about 2 billion stars, still it only covers 1% of the Milky Way stars. Some parts of our Milky Way are largely unexplored and are difficult to map even for a dedicated mapping mission like Gaia. Especially the area behind the Galactic Centre is hard to map, there are already so many stars in view when Gaia scans across the Galactic centre that the part behind is completely obscured by them (or should we say, Gaia is blinded out by the sheer amount of stars there). This is why we refer to the below image as an artistic impression. It is partly constructed from data, and partly from the latest Milky Way models.

 

Figure 5. Artistic impression of the Milky Way - face-on, based on the latest Gaia data. Credits: ESA/Gaia/DPAC, Stefan Payne-Wardenaar - CC BY-SA 3.0 IGO.

 

A second iconic image highlights the multi-dimensional data in the Gaia catalogues. It shows several different data products and was created to celebrate the first anniversary of Gaia's Data Release 3. From top to bottom we see a part of several Gaia sky maps: stellar motion, stellar age, brightnesses, variable stars, stellar extinction, interstellar medium, line-of-sight velocities, chemical information, 3D motion and colour information. While Gaia Data Release 3 contains about 60 different data products, the next data release is expected to contain about double this amount. We hope to provide a more detailed overview of the type of data to be expected with Gaia Data Release 4 soon. A first overview was provided during the Gaia symposium at the European Astronomical Society's annual meeting.

 

Figure 6. A composition of Gaia sky maps, based on different Gaia data products from Gaia's third data release. Created to celebrate the first anniversary of Gaia Data Release 3. Find all sky maps used for this creation here. Credits: ESA/Gaia/DPAC - CC BY-SA 3.0 IGO. Acknowledgements: created by Tineke Roegiers, based on different Gaia sky maps created by ESA/Gaia/DPAC - CC BY-SA 3.0 IGO and inspired by NASA's Multiwavelength Milky Way Images.

 

Celebrate with us Gaia's 10 years of science operations! The Gaia mission has come a long way since 25 July 2014 and the symbolic handover of the Gaia flag (featuring the fairing logo) by the team operating the spacecraft to the team responsible for science operations, marking the official start of Gaia's science operations phase. Soon, Gaia will stop taking new science observations. The cold gas needed to keep the spacecraft scanning at a stable pace will be depleted early 2025. The phase of capturing science observations is planned to end on 15 January 2024 and will be followed by a series of technology tests to help future missions with similar instruments onboard. The mission will then focus on producing the last data releases: Gaia Data Release 4, based on 66 months of data and containing for the first time all data products planned, and the final legacy catalogue: Gaia Data Release 5.

 

Figure 7. Gaia flag arrives at ESAC, as published here. Image: courtesy of Wil O'Mullane.

 

Figure 8. Visual created by the the Art of Gueguel. Original creator of Gaia's fairing logo. The girl, Sharly, originally reaching for the stars at a young age, has aged along with Gaia these 10 years. Credits: The Art of Gueguel and Sharly.

 

Story written by T. Roegiers

 

Credits: ESA/Gaia/DPAC

[Published: 25/07/2024]

Image of the Week Archive

2024

20/08: Gaia discovers interesting duo belonging to the Milky Way halo: an ultracool subdwarf with a white dwarf companion

25/07: 10 years of Gaia science operations

23/07: How binary stars change their stellar dance with age

25/06: Dynamical masses across the Hertzsprung-Russell diagram

28/05: Did Gaia find its first neutron star?

26/04: A textbook solar eruption

22/04: Gaia's contribution to discovering distant worlds

16/04: Gaia spots Milky Way's most massive black hole of stellar origin

02/04: The Gaia Cataclysmic Variable hook

2023

19/12: 10 Science topics to celebrate Gaia's 10 years in space

31/10: Gaia observes cosmic clock inside a heavenly jewel

10/10: Gaia Focused Product Release stories

27/09: Does the Milky Way contain less dark matter than previously thought?

22/09: Mass-luminosity relation from Gaia's binary stars

13/09: Gaia DPAC CU8 seminars

13/06: Gaia's multi-dimensional Milky Way

18/05: Mapping the Milky Way

15/05: Goonhilly station steps in to save Gaia science data

25/04: The Gaia ESA Archive

05/04: Dual quasar found to be hosted by an ongoing galaxy merger at redshift 2.17

21/03: GaiaVari: a citizen science project to help Gaia variability classificaton

09/02: Missing mass in Albireo Ac: massive star or black hole?

31/01: Gaia reaches to the clouds – 3D kinematics of the LMC

25/01: Meet your neighbours: CNS5 - the fifth catalogue of nearby stars

18/01: A single-object visualisation tool for Gaia objects

2022

25/11: 100 months of Gaia data

23/11: The astonishment

09/11: Gamma-Ray Burst detection from Lagrange 2 point by Gaia

04/11: Gaia's first black hole discovery: Gaia BH1

26/10: Are Newton and Einstein in error after all?

21/10: Gaia ESA Archive goes live with third data release

06/10: Mapping the interstellar medium using the Gaia RVS spectra

26/09: Gaia on the hunt for dual quasars and gravitational lenses

23/09: Gaia's observation of relativistic deflection of light close to Jupiter

13/06: Gaia Data Release 3

10/06: MK classification of stars from BP/RP spectrophotometry across the Hertzsprung-Russell diagram

09/06: BP/RP low-resolution spectroscopy across the Hertzsprung-Russell diagram

27/05: Cepheids and their radial velocity curves

23/05: The Galaxy in your preferred colours

19/05: GaiaXPy 1.0.0 released, a tool for Gaia's BP/RP spectra users

11/05: Systemic proper motions of 73 galaxies in the Local group

28/03: Gaia query statistics

16/03: Gaia's first photo shooting of the James Webb Space Telescope

08/03: Gaia's women in science - coordination unit 8

25/02: Not only distances: what Gaia DR3 RR Lyrae stars will tell us about our Galaxy and beyond

11/02: Gaia's women in science

31/01: Astrometric orbit of the exoplanet-host star HD81040

12/01: The Local Bubble - source of our nearby stars

05/01: A Milky-Way relic of the formation of the Universe

2021

23/12: Signal-to-Noise ratio for Gaia DR3 BP/RP mean spectra

22/12: The 7 October 2021 stellar occultation by the Neptunian system

01/12: Observation of a long-predicted new type of binary star

24/09: Astrometric microlensing effect in the Gaia16aye event

22/09: the power of the third dimension - the discovery of a gigantic cavity in space

16/09: An alternative Gaia sky chart

25/08: Gaia Photometric Science Alerts and Gravitational Wave Triggers

09/07: How Gaia unveils what stars are made of

23/06: Interviews with CU3

27/04: HIP 70674 Orbital solution resulting from Gaia DR3 processing

30/03: First transiting exoplanet by Gaia

26/03: Apophis' Yarkovsky acceleration improved through stellar occultation

26/02: Matching observations to sources for Gaia DR4

2020

22/12: QSO emission lines in low-resolution BP/RP spectra

03/12: Gaia Early Data Release 3

29/10: Gaia EDR3 passbands

15/10: Star clusters are only the tip of the iceberg

04/09: Discovery of a year long superoutburst in a white dwarf binary

12/08: First calibrated XP spectra

22/07: Gaia and the size of the Solar System

16/07: Testing CDM and geometry-driven Milky Way rotation Curve Models

30/06: Gaia's impact on Solar system science

14/05: Machine-learning techniques reveal hundreds of open clusters in Gaia data

20/03: The chemical trace of Galactic stellar populations as seen by Gaia

09/01: Discovery of a new star cluster: Price-Whelan1

08/01: Largest ever seen gaseous structure in our Galaxy

2019

20/12: The lost stars of the Hyades

06/12: Do we see a dark-matter like effect in globular clusters?

12/11: Hypervelocity star ejected from a supermassive black hole

17/09: Instrument Development Award

08/08: 30th anniversary of Hipparcos

17/07: Whitehead Eclipse Avoidance Manoeuvre

28/06: Following up on Gaia Solar System Objects

19/06: News from the Gaia Archive

29/05: Spectroscopic variability of emission lines stars with Gaia

24/05: Evidence of new magnetic transitions in late-type stars

03/05: Atmospheric dynamics of AGB stars revealed by Gaia

25/04: Geographic contributions to DPAC

22/04: omega Centauri's lost stars

18/04: 53rd ESLAB symposium "the Gaia universe"

18/02: A river of stars

2018
21/12: Sonification of Gaia data
18/12: Gaia captures a rare FU Ori outburst
12/12: Changes in the DPAC Executive
26/11:New Very Low Mass dwarfs in Gaia data
19/11: Hypervelocity White Dwarfs in Gaia data
15/11: Hunting evolved carbon stars with Gaia RP spectra
13/11: Gaia catches the movement of the tiny galaxies surrounding the Milky Way
06/11: Secrets of the "wild duck" cluster revealed
12/10: 25 years since the initial GAIA proposal
09/10: 3rd Gaia DPAC Consortium Meeting
30/09: A new panoramic sky map of the Milky Way's Stellar Streams
25/09: Plausible home stars for interstellar object 'Oumuamua
11/09: Impressions from the IAU General Assembly
30/06: Asteroids in Gaia Data
14/06: Mapping and visualising Gaia DR2

25/04: In-depth stories on Gaia DR2

14/04: Gaia tops one trillion observations
16/03: Gaia DR2 Passbands
27/02: Triton observation campaign
11/02: Gaia Women In Science
29/01: Following-up on Gaia
2017
19/12: 4th launch anniversary
24/11: Gaia-GOSA service
27/10: German Gaia stamp in the making
19/10: Hertzsprung-russell diagram using Gaia DR1
05/10: Updated prediction to the Triton occultation campaign
04/10: 1:1 Gaia model arrives at ESAC
31/08: Close stellar encounters from the first Gaia data release
16/08: Preliminary view of the Gaia sky in colour
07/07: Chariklo stellar occultation follow-up
24/04: Gaia reveals the composition of asteroids
20/04: Extra-galactic observations with Gaia
10/04: How faint are the faintest Gaia stars?
24/03: Pulsating stars to study Galactic structures
09/02: Known exoplanetary transits in Gaia data
31/01: Successful second DPAC Consortium Meeting
2016
23/12: Interactive and statistical visualisation of Gaia DR1 with vaex
16/12: Standard uncertainties for the photometric data (in GDR1)
25/11: Signature of the rotation of the galactic bar uncovered
15/11: Successful first DR1 Workshop
27/10: Microlensing Follow-Up
21/10: Asteroid Occultation
16/09: First DR1 results
14/09: Pluto Stellar Occultation
15/06: Happy Birthday, DPAC!
10/06: 1000th run of the Initial Data Treatment system
04/05: Complementing Gaia observations of the densest sky regions
22/04: A window to Gaia - the focal plane
05/04: Hipparcos interactive data access tool
24/03: Gaia spots a sunspot
29/02: Gaia sees exploding stars next door
11/02: A new heart for the Gaia Object Generator
04/02: Searching for solar siblings with Gaia
28/01: Globular cluster colour-magnitude diagrams
21/01: Gaia resolving power estimated with Pluto and Charon
12/01: 100th First-Look Weekly Report
06/01: Gaia intersects a Perseid meteoroid
2015
18/12: Tales of two clusters retold by Gaia
11/11: Lunar transit temperature plots
06/11: Gaia's sensors scan a lunar transit
03/11: Celebrity comet spotted among Gaia's stars
09/10: The SB2 stars as seen by Gaia's RVS
02/10: The colour of Gaia's eyes
24/09: Estimating distances from parallaxes
18/09: Gaia orbit reconstruction
31/07: Asteroids all around
17/07: Gaia satellite and amateur astronomers spot one in a billion star
03/07: Counting stars with Gaia
01/07: Avionics Model test bench arrives at ESOC
28/05: Short period/faint magnitude Cepheids in the Large Magellanic Cloud
19/05: Visualising Gaia Photometric Science Alerts
09/04: Gaia honours Einstein by observing his cross
02/04: 1 April - First Look Scientists play practical joke
05/03: RR Lyrae stars in the Large Magellanic Cloud as seen by Gaia
26/02: First Gaia BP/RP deblended spectra
19/02: 13 months of GBOT Gaia observations
12/02: Added Value Interface Portal for Gaia
04/02: Gaia's potential for the discovery of circumbinary planets
26/01: DIBs in three hot stars as seen by Gaia's RVS
15/01: The Tycho-Gaia Astrometric Solution
06/01: Close encounters of the stellar kind
2014
12/12: Gaia detects microlensing event
05/12: Cat's Eye Nebula as seen by Gaia
01/12: BFOSC observation of Gaia at L2
24/11: Gaia spectra of six stars
13/11: Omega Centauri as seen by Gaia
02/10: RVS Data Processing
12/09: Gaia discovers first supernova
04/08: Gaia flag arrives at ESAC
29/07: Gaia handover
15/07: Eclipsing binaries
03/07: Asteroids at the "photo finish"
19/06: Calibration image III - Messier 51
05/06: First Gaia BP/RP and RVS spectra
02/06: Sky coverage of Gaia during commissioning
03/04: Gaia source detection
21/02: Sky-background false detections in the sky mapper
14/02: Gaia calibration images II
06/02: Gaia calibration image I
28/01: Gaia telescope light path
17/01: First star shines for Gaia
14/01: Radiation Campaign #4
06/01: Asteroid detection by Gaia
2013
17/12: Gaia in the gantry
12/12: The sky in G magnitude
05/12: Pre-launch release of spectrophotometric standard stars
28/11: From one to one billion pixels
21/11: The Hipparcos all-sky map
15/10: Gaia Sunshield Deployment Test
08/10: Initial Gaia Source List
17/09: CU1 Operations Workshop
11/09: Apsis
26/08: Gaia arrival in French Guiana
20/08: Gaia cartoons
11/07: Model Soyuz Fregat video
01/07: Acoustic Testing
21/06: SOVT
03/06: CU4 meeting #15
04/04: DPCC (CNES) 
26/03: Gaia artist impression 
11/02: Gaia payload testing  
04/01: Space flyby with Gaia-like data
2012
10/12: DPAC OR#2. Testing with Planck
05/11: Galaxy detection with Gaia
09/10: Plot of part of the GUMS-10 catalogue
23/07: "Gaia" meets at Gaia
29/06: The Sky as seen by Gaia
31/05: Panorama of BAM clean room
29/03: GREAT school results
12/03: Scanning-law movie
21/02: Astrometric microlensing and Gaia
03/02: BAM with PMTS
12/01: FPA with all the CCDs and WFSs
2011
14/12: Deployable sunshield
10/11: Earth Trojan search
21/10: First Soyuz liftoff from the French Guiana
20/09: Fast 2D image reconstruction algorithm
05/09: RVS OMA
10/08: 3D distribution of the Gaia catalogue
13/07: Dynamical Attitude Model
22/06: Gaia's view of open clusters
27/05: Accuracy of the stellar transverse velocity
13/05: Vibration test of BAM mirrors
18/04: L. Lindegren, Dr. Honoris Causa of the Observatory of Paris
19/01: Detectability of stars close to Jupiter
05/01: Delivery of the WFS flight models
2010
21/12: The 100th member of CU3
17/11: Nano-JASMINE and AGIS
27/10: Eclipsing binary light curves fitted with DPAC code
13/10: Gaia broad band photometry
28/09: Measuring stellar parameters and interstellar extinction
14/09: M1 mirror
27/08: Quest for the Sun's siblings
 
Please note: Entries from the period 2003-2010 are available in this PDF document.