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Gaia: science essays

In these short (mostly 2-page, weekly) 'essays', I have picked out some of the scientific highlights of the Gaia mission as they are emerging, or as they caught my attention. They offer a somewhat chronological snapshot of some of the discoveries that Gaia is making across all of astronomy. I've also included some essays on related topics, including the history of astrometry, and some more technical, managerial, or developmental aspects of both the Hipparcos and Gaia missions. In each, I have included a footnote DR1, DR2, EDR3, DR3, etc to indicate which of the (latest) data releases the essay refers to (described in essays #10 and #76), with DR0 signifying technical or historical material not connected with any specific data release. Who are they written for?  Anyone who might have a general interest in science and astronomy, including amateur astronomers, young scientists starting out on their careers, mid-career scientists looking in on Gaia for the first time to get a feeling of what is possible, and specialists looking in from different areas of astronomy, or physics more generally. Click on the access PDF icon to access the file. Only a few references are included, and these are 'discreetly' hyperlinked for those who want to read more... where references appear in the form (Einstein 1908) or www.gaia.com, clicking on the text (even though generally not highlighted!) should lead to the relevant online article. Essays 1-236 were published weekly, 237-241 monthly, and 242 onwards every two weeks.​ In a few cases, I've recorded an interview on the subject (see science interview page).

New: This table page lists all essays, updated to the end of June 2026 (1–235 inclusive), in tabular form. It includes a simple search on the title field.

New: These annual compilations are in both pdf and 'flipbook' form (open in new page; larger files as a download):

pdf:​

flipbook:

 

New: The material in essays 1–239 is broadly included in my review "Space astrometry with Gaia: Advances in understanding our Galaxy" published in Physics Reports, Volume 1150, pp. 1–229 (January 2026): available here

New: This Gaia Science Tree (v4.0, June 2026) presents essays 1–235 (Jan 2021–Jun 2026) as a hyperlinked "mind map"

* all end-nodes are hyperlinked to the given essay number (links are to "legacy" copies at the CERN-Zenodo site)
* catalogue content topics are at top right, background material at bottom left, otherwise moving "outwards" clockwise in the diagram
* I have prepared this as a didactic tool. Please feel free to make use of it as you wish

I have converted Essays 1–130 into audio "discussion-type" podcasts, entirely using generative AI. They are available at my Gaia Essay YouTube channel, and I describe their construction in Essay 227.

Please make use of this subscribe page to receive an email (usually Monday) when each new essay is published

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94. The mass of the Local Group

The sum of all our neighbours

I look at the latest estimates of the total mass of our Local Group of galaxies. These take into account increasingly subtle effects related to their detailed dynamics, many being clarified by Gaia. And they must also be consistent with the increasingly detailed predictions of numerical models of the formation and evolution of structure in the Universe.

17 October 2022

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93. The mass of the Milky Way

Why it's so difficult to measure

What is the mass of our Milky Way galaxy? Why is it important to know? Why is it so difficult to measure? And what is Gaia contributing to our knowledge? Here, I take a look at the Gaia-related papers that have been trying to tackle this problem, and see why the Galaxy halo still resists our attempts to fully characterise it.

10 October 2022

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92. Diffuse interstellar bands

A slowly advancing mystery

Diffuse interstellar bands, or DIBs, comprise some 600 known absorption features widely observed in stellar spectra. Known for more than a century, only one has been securely identified. Nearly half a million sources show the 862 nm DIB in their Gaia spectra, providing new insight into interstellar absorption.

3 October 2022

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91. Cerium and the Galaxy infall history

Its use in Galactic archaeology

As one of the developments in Galactic archaeology being enabled by Gaia, I will explain what cerium is, why it is relevant to astronomy, how it is measured by Gaia, and what its occurrence tells us about the formation, and in particular the complex infall history, of our Galaxy.

26 September 2022

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90. Astrophysics of our Galaxy

Examples of Gaia's astrophysical parameters

I continue with the subject of my previous essay, and give some examples of the way in which the derived astrophysical data are providing new insights in understanding the structure, formation, and evolution of huge numbers of stars in our Galaxy. They give just a flavour of what Gaia is providing.

19 September 2022

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89. A revolution in stellar astrophysics

How the astrophysical parameters are derived

The recently published Data Release 3 includes a wealth of `extracted' astrophysical data, of staggering extent, including stellar spectroscopic and evolutionary parameters for up to 470 million sources. A dozen refereed papers detail the underlying computations. Here, I provide a synopsis of the methods, and results.

12 September 2022

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88. Pinpointing exoplanets

Some other areas where Gaia assists

Continuing with the study of exoplanets, I focus here on three areas where Gaia is helping to vet, and to pinpoint, these other worlds: rejecting false positives from transit searches, establishing masses from radial velocity minimum estimates, and identifying accelerating systems for imaging searches.

5 September 2022

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87. Radial velocities: results from DR3

First science with RVS

Gaia Data Release 3 provides radial velocities for more than 33 million stars down to about 14 mag. Here I look at some of the first scientific results from these radial velocities: their distribution across our Galaxy, their high-velocity star content, and their distribution in the globular cluster 47 Tuc.

29 August 2022

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86. Radial velocities: their acquisition

How are radial velocities measured

Of the 1.8 billion sources in Gaia Data Release 3, more than 33 million have published radial velocities. More than 100 million are expected in DR4. I describe how the radial velocities are acquired on board, how they are processed, and the additional data that is being extracted from the spectra.

22 August 2022

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85. Radial velocities: what wavelength?

The wavelength choice for radial velocities

I look back to the period leading up to the selection of Gaia in 2000, and recall why the decision was made to acquire radial velocity observations on-board the satellite itself. And I recall the various considerations which influenced the choice of spectral range chosen for the Gaia radial velocity spectrometer.

15 August 2022

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