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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174. Proper motion anomalies
A fascinating subset of astrometric binaries
A subset of astrometric binaries evaded identification by Hipparcos, but they become recognisable from the difference in the proper motion determined by Hipparcos and that measured by Gaia. Recent work on these `proper motion anomalies' has underlined their ubiquity, and their scientific importance.
29 April 2024
173. The breathing motion of spiral arms
New insights into the dynamics and origin of spiral arms
In essay 114, I looked at advances being made in understanding our Galaxy's spiral arm structure. Here I will look at some remarkable insights into their kinematics. Gaia is providing confirmation of their `breathing modes' which, in turn, support some of the theoretical and numerical models being developed to understand their origin.
22 April 2024
172. The basic angle
Why was the basic angle 58 degrees for Hipparcos, and 106.5 degrees for Gaia?
For Hipparcos and Gaia, the `basic angle' is the angle between the instrument's two viewing directions on the sky. For Hipparcos, the basic angle was 58 degrees. For Gaia it is 106.5 degrees. What is the reason for the two fields of view in the first place? How is the angle between them chosen? And why is it so different for Hipparcos and Gaia?
15 April 2024
171. The Small Magellanic Cloud
A radically new view of one of our nearest neighbours
The Large and Small Magellanic Clouds are two of our nearest galaxy neighbours. The line-of-sight structure of the SMC is particularly complex, and the wealth of observational data has proven difficult to interpret. A recent study using Gaia DR3 suggests a radically new picture: that the SMC is composed of two distinct superimposed structures.
8 April 2024
170. Metrication in the UK
Some thoughts on the UK's move to the metric system
Metrication concerns the move from the historical use of feet and inches, of pounds and ounces, and of pints and gallons, to the coherent metric system in which units are inter-related. The UK's resistance to full adoption of the metric system, used by almost all other countries, has left society confused, and at an economic disadvantage.
1 April 2024
169. A billion radial velocities
A new catalogue of 125 million radial velocities
Gaia Data Release 3 includes 33 million radial velocities, obtained from its Radial Velocity Spectrometer, ten times as many as previously known. DR4, in 2025, should include some 100 million. A recent study has derived 125 million from the low-resolution BP/RP spectra, albeit of much lower accuracy, with perhaps 1–2 billion coming available in the future.
25 March 2024
168. S stars in the Wesenheit diagram
A powerful way of classifying AGB stars
S stars are cool luminous giants, lying between the O-rich M-type giants and the C-rich carbon stars on the AGB. With atmospheres enriched with s-process elements brought to the surface through the `third dredge-up', they have created around half the atomic nuclei heavier than iron. Gaia astrometry and photometry is advancing their understanding.
18 March 2024
167. Carbon stars
New insights into this important class of complex star
Carbon stars, which reside on the asymptotic giant branch, are an important phase of stellar evolution. Their very high luminosities makes them important for integrated light studies of galaxies, and they are being considered as potential standard distance indicators. Their large distances and complex physics provide numerous challenges for theoretical modelling.
11 March 2024
166. Hypervelocity stars: part 2
An update on hypervelocity stars
In essay 22 (May 2021) I described some of the early insights that Gaia was providing in the field of hypervelocity stars, a rare and exotic type of star, racing through our Galaxy with velocities of 500-1000 km per second or more. Here, I bring the Gaia results up-to-date, describing the latest searches, and more recent insights into their origin.
4 March 2024
165. Runaway stars
How these high velocity stars originate
Runaway stars are stars with such high space velocities that they must have been imparted by a particular formation process. Many insights into the favoured scenarios - binary-supernova and dynamical ejection - are being made as Gaia's astrometry yields their accurate distances and space motions.
26 February 2024
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