MICROPHOTOGRAPHIE - Écailles de serpent ou dendrites métalliques ?

Gros plan ici sur quelques écailles de serpents, pourrait-on penser. Ou sur l'écorce rugueuse d'un morceau de bois. Mais une fois encore, nous aurions tout faux.

Cette microphotographie révèle la surface d'une ouverture de faisceau d'ions gravée par des ions d'argon à incidence oblique dans un système d'amincissement par faisceau d'ions. Dans de tels systèmes, des échantillons de matériaux très minces sont générés. Ils sont transparents aux électrons à haute vitesse dans les microscopes électroniques à transmission modernes.

Les images connues de structures à résolution atomique proviennent généralement d'une telle préparation d'échantillon et sont principalement des piles d'atomes individuels orientées verticalement.

FuturaSciences

ASTRONOMY - To Fly Free in Space

 2026 February 15

To Fly Free in Space
Image Credit: NASA, STS-41B

Explanation: What would it be like to fly free in space? About 100 meters from the cargo bay of a space shuttle, Bruce McCandless II was living the dream -- floating farther out than anyone had ever been before. Guided by a Manned Maneuvering Unit (MMU), astronaut McCandless, pictured, was floating free in space. During Space Shuttle mission 41-B in 1984, McCandless and fellow NASA astronaut Robert Stewart were the first to experience such an "untethered space walk". The MMU worked by shooting jets of nitrogen and was used to help deploy and retrieve satellites. With a mass over 140 kilograms, an MMU is heavy on Earth, but, like everything, is weightless when drifting in orbit. The MMU was later replaced with the SAFER backpack propulsion unit.

ASTRONOMY - Red Spider Planetary Nebula from Webb

 2026 February 3

Red Spider Planetary Nebula from Webb
Image Credit: ESA/Webb, NASA & CSA, J. H. Kastner (RIT)

Explanation: Oh what a tangled web a planetary nebula can weave. The Red Spider Planetary Nebula shows the complex structure that can result when a normal star ejects its outer gases and becomes a white dwarf star. Officially tagged NGC 6537, this two-lobed symmetric planetary nebula houses one of the hottest white dwarfs ever observed, probably as part of a binary star system. Internal winds flowing out from the central stars, have been measured in excess of 1,000 kilometers per second. These winds expand the nebula, flow along the nebula's walls, and cause waves of hot gas and dust to collide. Atoms caught in these colliding shocks radiate light shown in the featured false-color infrared picture by the James Webb Space Telescope. The Red Spider Nebula lies toward the constellation of the Archer (Sagittarius). Its distance is not well known but has been estimated by some to be about 4,000 light-years.

SANTé/MEDECINE - Tout savoir sur le coeur - 11 - Opérations du cœur

À gauche, la valve mitrale a été remplacée par une valve artificielle. Cette opération est souvent nécessaire en cas de malformation de la valve auriculo-ventriculaire ou suite à une insuffisance valvulaire (défaut de fermeture de la valve). À droite, un pontage coronarien permet de contourner une artère coronaire bouchée et d'apporter du sang riche en oxygène au muscle cardiaque, grâce à un vaisseau greffé. Ce vaisseau greffé provient souvent de la jambe.

© 2018 Patrick Lynch

ASTRONOMY -The Bay of Rainbows

 2026 February 12

The Bay of Rainbows
Image Credit & Copyright: Olaf Filzinger

Explanation: Dark, smooth regions that cover the Moon's familiar face are called by Latin names for oceans and seas. That naming convention is historical, though it may seem a little ironic to denizens of the space age who recognize the Moon as a mostly dry and airless world, and the smooth, dark areas as lava-flooded impact basins. For example, this telescopic lunar vista, looks over the expanse of the northwestern Mare Imbrium, or Sea of Rains and into the Sinus Iridum, the Bay of Rainbows. Ringed by the Jura Mountains (montes), the bay is about 250 kilometers across. Seen after local sunrise, the mountains form part of the Sinus Iridum impact crater wall. Their rugged sunlit arc is bounded at the top by Cape (promontorium) Laplace reaching nearly 3,000 meters above the bay's surface. At the bottom of the arc is Cape Heraclides, depicted by Giovanni Cassini in his 1679 telescope-based drawings mapping the moon, as a moon maiden seen in profile with long, flowing hair.

SANTé/MEDECINE - Tout savoir sur le coeur humain - 10 - Infarctus dans le ventricule gauche

Si une artère coronaire est obstruée, l'irrigation du myocarde en sang diminue localement. Les cellules musculaires manquent d'oxygène et sont affaiblies. Si la situation se prolonge, elle risque de provoquer un infarctus du myocarde, ou crise cardiaque. Certaines régions du muscle cardiaque sont nécrosées : elles sont colorées en sombre en bas de l'illustration. Plus les lésions sont étendues, plus les chances de survie sont minces.

© Patrick J. Lynch, CC by-sa 2.5

ASTRONOMY - A Year of Sunspots

 2026 February 11

A Year of Sunspots
Image Credit: NASA, SDO; Processing & Copyright: Şenol Şanli & Uğur İkizler; Text: Cecilia Chirenti (NASA GSFC, UMCP, CRESST II)

Explanation: How many sunspots can you see? The central image shows the many sunspots that occurred in 2025, month by month around the circle, and all together in the grand central image. Each sunspot is magnetically cooled and so appears dark -- and can last from days to months. Although the featured images originated from NASA's Solar Dynamics Observatory, sunspots can be easily seen with a small telescope or binoculars equipped with a solar filter. Very large sunspot groups like recent AR 4366 can even be seen with eclipse glasses. Sunspots are still counted by eye, but the total number is not considered exact because they frequently change and break up. Last year, 2025, coincided with a solar maximum, the period of most intense magnetic activity during its 11-year solar cycle. Our Sun remains unpredictable in many ways, including when it ejects solar flares that will impact the Earth, and how active the next solar cycle will be.

ASTRONOMY - In Green Company: Aurora over Norway

 2026 February 10

In Green Company: Aurora over Norway
Image Credit & Copyright: Max Rive

Explanation: Raise your arms if you see an aurora. With those instructions, two nights went by with, well, clouds -- mostly. On the third night of returning to same peaks, though, the sky not only cleared up but lit up with a spectacular auroral display. Arms went high in the air, patience and experience paid off, and the creative featured image was captured as a composite from three separate exposures. The setting is a summit of the Austnesfjorden (a fjord) close to the town of Svolvear on the Lofoten islands in northern Norway. The year was 2014. This year, our Sun is just passing solar maximum, the peak in its 11-year surface activity cycle. As expected, some spectacular auroras have recently resulted.

ASTRONOMY - Miranda Revisited

 2026 February 9

Miranda Revisited
Image Credit: NASA, JPL, Voyager 2; Processing & License: Flickr: zelario12; Text: Keighley Rockcliffe (NASA GSFC, UMBC CSST, CRESST II)

Explanation: What is Miranda really like? Visually, old images from NASA's Voyager 2 have been recently combined and remastered to result in the featured image of Uranus's 500-kilometer-wide moon. In the late 1980s, Voyager 2 flew by Uranus, coming close to the cratered, fractured, and unusually grooved moon -- named after a character from Shakespeare’s The Tempest. Scientifically, planetary scientists are using old data and clear images to theorize anew about what shaped Miranda's severe surface features. A leading hypothesis is that Miranda, beneath its icy surface, may have once hosted an expansive liquid water ocean which may be slowly freezing. Thanks to the legacy of Voyager 2, Miranda has joined the ranks of Europa, Titan, and other icy moons in the search for water, and, possibly, microbial life, in our Solar System.

SANTé/MEDECINE - Tout savoir sur le coeur humain - 9 - Pseudo-anévrisme du ventricule gauche

Un pseudo-anévrisme, aussi appelé faux anévrisme, est une poche de sang qui se forme près du myocarde. Contrairement aux vrais anévrismes, il ne possède pas d'éléments du myocarde, mais risque de se rompre. Les pseudo-anévrismes du ventricule gauche sont rares, mais il s'agit souvent d'une complication d'un infarctus du myocarde. Ils peuvent aussi survenir après une opération cardiaque ou une infection.

© Patrick J. Lynch, CC by-sa 2.5