Astronomy - THE VELA SUPERNOVA REMNANT

 2026 June 2

The Vela Supernova Remnant
Image Credit & Copyright: José Mtanous

Explanation: The explosion is over, but the consequences continue. About twelve thousand years ago, a relatively normal star in the constellation Vela suddenly exploded, creating a strange point of light briefly visible to humans living near the beginning of recorded history. The outer layers of the star crashed into the interstellar medium, driving a shock wave that is still visible today. The featured image, taken piecemeal over 60 hours from the Khomas Region of Namibia, captures some of that filamentary and gigantic shock in visible light, with details highlighted by hydrogen (red) and oxygen (blue) emissions. As gas flies away from the detonated star, it decays and reacts with the interstellar medium, producing light in many different colors and energy bands. Remaining at the center of the Vela Supernova Remnant is a pulsar, a star as dense as nuclear matter that spins around more than ten times in a single second.

Astronomy - SATURN AT NIGHT

 2026 June 1

Saturn at Night
Image Credit: NASA, JPL-Caltech, Space Science Institute, Mindaugas Macijauskas

Explanation: Telescopic views of Saturn and its beautiful rings often make it the star of star parties. But this stunning view of the outer gas gaint planet's rings and night side just isn't possible from telescopes in the vicinity of planet Earth. Peering out from the inner Solar System they can only bring Saturn's day side into view. In fact, this image of Saturn's slender sunlit crescent with the planet's night shadow cast across its broad and complex ring system was captured by the robot spacecraft Cassini. After a seven year long journey from planet Earth, Cassini called Saturn orbit home for 13 years (from 2004 - 2017) before it was directed to dive into the atmosphere of the gas giant on September 15, 2017. This magnificent mosaic is composed of frames recorded by Cassini's wide-angle camera only two days before its grand final plunge. And Saturn's night will not be seen again until another spaceship from Earth calls.

Vulcanologie - SAKURAJIMA - JAPON -

Sakurajima, un des volcans les plus actifs au monde, se situe au Japon. Malgré ses éruptions terrifiantes, il offre toujours un beau paysage.

©Getty Images

Astronomy - EAGLE NEBULA PILLARS IN INFRARED FROM HUBBLE

 2026 May 31

Eagle Nebula Pillars in Infrared from Hubble
Image Credit: NASA, ESA, Hubble, HLA; Processing: Luis Romero Ventura

Explanation: Newborn stars are forming in the Eagle Nebula. They are gravitationally contracting in pillars of dense gas and dust. The intense radiation of these newly-formed bright stars is causing surrounding material to boil away. This image, taken with the Hubble Space Telescope in near infrared light, allows the viewer to see through much of the thick dust that makes the pillars opaque in visible light. The giant structures are light years in length and dubbed informally the Pillars of Creation. Associated with the open star cluster M16, the Eagle Nebula lies about 6,500 light years away. The Eagle Nebula is a satisfying target for small telescopes in a nebula-rich part of the sky toward the split constellation Serpens Cauda (the tail of the snake).

Géoglyphes - LE GEANT DE WILMINGTON EN ANGLETERRE

Le Géant de Wilmington, appelé traditionnellement Long Man, est un géoglyphe d'Angleterre tracé sur les coteaux pentus de Windover Hill dans le comté de Sussex de l'Est, sur la côte sud de l’Angleterre. C'est une silhouette humaine de presque 69 mètres de hauteur, avec une anamorphose qui donne des proportions correctes lorsque l'on regarde la figure depuis le bas de la colline. Son origine et sa date de réalisation sont inconnues.

© Cupcakekid, CC by-sa 3.0

Astronomy - SUPERMOON VERSUS MICROMOON

2026 May 30

Supermoon Versus Micromoon
Image Credit: Soumyadeep Mukherjee

Explanation: What is so micro about tonight's blue micromoon? Just after sunset, a full moon will appear slightly smaller and dimmer than usual. The reason is that the Moon's fully illuminated phase occurs within a short time of apogee - when the Moon is farthest from the Earth in its elliptical orbit. In fact, tonight's micromoon will be the farthest, smallest, and dimmest Moon this year. But tonight's micromoon is notable for yet another reason: it is also a blue moon, meaning that it is the second full moon in the same month (moon-th). Pictured here, a supermoon -- when the full moon appears near its largest -- is compared to a micromoon as photographed from Kolkata, India in May and December of 2021. Although the next micromoon occurs next month, and the next blue moon at the end of 2028, the next blue micromoon will not occur until 2053. 

Vulcanologie - POPOCATAPL (MEXIQUE)

Avec 5,458 mètres, c'est le deuxième plus grand volcan d'Amérique du nord.

©Getty Images

Astronomy - MESSIER 104

 2026 May 29

Messier 104
Image Credit: CTIO, NOIRLab, DOE, NSF, AURA;
Image Processing: T. A. Rector (U. Alaska Anchorage), D. de Martin (NSF’s NOIRLab) & M. Zamani (NSF, NOIRLab)

Explanation: A gorgeous spiral galaxy, Messier 104 is famous for its nearly edge-on profile featuring a broad ring of obscuring dust lanes. Seen in silhouette against an extensive central bulge of stars, the swath of cosmic dust lends a broad brimmed hat-like appearance to the galaxy suggesting a more popular moniker, the Sombrero Galaxy. Also known as NGC 4594, the Sombrero galaxy can be seen across the spectrum and is host to a central supermassive black hole. About 50,000 light-years across and 28 million light-years away, M104 is one of the largest galaxies at the southern edge of the Virgo Galaxy Cluster. Still, the spiky foreground stars in this field of view lie well within our own Milky Way. This broad view of the well-known galaxy was processed to reveal M104's extended halo, as well as a faint tidal stellar stream. It was captured by the Dark Energy Camera (DECam) on the Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory.

Musique - JAKUB NIEWIADOMSKI - BACH - 5 MINI-PIECES

Astronomy - NGC 1514 : THE CRYSTAL BALL NEBULA

 2026 May 28

NGC 1514: The Crystal Ball Nebula
Image Credit: International Gemini Observatory/NOIRLab/NSF/AURA; Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)
Text: Cecilia Chirenti (NASA GSFC, UMCP, CRESST II)

Explanation: What do you see in this crystal ball? The featured image shows NGC 1514, known as the Crystal Ball Nebula, observed by the Gemini North telescope on Maunakea, in Hawai'i. NGC 1514 is 1,500 light-years away and was discovered by William Herschel in 1790. This planetary nebula is formed when a star becomes a red giant and ejects its outer gas layers. The ejected shell of gas is heated up by the core of the star to temperatures hotter than the surface of our Sun: that makes the gas shine, creating beautiful images like this one. The slightly asymmetrical shape of the Crystal Ball Nebula reveals a secret: the bright star in the center has a companion. As the two stars orbit each other with a period of about nine years, they shape the gas around them. In about 10,000 - 25,000 years the nebula will be dissipated by their stellar winds.

Géoglyphes - LE CHANDELIER DE PARACAS AU PEROU

Le Chandelier de Paracas (en espagnol : el Candelabro de Paracas) est un géoglyphe à flanc de colline, à 150 mètres de la côte nord de la péninsule de Paracas, une péninsule désertique dans le sud du Pérou à près de 200 km de la capitale Lima.

Quasiment orienté nord-sud, il a la forme d'une sorte de candélabre d'environ 180 mètres de long pour une largeur de 70 mètres. Il a été réalisé en creusant des tranchées dans un sol sableux sur 50 cm de profondeur et en plaçant des pierres sur son pourtour. L'époque de construction du Chandelier n'est pas connue, pas plus que les auteurs du géoglyphe ni leurs motifs.

© Alex Zanuccoli, CC by-sa 2.0 ; abogawat, CC0

Astronomy - PK 164 + 31.1: THE HEADPHONE NEBULA

 2026 May 27

PK 164 +31.1: The Headphone Nebula
Image Credit & Copyright: Bernard Miller
Text: Keighley Rockcliffe (NASA GSFC, UMBC CSST, CRESST II)

Explanation: What is a pair of headphones doing in the sky? Today’s image features the Headphone Nebula, also known as PK 164 +31.1 or Jones-Emberson 1. This planetary nebula, the remnant of a dying Sun-like star, faintly occupies an angular region of the Lynx constellation about 1/5^th the diameter of the full moon. The red and blue-ish green colors trace hydrogen and oxygen atoms, respectively, that have been excited and ionized by the nebula's central white dwarf. The headphone shape, where two lobes of hydrogen puncture the inner region of oxygen, adds this object to a long list of oddly shaped nebulae. The morphology of such strange nebulae hint at the presence of a stellar or planetary companion, which can stir the material flowing out from the dying star. You can listen to Hubble and JWST sonifications of planetary nebulae through your very own headphones!

Astronomy - NGC 3360 AND BURCIN'S GALAXY

 2026 May 26

NGC 3660 and Burçin's Galaxy
Image Credit & Copyright: Adam Block, El Sauce Obs.

Explanation: The upper galaxy might be more photogenic, but the lower galaxy is more unusual. The galaxy up top is NGC 3660, a spiral galaxy similar to our own Milky Way galaxy in that it has several bright blue spiral arms and a central bar of stars, dust, and gas. Captured by chance in the featured deep and colorful image, surprisingly, is SN 2026cff, a supernova found just to the right of the central bar. Farther in the distance is the bottom galaxy, known informally as Burçin’s galaxy, but formally cataloged as LEDA 1000714. The center of this galaxy appears to be an old elliptical galaxy, but it is strangely surrounded by not one but two rings of stars. What created Burçin's galaxy is a mystery and remains a continuing topic of research, but it likely involves the accretion of one or more smaller galaxies.

Astronomy - THACKERAY'S GLOBULES

 2026 May 25

Thackeray's Globules
Image Credit & Copyright: John Hayes

Explanation: What are these strange space globs? Situated in rich star fields and glowing hydrogen gas, these opaque clouds of interstellar dust and gas are so large they might be able to form stars. Their home is known as IC 2944, a bright stellar nursery located about 7,600 light years away toward the constellation of the Centaur (Centaurus). The largest of these dark globules, first spotted by A. D. Thackeray in 1950 using a telescope in South Africa, is likely two separate but overlapping clouds, each more than one light-year wide. Along with other data, the featured Hubble palette image from the El Sauce Observatory in Chile, indicates that Thackeray's globules are fractured and churning as a result of intense ultraviolet radiation from young, hot stars already energizing and heating the bright emission nebula. These and similar dark globules known to be associated with other star forming regions may ultimately be dissipated by their hostile environment -- like cosmic lumps of butter in a hot frying pan.

Vulcanologie - PICO DO FOGO - (CAP-VERT)

Pico do Fogo est plus la grande montagne du Cap-Vert, avec 2829m d'altitude.

©Shutterstock

Géoglyphes - LES CELEBRES LIGNES DE NAZCA

Les géoglyphes de Nazca, encore appelés lignes de Nazca, sont de grandes figures tracées dans le désert de Nazca, dans le sud du Pérou. Réalisés pour la plupart entre -200 et 600 ap. J.-C., ils sont le fait de la civilisation Nazca, une culture pré-inca qui se développa entre 300 av. J.-C. et 800 de notre ère. On se perd en conjectures et spéculations parfois douteuses quant à la signification que ces figures avaient pour les Nazcas.

Le sol sur lequel se dessinent ces géoglyphes est couvert de cailloux que l'oxyde de fer colore en rouge. Et c'est en les ôtant, parfois sur des kilomètres, que les Nazcas ont révélé un sol gypseux grisâtre, faisant apparaître des figures réparties le long d'une ligne de 50 km reliant les villes de Nazca et de Palpa, dans la région d'Ica.

Les géoglyphes de Nazca, représentant souvent des animaux stylisés, sont parfois de simples lignes longues de plusieurs kilomètres.

© Diego Delso, CC by-sa 4.0

Astronomy - MESSIER 2

 2026 May 23

Messier 2
Image Credit: ESA/Hubble & NASA, G. Piotto et al.

Explanation: After the Crab Nebula, this giant star cluster is the second entry in 18th century astronomer Charles Messier's famous list of things that are not comets. M2 is one of the largest globular star clusters now known to roam the halo of our Milky Way galaxy. Though Messier originally described it as a nebula without stars, this stunning Hubble image resolves stars across the cluster's central 40 light-years. Its population of stars numbers close to 150,000, concentrated within a total diameter of around 175 light-years. About 55,000 light-years distant toward the constellation Aquarius, this ancient denizen of the Milky Way, also known as NGC 7089, is 13 billion years old. An extended stellar debris stream, a signature of past gravitational tidal disruption, was recently found to be associated with Messier 2.

Santé/Médecine - CANCER DU PANCREAS : SERIEUX ESPOIR

De par la capacité de ses cellules cancéreuses, qui parviennent à résister aux traitements conventionnels tels que la chimiothérapie, le cancer du pancréas demeure l’un des cancers les plus agressifs et des plus meurtriers. À l’heure actuelle, 5 ans après le diagnostic, seulement 13 % des patients sont généralement encore en vie.

Une grande avancée vient cependant d’être réalisée par une équipe de chercheurs conduite par des scientifiques du CNRS, du Centre Léon Bérard et de l'Université Claude Bernard Lyon 1. Ces derniers sont parvenus à développer un anticorps capable de bloquer l’un des mécanismes de résistance des cellules cancéreuses.

L’action de l’anticorps NP137 sur une protéine résistante

Publiée dans la revue Nature le 22 avril 2026, cette étude s’est concentrée dans un premier temps sur la façon dont certaines cellules tumorales du cancer du pancréas parvenaient à échapper aux traitements standards. Les scientifiques sont parvenus à la conclusion qu’une protéine, nommée la nétrine-1, était la principale responsable de cette résistance. Ils ont alors mis au point un anticorps, le NP137, capable de se fixer sur la protéine et d’empêcher cette dernière d’agir.

Après des essais concluants menés sur des animaux, un premier essai réalisé sur 43 adultes a montré que ceux ayant reçu cet anticorps pendant leur chimiothérapie voyaient leur taux de survie augmenter en moyenne de cinq mois, en comparaison de ceux ne l’ayant pas reçu. Un résultat pour le moins prometteur, qui doit être confirmé par d’autres essais cliniques de plus grande ampleur.

Un nouveau traitement en vue contre le cancer du pancréas ?

"Ces résultats ouvrent une option thérapeutique prometteuse pour ce cancer en forte progression, appelé à devenir la deuxième cause de mortalité par cancer d'ici les années 2030-2040, souligne le CNRS dans un communiqué publié le 22 avril 2026. À terme, cette piste thérapeutique pourrait dépasser le seul cadre du cancer du pancréas avec des applications possibles dans de nombreux autres types tumeurs qui partagent le même mécanisme de résistance".

MarieClaire

Astronomy - THE NEBULOUS REALM OF WR 134

 2026 May 22

The Nebulous Realm of WR 134
Image Credit & Copyright: Luigi Morrone and Telescope Live

Explanation: This cosmic snapshot covers a field of view over twice as wide as the full Moon within the boundaries of the high-flying constellation Cygnus. Made using astronomical narrowband filters, the image highlights the bright edge of a ring-like nebula traced by the glow of ionized hydrogen and oxygen gas. Embedded in the region's expanse of interstellar clouds, the complex, glowing arcs are sections of shells of material swept up by the wind from Wolf-Rayet star WR 134, the brightest star near image center. Distance estimates put WR 134 about 6,000 light-years away, making this telescopic frame over 100 light-years across. Shedding their outer envelopes in powerful stellar winds, massive Wolf-Rayet stars have burned through their nuclear fuel at a prodigious rate and end their final phase of massive star evolution in a spectacular supernova. Their stellar winds and final supernova explosion enrich the interstellar material with heavy elements to be incorporated in future generations of stars.

Vulcanologie - PACAYA - GUATEMALA

Le Pacaya très beau volcan à 50km au sud de la capitale du Guatemala.

©Shutterstock