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01/11/2024

ASTRONOMY -Spiral Galaxy NGC 6744

2024 November 1
See Explanation.  Clicking on the picture will download
the highest resolution version available.

Spiral Galaxy NGC 6744
Image Credit & CopyrightJohn Hayes

Explanation: Big, beautiful spiral galaxy NGC 6744 is nearly 175,000 light-years across, larger than our own Milky Way. It lies some 30 million light-years distant in the southern constellation Pavo but appears as only a faint smudge in the eyepiece of a small telescope. We see the disk of the nearby island universe tilted towards our line of sight in this remarkably deep and detailed galaxy portrait, a telescopic image that spans an area about the angular size of a full moon. In it, the giant galaxy's elongated yellowish core is dominated by the light from old, cool stars. Beyond the core, grand spiral arms are filled with young blue star clusters and speckled with pinkish star forming regions. An extended arm sweeps past smaller satellite galaxy NGC 6744A at the upper left. NGC 6744's galactic companion is reminiscent of the Milky Way's satellite galaxy the Large Magellanic Cloud

31/10/2024

VILLES BIONIQUES DU FUTUR - Lilypad : une ville flottante pour des mers qui montent


Prototype d'une cité amphibie, Lilypad pourrait abriter 50.000 personnes, par exemple les habitants de la côte rognée par la montée des eaux ou les réfugiés climatiques ultramarins qui auront dû abandonner leurs îles natales. Elle comporte un lagon central d'eau douce venue de la pluie. Trois marinas et trois montagnes sont dédiées, respectivement, au travail, au commerce et aux loisirs.

© Vincent Callebaut

ASTRONOMY - Rigel and the Witch Head Nebula

2024 October 31
See Explanation.  Clicking on the picture will download
the highest resolution version available.

Rigel and the Witch Head Nebula
Image Credit & CopyrightSimone Curzi

Explanation: By starlight, this eerie visage shines in the dark with a crooked profile evoking its popular name, the Witch Head Nebula. In fact, this entrancing telescopic portrait gives the impression that a witch has fixed her gaze on Orion's bright supergiant star Rigel. More formally known as IC 2118, the Witch Head Nebula spans about 50 light-years and is composed of interstellar dust grains reflecting Rigel's starlight. The color of the Witch Head Nebula is caused not only by Rigel's intense blue light, but because the dust grains scatter blue light more efficiently than red. The same physical process causes Earth's daytime sky to appear blue, although the scatterers in Earth's atmosphere are molecules of nitrogen and oxygen. Rigel and this dusty cosmic crone are about 800 light-years away. You may still see a few witches in your neighborhood tonight though, so have a safe and Happy Halloween! 

30/10/2024

VILLES BIONIQUES DU FUTUR - Physalia : un vaisseau-amiral pour la bataille de l’eau


Au forum mondial de l'eau qui s'est tenu à Istanbul en 2009, un consensus s'est fait autour de l'impérieuse nécessité d'accorder des moyens lourds pour que chaque être humain ait accès à l'eau potable. Un milliard de personnes en manquent mais bien peu est fait. Ce navire en forme de Physalie (un curieux animal cousin des coraux et des méduses), ce « morceau de terre vivante », selon Vincent Callebaut, est un projet pour promouvoir la bonne gestion de l'eau et des voies navigables.

© Vincent Callebaut

ASTRONOMY - NGC 7635: The Bubble Nebula

 2024 October 30

A starfield is shown with a big light bubble in 
the center. A bright star is toward the upper right in
the translucent bubble. To some, the bubble may resemble
a skull.
Please see the explanation for more detailed information.

NGC 7635: The Bubble Nebula
Credit & Copyright: Chad Leader

Explanation: What created this huge space bubble? Blown by the wind from a star, this tantalizing, head-like apparition is cataloged as NGC 7635, but known simply as the Bubble Nebula. The featured striking view utilizes a long exposure to reveal the intricate details of this cosmic bubble and its environment. Although it looks delicate, the 10 light-year diameter bubble offers evidence of violent processes at work. Seen here above and right of the Bubble's center, a bright hot star is embedded in the nebula's reflecting dust. A fierce stellar wind and intense radiation from the star, which likely has a mass 10 to 20 times that of the Sun, has blasted out the structure of glowing gas against denser material in a surrounding molecular cloud. The intriguing Bubble Nebula lies a mere 11,000 light-years away toward the boastful constellation Cassiopeia.

29/10/2024

MUSIC - Jean-Sébastien Bach - Magnificat - (Jordi Savall)

"Magnificat"

LES NUAGES DIEUX DU CIEL - La formation du nuage lenticulaire


L'altocumulus lenticularis, ou nuage lenticulaire, est un nuage stationnaire, en forme de profil d'aile d'avion, qui se forme sous le vent des montagnes, signant la présence d'un ressaut ou onde. En réalité, il se forme en permanence du côté du vent et se dissout de l'autre côté, réalisant un nuage stationnaire contrastant avec un vent fort. Il se trouve souvent en empilements de plusieurs exemplaires formant une pile d'assiettes. Il est apprécié des vélivoles (ceux qui pratiquent le vol à voile) car il montre la présence d'une ascendance stable et puissante. Il est parfois cité par les sceptiques comme un stimulus possible à l'origine de visions d'ovnis. Cependant, il semblerait qu'à l'heure actuelle aucun cas de la casuistique ufologique de ce type n'ait été identifié avec certitude.

Texte d'après Wikipédia © DR

ASTRONOMY - NGC 602: Stars Versus Pillars from Webb

2024 October 29
A starfield is shown featuring many stars in the center
and many pillars of interstellar dust around the edges
pointing toward the center. The main image is in infrared
light, and a rollover image from Hubble shows the same
scene in visible light.
Please see the explanation for more detailed information.

NGC 602: Stars Versus Pillars from Webb
Credit: ESA/WebbNASA & CSAP. ZeidlerE. SabbiA. NotaM. Zamani (ESA/Webb)

Explanation: The stars are destroying the pillars. More specifically, some of the newly formed stars in the image center are emitting light so energetic that is evaporating the gas and dust in the surrounding pillars. Simultaneously, the pillars themselves are still trying to form new stars. The whole setting is the star cluster NGC 602, and this new vista was taken by the Webb Space Telescope in multiple infrared colors. In comparison, a roll-over image shows the same star cluster in visible light, taken previously by the Hubble Space Telescope. NGC 602 is located near the perimeter of the Small Magellanic Cloud (SMC), a small satellite galaxy of our Milky Way galaxy. At the estimated distance of the SMC, the featured picture spans about 200 light-years. A tantalizing assortment of background galaxies are also visible -- mostly around the edges -- that are at least hundreds of millions of light-years beyond. 

28/10/2024

VILLES BIONIQUES DU FUTUR - Coral Reef : un nouveau village pour Haïti


Après tous les désastres sismiques, Haïti est à reconstruire et le projet Coral Reef a pour objectif de bâtir un millier de logements préfabriqués en bord de mer, autonomes en énergie. À partir d'un module unique, l'ensemble prend la forme de deux vagues, inspirées des récifs coralliens, ménageant un espace central qui abrite un milieu naturel.

© Vincent Callebaut

ASTRONOMY - A Glowing River over France

 2024 October 28

A night sky is shown with a bright red band running
overhead. Above the red band is a diffuse red glow.
A path through a grassy filed is in the foreground
with a path going out toward the horizon. 
Please see the explanation for more detailed information.

STEVE: A Glowing River over France
Credit & Copyright: Louis LEROUX-GÉRÉ

Explanation: Sometimes a river of hot gas flows over your head. In this case the river created a Strong Thermal Emission Velocity Enhancement (STEVE) that glowed bright red, white, and pink. Details of how STEVEs work remain a topic of research, but recent evidence holds that their glow results from a fast-moving river of hot ions flowing over a hundred kilometers up in the Earth's atmosphere: the ionosphere. The more expansive dull red glow might be related to the flowing STEVE, but alternatively might be a Stable Auroral Red (SAR) arc, a more general heat-related glow. The featured picture, taken earlier this month in Côte d'OpaleFrance, is a wide-angle digital composite made as the STEVE arc formed nearly overhead. Although the apparition lasted only a few minutes, this was long enough for the quick-thinking astrophotographer to get in the picture -- can you find him?

METEOROLOGIE - Ciel de feu à Barcelone

Ce ciel de feu spectaculaire a été pris en photo à Barcelone en Espagne : on peut y voir des nuages lenticulaires très bien formés, par l&...