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19/06/2024

ASTRONOMY - NGC 6188: Dragons of Ara

 2024 June 19

Gas and dust are shown in a deep starfield. The gas
glows blue and red, while the dark dust is connected in
filaments across the image. To some, the filaments appear
to have the shape of two dragons fighting. 
Please see the explanation for more detailed information.

NGC 6188: Dragons of Ara
Image Credit & Copyright: Carlos Taylor

Explanation: Do dragons fight on the altar of the sky? Although it might appear that way, these dragons are illusions made of thin gas and dust. The emission nebula NGC 6188, home to the glowing clouds, is found about 4,000 light years away near the edge of a large molecular cloud, unseen at visible wavelengths, in the southern constellation Ara (the Altar). Massive, young stars of the embedded Ara OB1 association were formed in that region only a few million years ago, sculpting the dark shapes and powering the nebular glow with stellar winds and intense ultraviolet radiation. The recent star formation itself was likely triggered by winds and supernova explosions from previous generations of massive stars, that swept up and compressed the molecular gas. This impressively detailed image spans over 2 degrees (four full Moons), corresponding to over 150 light years at the estimated distance of NGC 6188.

18/06/2024

SANTé/MEDECINE - L'anatomie du coeur humain


Le cœur comprend quatre cavités : deux oreillettes, situées dans la partie supérieure, et deux ventricules, dans la partie inférieure du cœur. Les veines caves supérieure et inférieure entrent dans l'oreillette droite, tandis que les veines pulmonaires arrivent dans l'oreillette gauche. Le sang du ventricule droit est éjecté dans les artères pulmonaires droite et gauche, tandis que le ventricule gauche éjecte le sang dans l'aorte. Le muscle cardiaque, aussi appelé myocarde, est alimenté par le réseau de vaisseaux coronariens.

© Tvanbr, DP

SANTé/MEDECINE - L'immortalité pour bientôt - L'entropie

Le processus de décomposition s'appelle l'entropie et ne fait qu'augmenter avec le temps. Certains physiciens pensent qu'elle pourrait finir par s'étendre à tous les éléments de l'univers.

©Fournis par The Daily Digest

ASTRONOMY - Gigantic Jets over Himalayan Mountains

 2024 June 18

A landscape showing a night sky over distant mountains
is shown. Lakes dot the foreground in front of the mountains.
Extending from above the mountains into the night sky are 
six bright jets. The jets are violet at the bottom but red
at the top. 
Please see the explanation for more detailed information.

Gigantic Jets over Himalayan Mountains
Image Credit & Copyright: Li Xuanhua

Explanation: Yes, but can your thunderstorm do this? Pictured here are gigantic jets shooting up from a thunderstorm last week toward the Himalayan Mountains in China and Bhutan. The composite image captured four long jets that occurred only minutes apart. Gigantic jets, documented only in this century, are a type of lightning discharge that occurs between some thunderstorms and the Earth's ionosphere high above them. They are an unusual type of lightning that is much different from regular cloud-to-cloud and cloud-to-ground lightning. The bottoms of gigantic jets appear similar to a cloud-to-above strike called blue jets, while the tops appear similar to upper-atmosphere red sprites. Although the mechanism and trigger that cause gigantic jets remains a topic of research, it is clear that the jets reduce charge imbalance between different parts of Earth's atmosphere. A good way to look for gigantic jets is to watch a powerful but distant thunderstorm from a clear location.

17/06/2024

MUSIQUE - Johann Strauss Sr. - Marche de Radetzky

"Marche de Radetzky

ASTRONOMY - Ou4: The Giant Squid Nebula

 2024 June 17


A starfield has a red nebula covering much of the frame
but in the center, extending nearly vertically, is a blue
nebula that appears shaped, to some, like a squid.
Please see the explanation for more detailed information.

Ou4: The Giant Squid Nebula
Image Credit & Copyright: Alex Linde

Explanation: Squids on Earth aren't this big. This mysterious squid-like cosmic cloud spans nearly three full moons on planet Earth's sky. Discovered in 2011 by French astro-imager Nicolas Outters, the Squid Nebula's bipolar shape is distinguished here by the telltale blue emission from doubly ionized oxygen atoms. Though apparently surrounded by the reddish hydrogen emission region Sh2-129, the true distance and nature of the Squid Nebula have been difficult to determine. Still, one investigation suggests Ou4 really does lie within Sh2-129 some 2,300 light-years away. Consistent with that scenario, the cosmic squid would represent a spectacular outflow of material driven by a triple system of hot, massive stars, cataloged as HR8119, seen near the center of the nebula. If so, this truly giant squid nebula would physically be over 50 light-years across.

16/06/2024

SANTé/MEDECINE - L'immortalité pour bientôt - La possibilité de vivre éternellement


Par conséquent, si nous parvenons à surmonter les lois de la physique qui régissent notre corps, l'immortalité pourrait être une possibilité.

©Fournis par The Daily Digest

ASTRONOMY - Animation: Black Hole Destroys Star

 2024 June 16

Animation: Black Hole Destroys Star
Video Illustration Credit: DESYScience Communication Lab

Explanation: What happens if a star gets too close to a black hole? The black hole can rip it apart -- but how? It's not the high gravitational attraction itself that's the problem -- it's the difference in gravitational pull across the star that creates the destruction. In the featured animated video illustrating this disintegration, you first see a star approaching the black hole. Increasing in orbital speed, the star's outer atmosphere is ripped away during closest approach. Much of the star's atmosphere disperses into deep space, but some continues to orbit the black hole and forms an accretion disk. The animation then takes you into the accretion disk while looking toward the black hole. Including the strange visual effects of gravitational lensing, you can even see the far side of the disk. Finally, you look along one of the jets being expelled along the spin axis. Theoretical models indicate that these jets not only expel energetic gas, but also create energetic neutrinos -- one of which may have been seen recently on Earth.

15/06/2024

SANTé/MEDECINE - Le CBD

Le potentiel du CBD est reconnu des scientifiques et apprécié des consommateurs. Le CBD peut être consommé sous des formes aussi diverses que variées : en e-liquide pour les cigarettes électroniques, en huile pour les applications cutanées, en gélules pour une prise quotidienne ou encore en fleurs pour l’incorporer dans vos recettes de cuisine favorites. Quelles que soient les méthodes d’assimilation, un spécialiste du CBD en France partage les multiples promesses de cette molécule. Entre autres : c’est un remède efficace contre le stress, l’anxiété et même les états dépressifs ;
on lui prête aussi des vertus antalgiques pour atténuer les douleurs chroniques et les courbatures ;
elle réduit l’inflammation, notamment sur le plan digestif et diminue les troubles gastro-intestinaux;
on lui attribue également des pouvoirs antioxydants qui participent au renforcement du système immunitaire.

Idéal pour contrer des effets négatifs du stress, le CBD agit beaucoup sur l’humeur permettant d’être moins irritable, de ne plus ressentir cette impression d’être submergé ou dépassé, de se sentir libéré de certaines tensions, qu’elles soient physiques ou psychologiques et enfin de mieux dormir.

ASTRONOMY - Prominences and Filaments on the Active Sun

 2024 June 15

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

Prominences and Filaments on the Active Sun
Image Credit & CopyrightSteen Søndergaard

Explanation: This colorized and sharpened image of the Sun is composed of frames recording emission from hydrogen atoms in the solar chromosphere on May 15. Approaching the maximum of solar cycle 25, a multitude of active regions and twisting, snake-like solar filaments are seen to sprawl across the surface of the active Sun. Suspend in the active regions' strong magnetic fields, the filaments of plasma lofted above the Sun's edge appear as bright solar prominences. The large prominences seen near 4 o'clock, and just before 9 o'clock around the solar limb are post flare loops from two powerful X-class solar flares that both occurred on that day. In fact, the 4 o'clock prominence is associated with the monster active region AR 3664 just rotating off the Sun's edge.

ASTRONOMY - Diamond Dust Sky Eye

2024 December 25 Diamond Dust Sky Eye Image Credit & Copyright:  Jaroslav Fous Explanation:  Why is there a huge eye in the sky?  Diamon...