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05/02/2026

SANTé/MEDECINE - Tout savoir sur le coeur humain - 7 - La valve tricuspide


La valve auriculo-ventriculaire droite, aussi appelée valve tricuspide, est une valve cardiaque composée de trois cuspides, qui sont des lames d'endocarde. Cette valve est attachée par des cordons de collagène blanc, qui relient les cuspides à la paroi du ventricule. Quand le cœur est relâché, la valve est ouverte, puis elle se ferme quand les ventricules se contractent.

© Patrick J. Lynch, CC by-sa 2.5

ASTRONOMY - Artemis I: Flight Day 13

 2026 January 31

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

Artemis I: Flight Day 13
Image Credit: NASAArtemis I

Explanation: On flight day 13 (November 28, 2022) of the Artemis 1 mission, the Orion spacecraft reached its maximum distance from Earth. At over 430,000 kilometers from Earth, its distant retrograde orbit also puts Orion nearly 70,000 kilometers from the Moon. In the same field of view in this video frame from flight day 13, planet and large natural satellite even appear about the same apparent size from the spacecraft's perspective. On flight day 26 (December 11, 2022), the uncrewed spacecraft splashed down on its home world concluding the historic Artemis I mission. The Artemis II mission, carrying 4 astronauts around the moon and back again, will launch no earlier than February 8.

04/02/2026

ASTRONOMY - Spiral Galaxy NGC 1512: Wide Field

 2026 February 4

A spiral galaxy is shown that seems to have rings
in place of spiral arms. The outer ring is blue and filled
with stars, while the inner ring is more red. The center
has a vertical bar.
Please see the explanation for more detailed information.

Spiral Galaxy NGC 1512: Wide Field
Image Credit & Copyright: Daniel Stern

Explanation: Most galaxies don't have any rings -- why does this galaxy have three? To begin, a ring that's near NGC 1512's center -- and so hard to see here -- is the nuclear ring which glows brightly with recently formed stars. Next out is a ring of stars and dust appearing both red and blue, called, counter-intuitively, the inner ring. This inner ring connects ends of a diffuse central bar of stars that runs horizontally across the galaxy. Farthest out in this wide field image is a ragged structure that might be considered an outer ring. This outer ring appears spiral-like and is dotted with clusters of bright blue stars. All these ring structures are thought to be affected by NGC 1512's own gravitational asymmetries in a drawn-out process called secular evolution. The featured image was captured last month from a telescope at Deep Sky Chile in Chile.

03/02/2026

SANTé/MEDECINE - Tout savoir sur le coeur humain - 6 - Échocardiographie d’un cœur normal

Au centre, observez la valve de l'aorte qui empêche le sang de refluer dans le ventricule ; cette valve dite sigmoïde est composée de trois valvules en forme de pochettes. Le ventricule gauche est reconnaissable par sa paroi musculaire plus épaisse.

© Patrick J. Lynch, CC by-sa 2.5

02/02/2026

ASTRONOMY - Orion: The Running Man Nebula

2026 February 2
A complex nebula is shown that is mostly blue
and red on the left half and mostly brown on the right. 
Several bright stars are visible, and many filaments
run through, in particular on brown dust filamnents
on the image right. 
Please see the explanation for more detailed information.

Orion: The Running Man Nebula
Image Credit & Copyright: Robert G. Lyons (Robservatory)

Explanation: What part of Orion is this? Just north of the famous Orion Nebula is a picturesque star forming region in Orion's Sword that contains a lot of intricate dust -- some of which appears blue because it reflects the light of bright embedded stars. The region's popular name is the Running Man Nebula because, looked at from the right, part of the brown dust appears to be running legs. Cataloged as Sharpless 279, the reflection nebula is not only part of the constellation of Orion, but part of the greater Orion molecular cloud complex. Light from the Running Man's bright stars, including 42 Orionis, the bright star closest to the featured image center, is slowly destroying and reshaping the surrounding dust, which will likely be completely gone in about 10 million years. The nebula spans about 15 light years and lies about 1,500 light years away. 

01/02/2026

ASTRONOMY - Galle: Happy Face Crater on Mars

2026 February 1
Several craters are visible on a tan surface. 
The largest crater, on the right, has internal 
markings that make it look like a winking face
with a smile. 
Please see the explanation for more detailed information.

Galle: Happy Face Crater on Mars
Image Credit: NASAMGSMSSS

Explanation: Mars has put on a happy face. The Martian crater Galle is famous because it has internal markings that make it look like a face that is both smiling and winking. These markings were originally discovered in the 1970s in pictures taken by the Viking Orbiter. The Mars Global Surveyor (MGS) spacecraft that orbited Mars from 1996 to 2006 captured the featured picture. Happy Face Crater and its iconic features were formed by chance billions of years ago when a city-sized asteroid slammed into the Martian surface. All rocky planets and moons in our Solar System show impact craters, with the highest number of craters found on Earth's Moon and the planet MercuryEarth and Venus would show the most, though, were it not for weather and erosion

31/01/2026

SANTé/MEDECINE - Tout savoir sur le coeur humain - 5 - Vue gauche du cœur : les structures internes

Dans cette illustration, le cœur gauche est coloré en rouge et le droit en bleu, en référence aux sangs qui transitent dans leurs cavités : le cœur gauche envoie du sang riche en oxygène dans l'organisme, tandis que le cœur droit reçoit le sang pauvre en oxygène. Trois valves cardiaques sont représentées : les valves auriculo-ventriculaires et la valve du tronc pulmonaire.

© Patrick J. Lynch, CC by-sa 2.5

ASTRONOMY - NGC 1333: Stellar Nursery in Perseus

 2026 January 30

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

NGC 1333: Stellar Nursery in Perseus
Image Credit & Copyright: Robert Eder

Explanation: NGC 1333 is seen in visible light as a reflection nebula, dominated by bluish hues characteristic of starlight reflected by interstellar dust. A mere 1,000 light-years distant toward the heroic constellation Perseus, it lies at the edge of a large, star-forming molecular cloudThis telescopic close-up spans over two full moons on the sky or just over 15 light-years at the estimated distance of NGC 1333. It shows details of the dusty region along with telltale hints of contrasty red emission from Herbig-Haro objects, jets and shocked glowing gas emanating from recently formed stars. In fact, NGC 1333 contains hundreds of stars less than a million years old, most still hidden from optical telescopes by the pervasive stardust. The chaotic environment may be similar to one in which our own Sun formed over 4.5 billion years ago.

29/01/2026

ASTRONOMY - NGC 2442: Galaxy in Volans

2026 January 29
See Explanation.  Clicking on the picture will download
the highest resolution version available.

NGC 2442: Galaxy in Volans
Image Credit & CopyrightMike Selby

Explanation: Distorted galaxy NGC 2442 can be found in the southern constellation of the flying fish, (Piscis) Volans. Located about 50 million light-years away, the galaxy's two spiral arms extending from a pronounced central bar give it a hook-shaped appearance in this deep and colorful image, with foreground stars scattered across the telescopic field of view. The image also reveals the distant galaxy's obscuring dust lanes, young blue star clusters and reddish star forming regions surrounding a core of yellowish light from an older population of stars. But the star forming regions seem more concentrated along the drawn-out (upper right) spiral arm. The distorted structure is likely the result of an ancient close encounter with a smaller galaxy that lies off top left of the frame. This telescopic field of view spans over 200,000 light-years at the estimated distance of NGC 2442. 

28/01/2026

ASTRONOMY - M78: Reflecting Blue in a Sea of Red

 2026 January 28

In a starfield glowing red, several features stand
out. On the right is a diffuse white band, and on the 
upper right is some dark dust. Most prominently, though,
are two blue structures in the center, one of which has
a dark band running across near the middle. 
Please see the explanation for more detailed information.

M78: Reflecting Blue in a Sea of Red
Image Credit & Copyright: Daniel McCauley

Explanation: In the vast Orion Molecular Cloud complex, several bright blue nebulas are particularly apparent. Pictured here in the center are two of the most prominent reflection nebulas - dust clouds lit by the reflecting light of bright embedded stars. The more famous nebula is M78, in the image center, cataloged over 200 years ago. To its upper left is the lesser known NGC 2071. Astronomers continue to study these reflection nebulas to better understand how interior stars form. The overall red glow is from diffuse hydrogen gas that covers much of the Orion complex that spans much of the constellation of Orion. Nearby in the greater complex, which lies about 1,500 light years away, are the Orion Nebula, the Horsehead Nebula, and Barnard's Loop -- partially seen here as the white band on the upper left.

SANTé/MEDECINE - Tout savoir sur le coeur humain - 7 - La valve tricuspide

La valve auriculo-ventriculaire droite, aussi appelée valve tricuspide, est une valve cardiaque composée de trois cuspides, qui sont des lam...