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12/04/2022

ASTRONOMY - N11: Star Clouds of the LMC

2022 April 12
The featured image shows the dark nebula N11 which
appears in the Large Magellanic Cloud -- a satellite galaxy
of our Milky Way. 
Please see the explanation for more detailed information.

N11: Star Clouds of the LMC
Image Credit: NASAESAProcessing: Josh Lake
Explanation: Massive stars, abrasive winds, mountains of dust, and energetic light sculpt one of the largest and most picturesque regions of star formation in the Local Group of Galaxies. Known as N11, the region is visible on the upper right of many images of its home galaxy, the Milky Way neighbor known as the Large Magellanic Cloud (LMC). The featured image was taken for scientific purposes by the Hubble Space Telescope and reprocessed for artistry. Although the section imaged above is known as NGC 1763, the entire N11 emission nebula is second in LMC size only to the Tarantula Nebula. Compact globules of dark dust housing emerging young stars are also visible around the image. A recent study of variable stars in the LMC with Hubble has helped to recalibrate the distance scale of the observable universe, but resulted in a slightly different scale than found using the pervasive cosmic microwave background.

10/04/2022

ASTRONOMY - Shadows at the Moon's South Pole

2022 April 10
The featured image shows the permanently shadowed
region at the Moon's South Pole. The picture is a composite
of many lunar images taken from many illumination angles 
revealing which parts are never in direct sunlight.
Please see the explanation for more detailed information.

Shadows at the Moon's South Pole
Image Credit: NASAArizona State U.Lunar Reconnaissance Orbiter

Explanation: Was this image of the Moon's surface taken with a microscope? No -- it's a multi-temporal illumination map made with a wide-angle camera. To create it, the Lunar Reconnaissance Orbiter spacecraft collected 1,700 images over a period of 6 lunar days (6 Earth months), repeatedly covering an area centered on the Moon's south pole from different angles. The resulting images were stacked to produce the featured map -- representing the percentage of time each spot on the surface was illuminated by the Sun. Remaining convincingly in shadow, the floor of the 19-kilometer diameter Shackleton crater is seen near the map's center. The lunar south pole itself is at about 9 o'clock on the crater's rim. Crater floors near the lunar south and north poles can remain in permanent shadow, while mountain tops can remain in nearly continuous sunlight. Useful for future outposts, the shadowed crater floors could offer reservoirs of water-ice, while the sunlit mountain tops offer good locations to collect solar power.

08/04/2022

ASTRONOMY - Hale-Bopp: The Great Comet of 1997

2022 April 8
See Explanation.  Clicking on the picture will download
the highest resolution version available.

Hale-Bopp: The Great Comet of 1997
Image Credit & Copyright: Stefan Seip (TWAN)

Explanation: Only twenty-five years ago, Comet Hale-Bopp rounded the Sun and offered a dazzling spectacle in planet Earth's night skies. Digitized from the original astrophoto on 35mm color slide film, this classic image of the Great Comet of 1997 was recorded a few days after its perihelion passage on April 1, 1997. Made with a camera and telephoto lens piggy-backed on a small telescope, the 10 minute long, hand-guided exposure features the memorable tails of Hale-Bopp, a whitish dust tail and blue ion tail. Here, the ion tail extends well over ten degrees across the northern sky. In all, Hale-Bopp was reported as visible to the naked eye from late May 1996 through September 1997. Also known as C/1995 O1, Hale-Bopp is recognized as one of the most compositionally pristine comets to pass through the inner Solar System. A visitor from the distant Oort cloud, the comet's next perihelion passage should be around the year 4380 AD. Do you remember Hale-Bopp?

07/04/2022

ASTRONOMY - Messier 24: Sagittarius Star Cloud

2022 April 7
See Explanation.  Clicking on the picture will download
the highest resolution version available.

Messier 24: Sagittarius Star Cloud
Image Credit & Copyright: Gabriel Rodrigues Santos
Explanation: Unlike most entries in Charles Messier's famous catalog of deep sky objects, M24 is not a bright galaxy, star cluster, or nebula. It's a gap in nearby, obscuring interstellar dust clouds that allows a view of the distant stars in the Sagittarius spiral arm of our Milky Way galaxy. When you gaze at the star cloud with binoculars or small telescope you are looking through a window over 300 light-years wide at stars some 10,000 light-years or more from Earth. Sometimes called the Small Sagittarius Star Cloud, M24's luminous stars fill this gorgeous starscape. Covering over 3 degrees or the width of 6 full moons in the constellation Sagittarius, the telescopic field of view includes dark markings B92 and B93 just above center, along with other clouds of dust and glowing nebulae toward the center of the Milky Way.

06/04/2022

ART FRACTAL - Benoit Mandelbrot

L’objet de fractale le plus connu porte le nom de Benoît Mandelbrot, inventeur du terme, en 1974.

Fractale de Mandelbrot

Ce brave monsieur avait poussé un cri de désespoir face à ses consorts qui étudiaient alors le monde grâce à la théorie des grands nombres, laissant de côté un bon nombre de phénomènes (comme la forme des nuages, des fleuves…). N’empêche qu’après sa gueulante, on s’est un peu plus intéressé aux objets bizarres s’empoussiérant jusqu’alors dans les tiroirs des mathématiciens.

Lartboratoire

ASTRONOMY - NGC 1672: Barred Spiral Galaxy from Hubble

2022 April 6
See Explanation.  Clicking on the picture will download
the highest resolution version available.

NGC 1672: Barred Spiral Galaxy from Hubble
Image Credit: Hubble Legacy ArchiveNASAESAProcessing & Copyright: Daniel Nobre

Explanation: Many spiral galaxies have bars across their centers. Even our own Milky Way Galaxy is thought to have a modest central bar. Prominently barred spiral galaxy NGC 1672, featured here, was captured in spectacular detail in an image taken by the orbiting Hubble Space Telescope. Visible are dark filamentary dust lanes, young clusters of bright blue stars, red emission nebulas of glowing hydrogen gas, a long bright bar of stars across the center, and a bright active nucleus that likely houses a supermassive black hole. Light takes about 60 million years to reach us from NGC 1672, which spans about 75,000 light years across. NGC 1672, which appears toward the constellation of the Dolphinfish (Dorado), has been studied to find out how a spiral bar contributes to star formation in a galaxy's central regions.

05/04/2022

ASTRONOMY - Seven Sisters versus California

2022 April 5
The featured image shows a wide field with the 
red California Nebula on the far left, the blue 
Pleiades Star Cluster on the right, and much brown 
interstellar dust in between. 
Please see the explanation for more detailed information.

Seven Sisters versus California
Image Credit & Copyright: Neven Krcmarek

Explanation: On the upper right, dressed in blue, is the Pleiades. Also known as the Seven Sisters and M45the Pleiades is one of the brightest and most easily visible open clusters on the sky. The Pleiades contains over 3,000 stars, is about 400 light years away, and only 13 light years across. Surrounding the stars is a spectacular blue reflection nebula made of fine dustA common legend is that one of the brighter stars faded since the cluster was named. On the lower left, shining in red, is the California Nebula. Named for its shape, the California Nebula is much dimmer and hence harder to see than the Pleiades. Also known as NGC 1499, this mass of red glowing hydrogen gas is about 1,500 light years away. Although about 25 full moons could fit between them, the featured wide angle, deep field image composite has captured them both. A careful inspection of the deep image will also reveal the star forming region IC 348 and the molecular cloud LBN 777 (the Baby Eagle Nebula).

04/04/2022

ASTRONOMY - A Vortex Aurora over Iceland

2022 April 4
The featured image depicts a bright aurora that 
occurred over Iceland in March. The curvature of the
aurora makes it look like a vortex.
Please see the explanation for more detailed information.

A Vortex Aurora over Iceland
Image Credit & Copyright: Christophe Suarez
Explanation: No, the car was not in danger of being vacuumed into space by the big sky vortex. For one reason, the vortex was really an aurora, and since auroras are created by particles striking the Earth from space, they do not create a vacuum. This rapidly developing auroral display was caused by a Coronal Mass Ejection from the Sun that passed by the Earth closely enough to cause a ripple in Earth's magnetosphere. The upper red parts of the aurora occur over 250 kilometers high with its red glow created by atmospheric atomic oxygen directly energized by incoming particles. The lower green parts of the aurora occur over 100 kilometers high with its green glow created by atmospheric atomic oxygen energized indirectly by collisions with first-energized molecular nitrogen. Below 100 kilometers, there is little atomic oxygen, which is why auroras end abruptly. The concentric cylinders depict a dramatic auroral corona as seen from the side. The featured image was created from a single 3-second exposure taken in mid-March over Lake Myvatn in Iceland.

03/04/2022

ASTRONOMY - CMB Dipole: Speeding Through the Universe

2022 April 3
The featured image depicts the cosmic microwave
background radiation as seen by the NASA's COBE mission 
over four years ending in 1993. The hot and cold dipole
pattern is indiciative of the Sun moving with respect
to this microwave light, but the cause of the motion
remains mostly unknown. 
Please see the explanation for more detailed information.

CMB Dipole: Speeding Through the Universe
Image Credit: DMRCOBENASA, Four-Year Sky Map

Explanation: Our Earth is not at rest. The Earth moves around the Sun. The Sun orbits the center of the Milky Way Galaxy. The Milky Way Galaxy orbits in the Local Group of Galaxies. The Local Group falls toward the Virgo Cluster of Galaxies. But these speeds are less than the speed that all of these objects together move relative to the cosmic microwave background radiation (CMBR). In the featured all-sky map from the COBE satellite in 1993, microwave light in the Earth's direction of motion appears blueshifted and hence hotter, while microwave light on the opposite side of the sky is redshifted and colder. The map indicates that the Local Group moves at about 600 kilometers per second relative to this primordial radiation. This high speed was initially unexpected and its magnitude is still unexplained. Why are we moving so fastWhat is out there?

02/04/2022

ASTRONOMY - Nova Scotia Northern Lights

 2022 April 2

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

Nova Scotia Northern Lights
Image Credit & CopyrightJason Dain

Explanation: This almost otherworldly display of northern lights was captured in clear skies during the early hours of March 31 from 44 degrees north latitude, planet Earth. In a five second exposure the scene looks north from Martinique Beach Provincial Park in Nova Scotia, Canada. Stars of the W-shaped constellation Cassiopeia shine well above the horizon, through the red tint of the higher altitude auroral glow. Auroral activity was anticipated by skywatchers alerted to the possibility of stormy space weather by Sun-staring spacecraft. The predicted geomagnetic storm was sparked as a coronal mass ejection, launched from prolific solar active region 2975, impacted our fair planet's magnetosphere.

ASTRONOMY - Christmas Tree Aurora

 2024 December 23 Christmas Tree Aurora Image Credit & Copyright:  Jingyi Zhang Explanation:  It was December and the sky lit up like a ...