Explanation: What would it be like to fly free in space? At about 100 meters from the cargo bay of the space shuttle Challenger, Bruce McCandless II was living the dream -- floating farther out than anyone had ever been before. Guided by a Manned Maneuvering Unit (MMU), astronaut McCandless, pictured, was floating free in space. McCandless and fellow NASA astronaut Robert Stewart were the first to experience such an "untethered space walk" during Space Shuttle mission 41-B in1984. The MMU worked by shooting jets of nitrogen and was used to help deploy and retrieve satellites. With a mass over 140 kilograms, an MMU is heavy on Earth, but, like everything, is weightless when drifting in orbit. The MMU was later replaced with the SAFER backpack propulsion unit.
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09/02/2020
28/01/2020
Science et Technologie - Santé/Médecine - L'hypnose (1/12)
Cet état est généralement provoqué chez une personne par l'action
volontaire d'une autre personne. Ce processus est parfois nommé induction hypnotique.
Il se caractérise selon les individus par une réduction du champ
de conscience (hyperfocalisation), une introspection, le développement
d'hallucinations, de rêves, un sentiment d'absence, de dissociation, une
perte des repères spatio-temporels et d'autres phénomènes variables.
L'expérience hypnotique d'une personne dépend de sa personnalité, du
contexte, de la méthode employée, des suggestions qui lui sont faites, de la profondeur de l'induction hypnotique, et d'autres paramètres.
Une personne peut également développer une hypnose spontanée ou provoquer soi-même sa propre hypnose. On parle alors d’autohypnose.
Il existe un débat ancien entre ceux qui considèrent l'hypnose
comme un état mental spécifique et ceux qui le considèrent comme un jeu
de rôle comportemental en réponse pour se conformer à une attente, ainsi
que des positions médianes.
Le mot hypnose désigne également les techniques permettant de créer cet état et les pratiques thérapeutiques utilisées pendant cet état.
14/01/2020
Science & Technologie - Image astronomique du jour : La galaxie du Sombrero en infrarouge
Cet anneau en lévitation a la taille d'une galaxie. En fait, c'est
une galaxie, du moins une partie : la galaxie du Sombrero, une des plus
grandes galaxies du proche amas de la Vierge. La bande sombre de
poussière qui en lumière visible obscurcit le plan de la Galaxie du
Sombrero se révèle brillante en infrarouge. L'image ci-dessus montre la
lueur infrarouge captée par le télescope spatial Spitzer en orbite
autour de la Terre, superposée en fausses couleurs à une autre image
prise en lumière visible par le télescope spatial Hubble de la NASA. La
Galaxie du Sombrero, connue aussi sous le nom de M 104, mesure environ
50 000 années-lumière de diamètre et est située à 28 millions
d'années-lumière de la Terre. M104 est visible à l'aide d'un petit
instrument dans la direction de la constellation de la Vierge.
09/01/2020
Science & Technology - Astronomy picture of the day : Galaxies in the River
2020 January 8
Galaxies in the River
Image Credit & Copyright: Star Shadows Remote Observatory, PROMPT, CTIO
Image Credit & Copyright: Star Shadows Remote Observatory, PROMPT, CTIO
Explanation:
Large galaxies grow by eating small ones.
Even our own galaxy engages in
a sort of galactic
cannibalism, absorbing small galaxies that are too close and
are captured by
the Milky Way's gravity.
In fact, the
practice is common
in the universe and illustrated by this striking pair of interacting
galaxies
from the banks of the southern constellation
Eridanus,
The River.
Located over 50 million light years away,
the large, distorted
spiral NGC 1532 is seen locked in a
gravitational struggle with dwarf galaxy NGC 1531 (right of center),
a struggle the smaller galaxy will
eventually lose.
Seen edge-on, spiral NGC 1532 spans about 100,000 light-years.
Nicely detailed in this sharp image, the
NGC 1532/1531 pair is thought to be similar
to the well-studied system of face-on spiral and small companion
known as M51.
02/01/2020
Science & Technology - Astronomy picture of the day : The Fainting of Betelgeuse
2020 January 2
The Fainting of Betelgeuse
Image Credit & Copyright: Jimmy Westlake (Colorado Mountain College)
Image Credit & Copyright: Jimmy Westlake (Colorado Mountain College)
Explanation:
Begirt with many a blazing star,
Orion the Hunter is one of the most recognizable
constellations.
In this
night
skyscape
the Hunter's stars rise in the northern hemisphere's winter sky
on December 30, 2019, tangled in bare trees near
Newnan, Georgia, USA.
Red super giant star Betelgeuse
stands out in yellowish hues at
Orion's shoulder left of center, but it
no longer so strongly rivals the
blue supergiant star Rigel at the Hunter's foot.
In fact, skygazers around planet Earth can see a strikingly
fainter Betelgeuse now, its brightness
fading
by more than half in the final months of 2019.
Betelgeuse has long been known to be a variable star,
changing its brightness in multiple cycles with approximate
short and long term periods of hundreds of days to many years.
The star
is now close
to its faintest since photometric measurements in 1926/27,
likely due in part to a near coincidence in the minimum of short
and long term cycles.
Betelgeuse is also
recognized as a nearby red supergiant star
that will end its life in a core collapse supernova explosion
sometime in the next 1,000 years,
though that cosmic cataclysm will take place
a safe 700 light-years or so
from
our fair planet.
01/01/2020
Science & Technology - Astronomy picture of the day : Betelgeuse Imagined
2020 January 1
Betelgeuse Imagined
Illustration Credit: ESO, L. Calcada
Illustration Credit: ESO, L. Calcada
Explanation:
Why is Betelgeuse fading?
No one knows.
Betelgeuse,
one of the brightest and
most recognized stars
in the night sky, is only
half as bright as it used to be only five months ago.
Such variability is likely just
normal behavior for this famously variable
supergiant,
but the recent dimming has rekindled discussion on how long it may be before
Betelgeuse does go supernova.
Known for its red color,
Betelgeuse is one of the few stars to be
resolved by modern telescopes, although only barely.
The
featured artist's illustration imagines how
Betelgeuse might look up close.
Betelgeuse is thought to have a
complex and
tumultuous surface that frequently throws impressive flares.
Were it to replace the Sun
(not recommended), its surface would extend out near the orbit of
Jupiter, while gas plumes would bubble out past
Neptune.
Since
Betelgeuse
is about 700 light years away,
its eventual supernova will not endanger life on Earth
even though its brightness
may rival that of a full Moon.
Astronomers -- both amateur and professional -- will surely
continue to monitor
Betelgeuse as this new decade unfolds.
24/12/2019
Science & Technology - Astronomy picture of the day : A Northern Winter Sky Panorama
Image Credit & Copyright: Tomas Slovinsky
Explanation: What stars shine in Earth's northern hemisphere during winter? The featured image highlights a number of bright stars visible earlier this month. The image is a 360-degree horizontal-composite panorama of 66 vertical frames taken consecutively with the same camera and from the same location at about 2:30 am. Famous stars visible in the picture include Castor & Pollux toward the southeast on the left, Sirius just over the horizon toward the south, Capella just over the arch of the Milky Way Galaxy toward the west, and Polaris toward the north on the right. Captured by coincidence is a meteor on the far left. In the foreground is the Museum of the Orava Village in Zuberec, Slovakia. This village recreates rural life in the region hundreds of years ago, while the image captures a timeless sky surely familar to village residents, a sky also shared with northern residents around the world.
17/12/2019
Science & Technology - Astronomy picture of the day : The Horsehead Nebula
Image Credit & Copyright: Mark Hanson & Martin Pugh, SSRO, PROMPT, CTIO, NSF
Explanation: Sculpted by stellar winds and radiation, a magnificent interstellar dust cloud by chance has assumed this recognizable shape. Fittingly named the Horsehead Nebula, it is some 1,500 light-years distant, embedded in the vast Orion cloud complex. About five light-years "tall", the dark cloud is cataloged as Barnard 33 and is visible only because its obscuring dust is silhouetted against the glowing red emission nebula IC 434. Stars are forming within the dark cloud. Contrasting blue reflection nebula NGC 2023, surrounding a hot, young star, is at the lower left of the full image. The featured gorgeous color image combines both narrowband and broadband images recorded using several different telescopes.
15/12/2019
Science & Technology - Astronomy picture of the day : Mammatus Clouds over Nebraska
Image Credit & Copyright: Jorn Olsen Photography
Explanation: When do cloud bottoms appear like bubbles? Normally, cloud bottoms are flat. This is because moist warm air that rises and cools will condense into water droplets at a specific temperature, which usually corresponds to a very specific height. As water droplets grow, an opaque cloud forms. Under some conditions, however, cloud pockets can develop that contain large droplets of water or ice that fall into clear air as they evaporate. Such pocketsmay occur in turbulent air near a thunderstorm. Resulting mammatus clouds can appear especially dramatic if sunlit from the side. The mammatus clouds pictured here were photographed over Hastings, Nebraska during 2004 June.
14/12/2019
Sience & Technology - Astronomy picture of the day : Interstellar Comet 2I/Borisov
Image Credit: NASA, ESA, and D. Jewitt (UCLA) et al.
Explanation: From somewhere else in the Milky Way galaxy, Comet 2I/Borisov is just visiting the Solar System. Discovered by Crimean amateur astronomer Gennady Borisov on August 30, 2019, the first known interstellar comet is captured in these two recent Hubble Space Telescope images. On the left, a distant background galaxy near the line-of-sight to Borisov is blurred as Hubble tracked the speeding comet and dust tail about 327 million kilometers from Earth. At right, 2I/Borisov appears shortly after perihelion, its closest approach to Sun. Borisov's closest approach to our fair planet, a distance of about 290 million kilometers, will come on December 28. Even though Hubble's sharp images don't resolve the comet's nucleus, they do lead to estimates of less than 1 kilometer for its diameter.
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