La Guinée-Bissau est un petit pays en Afrique occidentale. Des différences sédimentaires complexes peuvent être vues dans les eaux peu profondes le long de son littoral, où la vase portée par le fleuve Geba et d'autres fleuves plonge dans l'océan Atlantique.
Explanation:
Blown by fast winds from a hot, massive star, this
cosmic bubble is much larger than the dolphin it appears to be.
Cataloged as
Sharpless 2-308
it lies some 5,200 light-years away toward the constellation of
the Big Dog
(Canis Major)
and covers slightly more of the sky than a
Full Moon.
That corresponds to a diameter of 60
light-years at its estimated distance.
The massive star that created the bubble, a
Wolf-Rayet
star, is the bright one near the center of the nebula.
Wolf-Rayet
stars have over 20 times the mass of the
Sun and are thought to be in a brief,
pre-supernova phase of massive
star evolution.
Fast winds from this
Wolf-Rayet
star create the bubble-shaped nebula as they
sweep up slower moving material from an earlier phase of evolution.
The windblown nebula has an age of about
70,000
years.
Relatively faint emission captured in the
featured expansive image
is dominated by the glow of ionized oxygen atoms
mapped to a blue hue.
Explanation:
What created this unusual hole in Mars?
The hole was discovered by chance in 2011 on images of the dusty slopes of Mars'
Pavonis Mons volcano taken by the
HiRISE instrument aboard the robotic
Mars Reconnaissance Orbiter currently circling Mars.
The hole, shown in representative color, appears to be an opening to an underground cavern, partly illuminated on the image right.
Analysis of this and follow-up images revealed the
opening to be about 35 meters across, while the interior
shadow angle indicates that the underlying cavern is roughly 20 meters deep.
Why there is a circular crater surrounding this hole remains a topic of
speculation,
as is the full extent of the underlying cavern.
Holes such as
this are of particular interest because their interior caves are relatively protected from the harsh surface of
Mars,
making them relatively good candidates to
contain Martian life.
These pits are therefore prime targets for
possible future spacecraft, robots, and even
human interplanetary explorers.
L'hypnose est un état psychologique particulier encore mal défini
qui revêt certains attributs physiologiques et marqué par le
fonctionnement de l'individu à un niveau d'attention autre que l'état de
conscience ordinaire. Il peut, sous certaines conditions, donner l'apparence du sommeil ou du somnambulisme sans en partager toutes les caractéristiques.
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.
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.
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.
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.
Betelgeuse Imagined 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.