Our Sun has become quite a busy place. Taken only two weeks ago, the Sun was captured sporting numerous tumultuous regions including active sunspot regions AR 2036 near the image top and AR 2036 near the center. Only four years ago the Sun was emerging from an unusually quiet Solar Minimum that had lasted for years. The above image was recorded in a single color of light called Hydrogen Alpha, inverted, and false colored. Spicules cover much of the Sun's face like a carpet. The gradual brightening towards the Sun's edges is caused by increased absorption of relatively cool solar gas and called limb darkening. Just over the Sun's edges, several filamentary prominences protrude, while prominences on the Sun's face are seen as light streaks. Possibly the most visually interesting of all are the magnetically tangled active regions containing relatively cool sunspots, seen as white dots. Currently at Solar Maximum -- the most active phase in its 11-year magnetic cycle, the Sun's twisted magnetic field is creating numerous solar "sparks" which include eruptive solar prominences, coronal mass ejections, and flares which emit clouds of particles that may impact the Earth and cause auroras. One flare two years ago released such a torrent of charged particles into the Solar System that it might have disrupted satellites and compromised power grids had it struck planet Earth.
Monday, May 5, 2014
Galaxy Cluster Magnifies Distant Supernova
Labels: Astronomy Picture, Astronomy picture of the day
How do you calibrate a huge gravitational lens? In this case the lens is the galaxy cluster Abell 383, a massive conglomeration of galaxies, hot gas, and dark matter that lies about 2.5 billion light years away (redshift z=0.187). What needs calibrating is the mass of the cluster, in particular the amount and distribution of dark matter. A new calibration technique has been tested recently that consists of waiting for supernovas of a very specific type to occur behind a galaxy cluster, and then figuring out how much the cluster must have magnified these supernovas through gravitational lensing. This technique complements other measures including computing the dark matter needed to contain internal galaxy motions, to confine cluster hot gas, and to create the gravitational lens image distortions. Pictured above from the Hubble Space Telescope, galaxy cluster A383 shows its gravitational lens capabilities on the right by highly distorting background galaxies behind the cluster center. On the left is a distant galaxy shown both before and after a recent revealing supernova. To date, calibration-quality supernovas of Type Ia have been found behind two other galaxy clusters by the Cluster Lensing And Supernova survey with Hubble (CLASH) project.
Sunday, May 4, 2014
A Scorpius Sky Spectacular
Labels: Astronomy Picture, Astronomy picture of the day
If Scorpius looked this good to the unaided eye, humans might remember it better. Scorpius more typically appears as a few bright stars in a well-known but rarely pointed out zodiacal constellation. To get a spectacular image like this, though, one needs a good camera, color filters, and a digital image processor. To bring out detail, the above image not only involved long duration exposures taken in several colors, but one exposure in a very specific red color emitted by hydrogen. The resulting image shows many breathtaking features. Vertically across the image left is part of the plane of our Milky Way Galaxy. Visible there are vast clouds of bright stars and long filaments of dark dust. Jutting out diagonally from the Milky Way in the image center are dark dust bands known as the Dark River. This river connects to several bright stars on the right that are part ofScorpius' head and claws, and include the bright star Antares. Above and right of Antares is an even brighter planet Jupiter. Numerous red emission nebulas and blue reflection nebulas are visible throughout the image.Scorpius appears prominently in southern skies after sunset during the middle of the year.
Thursday, September 26, 2013
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Magzter Digital Magazines have gained immense popularity and acceptance the world over and YOU are a great part of this success. To celebrate this phenomenon, Magzter look to give users unbelievable discounts and deals on magazines and subscriptions.
We are looking to make this a huge annual affair, with every magazine readers on Magzter. Your participation is extremely important and we are certain you will support us in this endeavour too.
Click here to get your Magazine Offers and Deals - www.magzter.com/offers.php or Visit us - www.magzter.com
About Magzter:
Magzter is the world's leading digital magazine store and newsstand provides a cloud-based service that enables readers to access magazines across all multi-platform mobile devices and tablets with more than 2,500 magazines from a wide range of publishers including back-issues, purchased individually or through subscriptions.
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Monday, April 16, 2012
The Eagle Nebula from Kitt Peak
Labels: Astronomy Picture, Astronomy picture of the day
From afar, the whole thing looks like an
Eagle.
A closer look at the
Eagle Nebula,
however, shows the
bright
region is actually a window into the center of a larger dark shell of
dust.
Through this window, a brightly-lit
workshop appears
where a whole open cluster
of stars is being formed.
In this cavity
tall pillars and
round globules of dark dust and cold
molecular gas
remain where stars are still forming.
Already visible are several young
bright blue stars
whose light and
winds are burning away and pushing back the
remaining filaments
and walls of gas and dust.
The Eagle emission nebula,
tagged M16, lies about 6500
light years away, spans about 20 light-years,
and is visible with
binoculars toward
the constellation of the Serpent
(Serpens).
This picture combines three specific emitted colors
and was taken with the
0.9-meter telescope on
Kitt Peak,
Arizona,
USA.
Sunday, April 15, 2012
Fata Morgana: A Possibly Titanic Mirage
Labels: Astronomy Picture, Astronomy picture of the day
Did this mirage help sink the Titanic?
The optical phenomenon called
Fata Morgana can make
strange shapes or a
false wall of water appear above a watery horizon.
When conditions are right, light reflecting off of cold water will be
bent by an unusual layer of warm air above to arrive at the observer from several different angles.
A conceptually comparable
mirage can make a
setting Sun appear
strangely distorted or a
distant pavement appear wet.
One hundred years ago today, such a Fata Morgana mirage
might have obscured real
icebergs from the clear view of
crew onboard the
Titanic.
Additional evidence for this
distortion hypothesis arises from the nearby vessel
SS Californian which reported sightings consistent with
Fata Morgana mirages.
The above Fata Morgana mirage was taken off the US Pacific coast in 2008.
Saturday, April 14, 2012
Six Moons of Saturn
Labels: Astronomy Picture, Astronomy picture of the day
How many moons does Saturn have?
So far 62 have
been discovered, the smallest only a fraction
of a kilometer across.
Six of its largest satellites can be seen here, though, in a sharp
Saturnian family portrait
taken on March 9.
Larger than Earth's Moon and even slightly larger than Mercury,
Titan
has a diameter of 5,150 kilometers and starts the line-up
at the lower left.
Continuing to the right across the frame are
Mimas,
Tethys, [Saturn],
Enceladus,
Dione, and
Rhea at far right.
Saturn's first known natural satellite, Titan was
discovered in 1655 by
Dutch astronomer Christiaan Huygens, while most recently the
satellite provisionally designated
S/2009 S1 was found
by the Cassini Imaging Science Team in 2009.
Tonight,
Saturn reaches opposition
in planet Earth's sky, offering
the best telescopic views of the ringed planet and moons
Friday, April 13, 2012
A Dust Devil of Mars
Labels: Astronomy Picture, Astronomy picture of the day
It was late in the northern martian spring
when the HiRISE camera onboard the Mars Reconnaissance Orbiter
spied
this local denizen.
Tracking south and east (down and right)
across the flat, dust-covered
Amazonis Planitia
the core of the
whirling dust devil is about 30 meters in diameter.
Lofting dust into the thin
martian
atmosphere, its plume
reaches more than 800 meters above the surface.
Not following the path of the dust devil, the plume is blown toward
the east by a westerly breeze.
Common in this region,
dust devils occur as the surface is heated by the Sun,
generating warm, rising air currents that begin to rotate.
Tangential
wind speeds of up to 110 kilometers per hour are reported
for
dust devils in other HiRISE images.
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