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Εργαλεία Θεμάτων Τρόποι εμφάνισης
  #3646  
Παλιά 17-10-16, 09:34
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Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

17 October 2016



An Atlas V Rocket Launches OSIRIS-REx

Video Credit & Copyright: United Launch Alliance, NASA

Explanation: Have you ever seen a rocket launched into the Solar System? Last month a large Atlas V rocket blasted off from Launch Complex 41 in Florida carrying the ORISIX-REx spacecraft. This robotic spacecraft will attempt to land on Asteroid Bennu and return some of its soil to Earth. Asteroid 101955 Bennu orbits the Sun near the Earth, spans about 500-meters, is dark because its surface is covered with carbon, and has about a 1 in 2500 chance of striking the Earth in the next few thousand years. The exciting 2.5-minute video shows the Atlas V rocket being rolled out, prepared, and launched -- complete with a clip of side-boosters separating. If things go according to plan, ORISIS-REx will reach Bennu in 2018 and return samples to Earth in 2023. One science goal of OSIRIS-REx is to better determine whether ancient collisions between Earth and carbonaceous asteroids like Bennu provided Earth with a significant amount of the water and organic molecules necessary for the development of life.

Free Download: APOD 2017 Calendar: NASA Images

Tomorrow's picture: galaxies galore


ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3647  
Παλιά 18-10-16, 09:36
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Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

18 October 2016



The Antlia Cluster of Galaxies

Image Credit & Copyright: Rolf Olsen
Explanation: Galaxies dot the sky in this impressively wide and deep image of the Antlia Cluster. The third closest cluster of galaxies to Earth after Virgo and Fornax, the Antlia cluster is known for its compactness and its high fraction of elliptical galaxies over (spirals. Antlia, cataloged as Abell S0636, spans about 2 million light years and lies about 130 million light years away toward the constellation of the Air Pump (Antlia). The cluster has two prominent galaxy groups - bottom center and upper left -- among its over 200 galactic members, but no single central dominant galaxy. The vertical red ribbon of gas on the left is thought related to the foreground Antlia supernova remnant and not associated with the cluster. The featured image composite, taken from New Zealand, resulted from 150+ hours of exposures taken over six months.

Tomorrow's picture: star sisters


ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3648  
Παλιά 19-10-16, 09:15
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Astronomy Picture of the Day

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19 October 2016



M45: The Pleiades Star Cluster

Image Credit & Copyright: Hermann von Eiff

Explanation: Have you ever seen the Pleiades star cluster? Even if you have, you probably have never seen it as dusty as this. Perhaps the most famous star cluster on the sky, the bright stars of the Pleiades can be seen without binoculars even from the heart of a light-polluted city. With a long exposure from a dark location, though, the dust cloud surrounding the Pleiades star cluster becomes very evident. The featured image was a long duration exposure taken last month from Namibia and covers a sky area many times the size of the full moon. Also known as the Seven Sisters and M45, the Pleiades lies about 400 light years away toward the constellation of the Bull (Taurus). A common legend with a modern twist is that one of the brighter stars faded since the cluster was named, leaving only six stars visible to the unaided eye. The actual number of visible Pleiades stars, however, may be more or less than seven, depending on the darkness of the surrounding sky and the clarity of the observer's eyesight.

Updates: ESA's ExoMars arrives at Mars today
APOD Retrospective: The Pleiades Star Cluster

Tomorrow's picture: pixels in space


ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3649  
Παλιά 20-10-16, 18:09
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Astronomy Picture of the Day

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20 October 2016



The Tulip in the Swan

Image Credit & Copyright: Martin Pugh

Explanation: Framing a bright emission region this telescopic view looks out along the plane of our Milky Way Galaxy toward the nebula rich constellation Cygnus the Swan. Popularly called the Tulip Nebula, the glowing cloud of interstellar gas and dust is also found in the 1959 catalog by astronomer Stewart Sharpless as Sh2-101. About 8,000 light-years distant and 70 light-years across the complex and beautiful nebula blossoms at the center of the composite image. Red, green, and blue hues map emission from ionized sulfur, hydrogen, and oxygen atoms. Ultraviolet radiation from young, energetic stars at the edge of the Cygnus OB3 association, including O star HDE 227018, ionizes the atoms and powers the visible light emission from the Tulip Nebula. HDE 227018 is the bright star very near the blue arc at the center of the cosmic tulip.

Tomorrow's picture: moonrise, mountainshadow

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3650  
Παλιά 21-10-16, 12:12
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Astronomy Picture of the Day

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21 October 2016



Full Moon in Mountain Shadow
Image Credit & Copyright: Greg Chavdarian

Explanation: On October 15, standing near the summit of Hawaii's Mauna Kea and looking away from a gorgeous sunset produced this magnificent snapshot of a Full Moon rising within the volcanic mountain's shadow. An alignment across the Solar System is captured in the stunning scene and seeming contradiction of bright Moon in dark shadow. The triangular appearance of a shadow cast by a mountain's irregular profile is normal. It's created by the perspective of the distant mountaintop view through the dense atmosphere. Rising as the Sun sets, the antisolar point or the point opposite the Sun is close to the perspective's vanishing point near the mountain shadow's peak. But extending in the antisolar direction, Earth's conical shadow is only a few lunar diameter's wide at the distance of the Moon. So October's Full Hunters Moon is still reflecting sunlight, seen through the mountain's atmospheric shadow but found too far from the antisolar point and the Earth's extended shadow to be eclipsed.

Tomorrow's picture: light-weekend

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3651  
Παλιά 22-10-16, 11:27
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22 October 2016



Cerro Tololo Trails
Image Credit & Copyright: Babak Tafreshi (TWAN), AURA

Explanation: Early one moonlit evening car lights left a wandering trail along the road to the Chilean Cerro Tololo Inter-American Observatory. Setting stars left the wandering trails in the sky. The serene view toward the mountainous horizon was captured in a telephoto timelapse image and video taken from nearby Cerro Pachon, home to Gemini South. Afforded by the mountaintop vantage point, the clear, long sight-line passes through layers of atmosphere. The changing atmospheric refraction shifts and distorts the otherwise steady apparent paths of the stars as they set. That effect also causes the distorted appearance of Sun and Moon as they rise or set near a distant horizon.

Tomorrow's picture: auroral eagle

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3652  
Παλιά 23-10-16, 10:12
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23 October 2016



Eagle Aurora over Norway
Image Credit & Copyright: Bjørn Jørgensen

Explanation: What's that in the sky? An aurora. A large coronal mass ejection occurred on our Sun five days before this 2012 image was taken, throwing a cloud of fast moving electrons, protons, and ions toward the Earth. Although most of this cloud passed above the Earth, some of it impacted our Earth's magnetosphere and resulted in spectacular auroras being seen at high northern latitudes. Featured here is a particularly photogenic auroral corona captured above Grotfjord, Norway. To some, this shimmering green glow of recombining atmospheric oxygen might appear as a large eagle, but feel free to share what it looks like to you. Although now past Solar Maximum, our Sun continues to show occasional activity creating impressive auroras on Earth visible only last week.

Tomorrow's picture: our molecular sky

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3653  
Παλιά 24-10-16, 09:23
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Astronomy Picture of the Day

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24 October 2016



HI4PI: The Hydrogen Sky
Image Credit: Benjamin Winkel & the HI4PI Collaboration

Explanation: Where are the Milky Way's gas clouds and where are they going? To help answer this question, a new highest-resolution map of the sky in the universe's most abundant gas -- hydrogen -- has been completed and recently released, along with its underlying data. Featured above, the all-sky map of hydrogen's 21-cm emission shows abundance with brightness and speed with color. Low radial speeds toward us artificially colored blue and low radial speeds away colored green. The band across the middle is the plane of our Milky Way Galaxy, while the bright spots on the lower right are the neighboring Magellanic Clouds. The HI4PI map collects data from over one million observations with the northern Eiffelsberg 100-Meter Radio Telescope in Germany and the southern Parkes 64-Meter Radio Telescope in Australia, also known as "The Dish". The details of the map not only better inform humanity about star formation and interstellar gas in our Milky Way galaxy, but also how much light this local gas is likely to absorb when observing the outside universe. Many details on the map are not yet well understood.

Tomorrow's picture: news from jupiter

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html[/QUOTE]
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  #3654  
Παλιά 25-10-16, 09:40
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Astronomy Picture of the Day

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25 October 2016



Clouds Near Jupiter's South Pole from Juno
Image Credit: NASA, JPL-Caltech, SwRI, MSSS; Processing & CC-BY: Alex Mai

Explanation: What's happening near the south pole of Jupiter? Recent images sent back by NASA's robotic Juno spacecraft are showing an interesting conglomeration of swirling clouds and what appear to be white ovals. Juno arrived at Jupiter in July and is being placed into a wide, looping orbit that will bring it near the gas giant -- and over its poles -- about twice a month. The featured image is a composite taken by JunoCam and post-processed by a digitally savvy citizen scientist. White ovals have been observed elsewhere on Jupiter and are thought to be giant storm systems. They have been observed to last for years, while typically showing Category 5 wind speeds of around 350 kilometers per hour. Unlike Earthly cyclones and hurricanes where high winds circle regions of low pressure, white ovals on Jupiter show rotational directions indicating that they are anticylones -- vortices centered on high pressure regions. Juno will continue to orbit Jupiter over thirty more times while recording optical, spectral, and gravitational data meant to help determine Jupiter's structure and evolution.

Tomorrow's picture: saturnian propellers

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3655  
Παλιά 26-10-16, 09:11
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26 October 2016



Propeller Shadows on Saturn's Rings
Image Credit: NASA, JPL-Caltech, Space Science Institute

Explanation: What created these unusually long shadows on Saturn's rings? The dark shadows -- visible near the middle of the image -- extend opposite the Sun and, given their length, stem from objects having heights up to a few kilometers. The long shadows were unexpected given that the usual thickness of Saturn's A and B rings is only about 10 meters. After considering the choppy but elongated shapes apparent near the B-ring edge, however, a leading theory has emerged that some kilometer-sized moonlets exist there that have enough gravity to create even larger vertical deflections of nearby small ring particles. The resulting ring waves are called propellers, named for how they appear individually. It is these coherent groups of smaller ring particles that are hypothesized to be casting the long shadows. The featured image was taken by the robotic Cassini spacecraft currently orbiting Saturn. The image was captured in 2009, near Saturn's equinox, when sunlight streamed directly over the ring plane and caused the longest shadows to be cast.

Tomorrow's picture: open space

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3656  
Παλιά 27-10-16, 08:53
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27 October 2016



A Giant Squid in the Flying Bat
Image Credit & Copyright: Rolf Geissinger

Explanation: Very faint but also very large on planet Earth's sky, a giant Squid Nebula cataloged as Ou4, and Sh2-129 also known as the Flying Bat Nebula, are both caught in this cosmic scene toward the royal constellation Cepheus. Composed with almost 17 hours of narrowband image data, the telescopic field of view is 4 degrees or 8 Full Moons across. Discovered in 2011 by French astro-imager Nicolas Outters, the Squid Nebula's alluring bipolar shape is distinguished here by the telltale blue-green emission from doubly ionized oxygen atoms. Though apparently completely surrounded by the reddish hydrogen emission region Sh2-129, the true distance and nature of the Squid Nebula have been difficult to determine. Still, a recent investigation suggests Ou4 really does lie within Sh2-129 some 2,300 light-years away. Consistent with that scenario, Ou4 would represent a spectacular outflow driven by HR8119, a triple system of hot, massive stars seen near the center of the nebula. The truly giant Squid Nebula would physically be nearly 50 light-years across.

Tomorrow's picture: haunting Cepheus

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3657  
Παλιά 28-10-16, 10:25
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28 October 2016



Haunting the Cepheus Flare

Image Credit & Copyright: Thomas Lelu

Explanation: Spooky shapes seem to haunt this jeweled expanse, drifting through the night in the royal constellation Cepheus. Of course, the shapes are cosmic dust clouds faintly visible in dimly reflected starlight. Far from your own neighborhood on planet Earth, they lurk along the plane of the Milky Way at the edge of the Cepheus Flare molecular cloud complex some 1,200 light-years away. Over 2 light-years across and brighter than the other ghostly apparitions, vdB 141 or Sh2-136 is also known as the Ghost Nebula, seen at the right of the starry field of view. Within the nebula are the telltale signs of dense cores collapsing in the early stages of star formation.

Tomorrow's picture: Dracula's Castle

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3658  
Παλιά 29-10-16, 09:41
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29 October 2016



Moonset at Whitby Abbey

Image Credit & Copyright: Chris Kotsiopoulos (GreekSky)


Explanation: October's Hunters Moon shines near the horizon, setting beyond the arches of Whitby Abbey in this eerie night scene. The moonlight partly illuminates the ruined Benedictine abbey's grounds and walls on a cliff overlooking the North Sea from England's Yorkshire coast. Fans of Bram Stoker's 1897 novel Dracula will recognize the abbey and town of Whitby as the location of the Transylvanian count's shipwrecked landing on English shores. There fiction's most famous vampire transformed into an immense dog, jumped ashore and ran up the cliff to the ruined abbey. A 360 degree panorama, the dramatic fisheye view was created from 23 digitally stitched photos.

Tomorrow's picture: ghost head nebula

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3659  
Παλιά 30-10-16, 11:47
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30 October 2016



Halloween and the Ghost Head Nebula

Image Credit: Mohammad Heydari-Malayeri (Observatoire de Paris) et al., ESA, NASA


Explanation: Halloween's origin is ancient and astronomical. Since the fifth century BC, Halloween has been celebrated as a cross-quarter day, a day halfway between an equinox (equal day / equal night) and a solstice (minimum day / maximum night in the northern hemisphere). With a modern calendar however, even though Halloween occurs tomorrow, the real cross-quarter day will occur next week. Another cross-quarter day is Groundhog Day. Halloween's modern celebration retains historic roots in dressing to scare away the spirits of the dead. Perhaps a fitting tribute to this ancient holiday is this view of the Ghost Head Nebula taken with the Hubble Space Telescope. Similar to the icon of a fictional ghost, NGC 2080 is actually a star forming region in the Large Magellanic Cloud, a satellite galaxy of our own Milky Way Galaxy. The Ghost Head Nebula spans about 50 light-years and is shown in representative colors.

Tomorrow's picture: sky wizard

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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  #3660  
Παλιά 31-10-16, 10:21
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Astronomy Picture of the Day

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31 October 2016



Ghost Aurora over Canada

Image Credit & Copyright: Yuichi Takasaka

Explanation: What does this aurora look like to you? While braving the cold to watch the skies above northern Canada early one morning in 2013, a most unusual aurora appeared. The aurora definitely appeared to be shaped like something , but what? Two ghostly possibilities recorded by the astrophotographer were "witch" and "goddess of dawn", but please feel free to suggest your own Halloween-enhanced impressions. Regardless of fantastical pareidolic interpretations, the pictured aurora had a typical green color and was surely caused by the scientifically commonplace action of high energy particles from space interacting with oxygen in Earth's upper atmosphere. In the image foreground, at the bottom, is a frozen Alexandra Falls, while evergreen trees cross the middle.

Tomorrow's picture: holes in galaxies

ΠΗΓΗ: http://apod.nasa.gov/apod/astropix.html
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