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panzer
Advanced Member
12516 Posts
Member since 18/05/2005 |
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Just_Charlie
Advanced Member
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8577 Posts
Member since 07/01/2008 |
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Poli
Advanced Member
Slovenia
37354 Posts
Member since 26/10/2007 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
 Posted - 04/02/2014 : 03:00:15
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Credit & Copyright: Piotrek Sadowski
Originally published by NASA APOD
NGC 6188
Dark shapes with bright edges winging their way through dusty NGC 6188 are tens of light-years long. The emission nebula is found near the edge of an otherwise dark large molecular cloud in the southern constellation Ara, about 4,000 light-years away. Formed in that region only a few million years ago, the massive young stars of the embedded Ara OB1 association sculpt the fantastic shapes and power the nebular glow with stellar winds and intense ultraviolet radiation. The recent star formation itself was likely triggered by winds and supernova explosions, from previous generations of massive stars, that swept up and compressed the molecular gas. A false-color Hubble palette was used to create this sharp close-up image and shows emission from sulfur, hydrogen, and oxygen atoms in red, green, and blue hues. At the estimated distance of NGC 6188, the picture spans about 200 light-years.
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~ Prvo suputnik onda put ~
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lwood
Advanced Member
Colombia
46541 Posts
Member since 09/12/2005 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 09/02/2014 : 16:26:25
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The Soul Nebula
IC 1805 (SH2-199) is an emission nebula located in the constellation Cassiopeia
and is the eastern neighbor of IC 1805 (Heart nebula). |
~ Prvo suputnik onda put ~
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 11/02/2014 : 00:29:36
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Na majcici zemlji smo. Ledeni Antarktik
New Species of Sea Anemone Found in Antarctic Ice
In 2010, a team of scientists discovered a new species of sea anemones beneath Antarctica's Ross Ice Shelf. The new anemones are the first known to live in ice. On this picture, red dots are 10 cm apart.
The discovery of these sea anemones is so new that scientists don't yet know how these creatures are able to survive, but there could be exciting implications in the search for extraterrestrial life, such as Jupiter's ice-covered moon Europa.
http://www.astrobio.net/exclusive/5991/new-species-of-sea-anemone-found-in-antarctic-ice
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~ Prvo suputnik onda put ~
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lwood
Advanced Member
Colombia
46541 Posts
Member since 09/12/2005 |
Posted - 11/02/2014 : 01:14:20
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quote:
Originally posted by Just_Charlie
Zemljica ko krafnica? 
What would the Earth be like if it was the shape of a donut?
According to the laws of physics, a planet the shape of a donut, or toroid, could actually exist — but it's extremely unlikely to ever form naturally. But what if an advanced alien civilization decided to build one? What properties would a toroid-Earth exhibit? And what would life be like? ..
http://io9.com/what-would-the-earth-be-like-if-it-was-the-shape-of-a-d-1515700296
ovo je baš sexy  |
Dajte nam Banija Libre;može i mekokoricen (ali s osvrtom na forumaše obavezno)!
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 11/02/2014 : 02:01:53
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pa dobro, zar bas svaka rupa u Svemiru mora biti seksi?!
Kako je tim muzjacima sve jednostavno! 
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~ Prvo suputnik onda put ~
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nagor
Advanced Member
Croatia
12553 Posts
Member since 21/02/2012 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 27/02/2014 : 21:09:39
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ovo je prizor od kojeg zastaje dah.
Hubble’s Wide Field Camera 3 has captured this image of a giant cloud of hydrogen gas illuminated by a bright young star. The image shows how violent the end stages of the star-formation process can be, with the young object shaking up its stellar nursery.Despite the celestial colours of this picture, there is nothing peaceful about star forming region Sh 2-106, or S106 for short. A devilish young star, named S106 IR, lies in it and ejects material at high speed, which disrupts the gas and dust around it. The star has a mass about 15 times that of the Sun and is in the final stages of its formation. It will soon quieten down by entering the main sequence, the adult stage of stellar life.For now, S106 IR remains embedded in its parent cloud, but it is rebelling against it. The material spewing off the star not only gives the cloud its hourglass shape but also makes the hydrogen gas in it very hot and turbulent. The resulting intricate patterns are clearly visible in this Hubble image.The young star also heats up the surrounding gas, making it reach temperatures of 10 000 degrees Celsius. The star’s radiation ionises the hydrogen lobes, making them glow. The light from this glowing gas is coloured blue in this image.Separating these regions of glowing gas is a cooler, thick lane of dust, appearing red in the image. This dark material almost completely hides the ionising star from view, but the young object can still be seen peeking through the widest part of the dust lane.S106 was the 106th object to be catalogued by the astronomer Stewart Sharpless in the 1950s. It is a few thousand light-years distant in the direction of Cygnus (The Swan). The cloud itself is relatively small by the standards of star-forming regions, around 2 light-years along its longest axis. This is about half the distance between the Sun and Proxima Centauri, our nearest stellar neighbour.This composite picture was obtained with the Wide Field Camera 3 on the NASA/ESA Hubble Space Telescope. It results from the combination of two images taken in infrared light and one which is tuned to a specific wavelength of visible light emitted by excited hydrogen gas, known as H-alpha. This choice of wavelengths is ideal for targetting star-forming regions. The H-alpha filter isolates the light emitted from hydrogen in gas clouds while the infrared light can shine through the dust that often obscures these regions. |
~ Prvo suputnik onda put ~
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 27/02/2014 : 21:17:43
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Galaksija Vrtlog poznata još kao Messier 51a, M51a ili NGC 5194 je spiralna galaksija u zviježđu Lovački psi. Otkrio ju je Charles Messier 1773. godine |
~ Prvo suputnik onda put ~
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 12/03/2014 : 00:14:50
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Međunarodni dan planetarija u Astronomskom centru Rijeka
Povodom Međunarodnog dana planetarija Astronomski centar Rijeka i ove je godine, u subotu 15. ožujka pripremio poseban program koji će se odvijati tokom cijelog dana. Ulaz u planetarij na taj dan bit će prigodnih 10 kuna za filmove i interaktivne prezentacije, a program u jedinom digitalnom planetariju u Hrvatskoj i šire podijeljen je na jutarnji i večernji. Jutarnji program donosi filmove i interaktivne prezentacije za djecu i odrasle, dok će u večernjem programu moći uživati studenti i odrasle osobe.
Ova se manifestacija obilježava od 1995. godine diljem svijeta i predstavlja priliku popularizacije svijeta planetarija i udruživanja strukovnih institucija. Ista organizacija broji oko 700 članova iz 35 različitih zemalja.
Riječki Astronomski centar, čiji je vlasnik Rijeka sport, obilježava ovu manifestaciju od 2010. godine. Također, ove godine Centar obilježava petu godišnjicu rada i do sada je u digitalnom planetariju bilo sinkronizirano osam filmova i to Pogled na planete, Vibrato, Utrka do Zemlje, Dva mala komada stakla, Misija: Mars, Dotaknuti rub Svemira, Kaluoka'hina – začarani greben i Carstvo svjetlosti. Također, u digitalnom planetariju posjetitelji su mogli pogledati live prezentacije Vodič noćnim nebom, Mala tijela Sunčevog sustava, Moj prvi pogled u nebo, Susret s astronomijom, Svemir: na vama je da ga otkrijete, Safari Sunčevim sustavom, Od Zemlje do Svemira, Mjesec u sjeni, Nebo ispod nas, 10 najzviježđa, 10 zašto volim astronomiju, Naša zvijezda Sunce, U potrazi za kometima. Do sada je program u prostoru riječkog planetarija pogledalo 49.500 posjetitelja iz Hrvatske i inozemstva.
http://www.rijekasport.hr/astronomskicentar
p.s. - 29. ožujka - Sat za Zemlju - akcija gašenja vanjske rasvjete |
~ Prvo suputnik onda put ~
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mladjo
Advanced Member
.jpg)
Croatia
20013 Posts
Member since 15/04/2007 |
Posted - 12/03/2014 : 00:38:15
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quote:
Originally posted by Just_Charlie
ovo je prizor od kojeg zastaje dah.
Hubble’s Wide Field Camera 3 has captured this image of a giant cloud of hydrogen gas illuminated by a bright young star. The image shows how violent the end stages of the star-formation process can be, with the young object shaking up its stellar nursery.Despite the celestial colours of this picture, there is nothing peaceful about star forming region Sh 2-106, or S106 for short. A devilish young star, named S106 IR, lies in it and ejects material at high speed, which disrupts the gas and dust around it. The star has a mass about 15 times that of the Sun and is in the final stages of its formation. It will soon quieten down by entering the main sequence, the adult stage of stellar life.For now, S106 IR remains embedded in its parent cloud, but it is rebelling against it. The material spewing off the star not only gives the cloud its hourglass shape but also makes the hydrogen gas in it very hot and turbulent. The resulting intricate patterns are clearly visible in this Hubble image.The young star also heats up the surrounding gas, making it reach temperatures of 10 000 degrees Celsius. The star’s radiation ionises the hydrogen lobes, making them glow. The light from this glowing gas is coloured blue in this image.Separating these regions of glowing gas is a cooler, thick lane of dust, appearing red in the image. This dark material almost completely hides the ionising star from view, but the young object can still be seen peeking through the widest part of the dust lane.S106 was the 106th object to be catalogued by the astronomer Stewart Sharpless in the 1950s. It is a few thousand light-years distant in the direction of Cygnus (The Swan). The cloud itself is relatively small by the standards of star-forming regions, around 2 light-years along its longest axis. This is about half the distance between the Sun and Proxima Centauri, our nearest stellar neighbour.This composite picture was obtained with the Wide Field Camera 3 on the NASA/ESA Hubble Space Telescope. It results from the combination of two images taken in infrared light and one which is tuned to a specific wavelength of visible light emitted by excited hydrogen gas, known as H-alpha. This choice of wavelengths is ideal for targetting star-forming regions. The H-alpha filter isolates the light emitted from hydrogen in gas clouds while the infrared light can shine through the dust that often obscures these regions.
Liči mi na čovjeka s naočalama.
Al dobro, ja svuda vidim oblike.
Inače, stara je znala gatati na grah i iz kave tak da sam to valjda nasljedil od nje:)) |
COUNT ZERO INTERRUPT
an interrupt of a process decrements a counter to zero
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
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panzer
Advanced Member
12516 Posts
Member since 18/05/2005 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 17/03/2014 : 01:28:08
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A powerful telescope in Chile has imaged the largest yellow star ever discovered. The star, called HR 5171 A, shines 12,000 light-years from Eart |
~ Prvo suputnik onda put ~
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mladjo
Advanced Member
Croatia
20013 Posts
Member since 15/04/2007 |
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panzer
Advanced Member
12516 Posts
Member since 18/05/2005 |
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mladjo
Advanced Member
Croatia
20013 Posts
Member since 15/04/2007 |
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Just_Charlie
Advanced Member
8577 Posts
Member since 07/01/2008 |
Posted - 20/03/2014 : 23:42:33
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Komadic mog neba i moje najsjajnije zvijezde na njemu.
  
  
 
Svaki dan promatramo zalazak Sunca, i prve zvijezde,
i tad promrzli(gore je hladno kad Sunce zađe)
odlazimo posljednji..
Srdacno vasa.. slikom recenim stilom   |
~ Prvo suputnik onda put ~
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Edited by - Just_Charlie on 20/03/2014 23:46:12 |
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SHINING LIKE BRIGHT DIAMONDS, THE GALAXIES...
