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Space images thread

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NGC 7674 is a luminous infrared galaxy. It is located in the constellation of Pegasus, ~ 400 million ly away from us.
The central bar-shaped structure is made up of stars. The shape, including the long narrow streamers seen to the left of and below the galaxy can be accounted for by tidal interactions with its companions.
 
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Best image of Lobster Nebula ever taken



M17 is located ~ 5500 ly from us near the plane of the Milky Way. Its gas and dust clouds measure ~ 15 ly across. The gas in the nebula is estimated to have more than 30 000 times the mass of the Sun.

Download bigger version (Warning: file size is 158 MB)
 
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Barred spiral galaxy NGC 613

It lies 67 million ly away in the constellation of Sculptor. A monstrous black hole resides at the heart of NGC 613. Its mass is estimated at about ten times that of the Milky Way's supermassive black hole and it is consuming stars, gas and dust.
 
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Gemini Observatory has released one of the most detailed images ever obtained of emerging gas jets streaming from a region of newborn stars called Herbig-Haro 24. Located in the Orion B cloud, at a distance of about 400 parsecs, or ~ 1300 ly from us, this region is rich in young stars.

 
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NGC 559 is a moderately large and compact open cluster in Cassiopeia. The stars are fairly bright and the cluster appears best with moderate magnification.



The galaxy cluster SPT-CLJ2344-4243, nicknamed the Phoenix Cluster.
 
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Pulsar PSR B1257+12 (located 1000 ly from us)



Ultraviolet image of the globular cluster NGC 1851 in the southern constellation Columba.

 
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The old open cluster NGC 188



NGC 185 (Caldwell 18) is a dwarf spheroidal galaxy ~ 2.08 million ly away in the constellation Cassiopeia. It is a member of the Local group, and is a satellite galaxy of the Andromeda Galaxy.



Astronomers have discovered never-before-seen structures within a dusty disc surrounding a nearby star AU Microscopii (32 ly away). The fast-moving wave-like features in the disc of the star are unlike anything ever observed. The origin and nature of these features present a new mystery for astronomers to explore.
 
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Another "view" of 40-billion-mile-diameter edge-on disk encircling the young star AU Microscopii. The ripples are moving across the disk at a speed of 22000 mph.



White dwarf stars WD 0421+162 and WD 0431+126 in the Hyades star cluster, the nearest open cluster to us.

 
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A Hubble Space Telescope color image of a small portion of the M4 cluster only 0.63 ly across reveals 8 white dwarf stars among the cluster's much brighter population of yellow sun-like stars and cooler red dwarf stars.
 
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HH 211 is located ~ 1000 ly away in the constellation of Perseus. Astronomers estimate that the small protostar hidden within HH 211 is <1000 years old-a mere baby by astronomical standards, so young that it is still growing by accumulating matter from a surrounding disk of gas and dust. The protostar eventually will become a low-mass star similar to the sun.



A pair of jets protrude outwards in near-perfect symmetry in this image of HH 212. The object lies in the constellation of Orion. The jet pulses vary quite regularly, and over a short timescale - maybe even as short as 30 years!
 
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The extended gas cloud near the planetary nebula NGC 3242



Composite image of an edge-on spiral galaxy with a radio halo produced by fast-moving particles in the galaxy's magnetic field. In this image, the large, grey-blue area is a single image formed by combining the radio halos of 30 different galaxies, as seen with the Very Large Array. At the center is a visible-light image of one of the galaxies, NGC 5775, made using the Hubble Space Telescope. This visible-light image shows only the inner part of the galaxy's star-forming region, outer portions of which extend horizontally into the area of the radio halo. This spectacular image shows that cosmic rays and magnetic fields not only permeate the galaxy disk itself, but extend far above and below the disk.
 
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Coalsack Nebula! Yay!



Coalsack Nebula is 600 ly away in the constellation of Crux.

The little light that does make it through the nebula does not come out the other side unchanged. The light we see in this image looks redder than it ordinarily would. This is because the dust in dark nebulae absorbs and scatters blue light from stars more than red light, tinting the stars several shades more crimson than they would otherwise be.

Millions of years in the future the Coalsack's dark days will come to an end. As the stray material in the Coalsack coalesces under the mutual attraction of gravity, stars will eventually light up.

Download giant version 210 MB
 
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Left: Map of the galaxy PACS-867 taken by ALMA where the emission from carbon monoxide (CO) shows the molecular gas reservoir out of which stars form. Centre: Image taken by the Hubble Space Telescope Advanced Camera for Surveys of PACS-867 that shows the rest-frame UV light from young stars in the individual components of highly disturbed galaxies as a result of a massive merger. The location of the molecular gas in Image 1 is overlaid (blue contours) that shows where new stars, enshrouded by dust, are forming. Right: Spitzer Space Telescope infrared image (3.6 micron) of PACS-867 highlights the stars embedded in dust and associated with the molecular gas. The UV light associated with the gas is faint while it is brighter in the infrared. This is due to the presence of dust that impacts the UV more than the IR.



Interacting galaxy Zw II 96 in the constellation of Delphinus, is an example of a galaxy merger located some 500 million ly away.



The green and red splotch in this image is the most active star-making galaxy in the very distant universe. Nicknamed "Baby Boom," the galaxy is churning out an average of up to 4000 stars per year, more than 10 times the number produced in our own Milky Way galaxy. It was spotted 12.3 billion ly away by a suite of telescopes, including NASA's Spitzer Space Telescope.

Baby Boom is a type of galaxy called a starburst. Like some other starbursts, it is thought to be a collection of colliding galaxies. As the galaxies smash together, gas becomes compressed, triggering the birth of stars. In this multi-wavelength portrait, the color red shows where loads of new stars are forming in Baby Boom, and where warm dust heated by the stars is giving off infrared light.

Green (visible-light wavelengths) denotes gas in the Baby Boom galaxy, while blue (also visible light) shows galaxies in the foreground that are not producing nearly as many stars. Yellow/orange (near-infrared light) indicates starlight from the outer portion of Baby Boom. The red blob to the left is another foreground galaxy that is not producing a lot of stars.



Cloud and Star Formation near the Filamentary Ministarburst RCW 106
 

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Why we " aint seen nothing yet"

The James Webb Telescope

http://www.jwst.nasa.gov/


Hubbles primary mirror is the silver disc

1. It’s as big as a tennis court
With a sunshield 22 metres (72 feet) in length, the size of a tennis court, and a mirror 6.5 metres (21 feet) wide the JWST, which is due to launch in October 2018, is over twice the size of the Hubble Space Telescope, making it the largest space telescope ever launched.

2. The mirrors are coated in a golf ball’s worth of gold
The JWST’s mirrors are covered in gold to optimise them for infrared light, with the gold further protected by a thin layer of glass. The thickness of this gold coating is 0.00001 centimetres across the 25 square-metre mirror’s surface, and in total the gold weighs 48.25 grams, roughly equivalent to the weight of a golf ball.

3. It’ll be about four times further from Earth than the Moon
The JWST will take about a month to reach a position 1.5 million kilometres (930,000 miles) from Earth known as Lagrange point 2, or L2. Here the telescope’s observations will be unhindered by Earth and the Moon although, if it malfunctions (as happened with Hubble), we currently have no way to go and fix it.

4. It could see a penny 24 miles away
The angular resolution of the JWST, which is the sharpness of the images, is incredibly precise. It can see at a resolution of 0.1 arc-seconds, which means that it could resolve a penny 24 miles (40 kilometres) away or a football 340 miles (550 kilometres) away.

5. It could find water on exoplanets
One of the JWST’s most notable abilities is that it will be able to detect planets around nearby stars by measuring infrared radiation, and it will even be able to measure the atmospheres of exoplanets by studying the starlight that passes through. By doing this it will be able to determine if an exoplanet has liquid water on its surface.

6. It’s seven times more powerful than the Hubble Space Telescope
The giant mirror of the JWST is made of 18 individual hexagonal segments composed of lightweight beryllium. It is almost three times the size of Hubble’s mirror, boasting a light-collecting area seven times greater, but both mirrors weigh almost the same owing to the lighter materials used on the JWST’s mirror.

7. It’ll see the first light of the universe
One of the goals of the JWST is to observe the first stars and galaxies that formed just a few hundred million years after the Big Bang, an era of the universe that is not fully understood. The telescope will be sensitive to infrared light, which will enable it to do this.

8. It will unfold to its massive size in space
Many features of the JWST, including its giant mirrors and sunshield, are designed to be launched on a rocket in a smaller payload. The telescope will launch in a compact outfit and will unfold in its full configuration once it reaches space.

9. One side is hotter than Death Valley, the other is colder than Antarctica
The side of the JWST that will always face the Sun, the bottom of the sunshield, will reach temperatures of 85°C (185 °F). The other side, which houses the mirrors and science instruments, will operate at a much nippier -233°C (-388 °F).

10. It could keep working for a decade
The official mission lifespan for the JWST is between five and ten years. The telescope is limited by the amount of fuel it has on board used to maintain its position, which will be enough for a ten-year lifetime. Of course, other factors like budget cuts or malfunctions could end the mission earlier.

Launch is scheduled for launch in October 2018

Ariane 5 is the European launch vehicle chosen to fly from Kourou, French Guiana.

An Ariane 5 launch for you


https://en.wikipedia.org/wiki/James_Webb_Space_Telescope
 
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Radio and optical image showing the giant radio galaxy IC 711 and companions IC 708 and IC 712. All three systems are part of the distant galaxy cluster Abell 1314 and were serendipitously located in a field pointed at an unrelated low redshift galaxy.

 
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JHK image of the Milky Way's nuclear star cluster



Bipolar jet from a high-mass protostar IRAS20126+4104


This image shows IRAS 04302+2247, a star hidden from direct view and seen only by the nebula it illuminates. Dividing the nebula in two is a dense, edge-on disk of dust and gas which appears as the thick, dark band crossing the center of the image. The disk has a diameter of 80 billion miles (15 times the diameter of Neptune's orbit), and has a mass comparable to the Solar Nebula, which gave birth to our planetary system. Dark clouds and bright wisps above and below the disk suggest that it is still building up from infalling dust and gas.
 
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