Space Images

Galaxy's detected at nearly 97% of the way back to the Big Bang:

webb-offers-never-befo.jpg

The massive gravity of galaxy cluster MACS0647 acts as a cosmic lens to bend and magnify light from the more distant MACS0647-JD system. It also triply lensed the JD system, causing its image to appear in three separate locations. These images, which are highlighted with white boxes, are marked JD1, JD2, and JD3; zoomed-in views are shown in the panels at right. In this image from Webb’s Near Infrared Camera (NIRCam) instrument, blue was assigned to wavelengths of 1.15 and 1.5 microns (F115W, F150W), green to wavelengths of 2.0 and 2.77 microns (F200W, F277W) and red to wavelengths of 3.65 and 4.44 microns (F365W, F444W). Credit: NASA, ESA, CSA, STScI, Tiger Hsiao, Alyssa Pagan

Imaging two separate structures was a surprise since Hubble displayed only one galaxy. Mankind's ability to perform research about the evolution of galaxies in time has gained a lot of traction since the James Webb telescope was finally deployed.

"Every single one of them. It's amazing the amount of information that we're getting that we just weren't able to see before. And this is not a deep field. This is not a long exposure. We haven't even really tried to use this telescope to look at one spot for a long time. This is just the beginning."
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An intergalactic bridge (a gravitational tidal tail) was captured by the Hubble space telescope.

hubble-arp248-potw2244a.jpg

Credit(s): ESA/Hubble & NASA, Dark Energy Survey/Department of Energy/Fermilab Cosmic Physics Center/Dark Energy Camera/
Cerro Tololo Inter-American Observatory/NOIRLab/National Science Foundation/AURA Astronomy; J. Dalcanton



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Reference: CNET
 
Mercury's sodium tail:

MercuryTailPleiades_Voltmer_960.jpg

"Mercury's thin atmosphere contains small amounts of sodium that glow when excited by light from the Sun.
Sunlight also liberates these atoms from Mercury's surface and pushes them away. The yellow glow from
sodium, in particular, is relatively bright."


About - sodium ( click on the symbol "Na" on the left-hand-side of the periodic table )

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Reference: Astronomy picture of the Day
 
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The cosmic web ( wait for it...)



Credit: Pawel Czubinski · Jul 31, 2013


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Reference: Nature

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Icy Enceladus is very fascinating.

^That^ is an exploration understatement. :cool:

Sending a number of robotic drills stuffed with a set of robust diagnostics* to discover what is underneath the water ice would be wonderful.

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* A miniature submarine fleet in contact with surface drills and transmission antennae systems - perhaps
 
A Wolf-Rayet star as imaged by James Webb below has strong emission lines is very hot with temperatures from 25,00 K - 100,000 K, and on average they tend to lose mass in excess of 1*10^-5 of the mass our sun per year.




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About those extra-large neutrons -

A neutron star X-ray telescope


NICER

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Uranus at 19.194 AU from the sun, with an orbital inclination of 0.77 deg. to the ecliptic plane, also has a 97.86 deg. polar inclination to the ecliptic as shown below.


Twelve minute exposure of Uranus.jpg
Image Credit: NASA, ESA, CSA, STScI, with image processing by Joseph DePasquale (STScI)

The gas giant also experiences 42 years of sunlight and 42 years of darkness from its 84 year orbit around our sun.

___________ :coffee:


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Galaxy's detected at nearly 97% of the way back to the Big Bang:

webb-offers-never-befo.jpg

The massive gravity of galaxy cluster MACS0647 acts as a cosmic lens to bend and magnify light from the more distant MACS0647-JD system. It also triply lensed the JD system, causing its image to appear in three separate locations. These images, which are highlighted with white boxes, are marked JD1, JD2, and JD3; zoomed-in views are shown in the panels at right. In this image from Webb’s Near Infrared Camera (NIRCam) instrument, blue was assigned to wavelengths of 1.15 and 1.5 microns (F115W, F150W), green to wavelengths of 2.0 and 2.77 microns (F200W, F277W) and red to wavelengths of 3.65 and 4.44 microns (F365W, F444W). Credit: NASA, ESA, CSA, STScI, Tiger Hsiao, Alyssa Pagan

Imaging two separate structures was a surprise since Hubble displayed only one galaxy. Mankind's ability to perform research about the evolution of galaxies in time has gained a lot of traction since the James Webb telescope was finally deployed.

"Every single one of them. It's amazing the amount of information that we're getting that we just weren't able to see before. And this is not a deep field. This is not a long exposure. We haven't even really tried to use this telescope to look at one spot for a long time. This is just the beginning."
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This discovery actually presented quite a problem. Link created to show why.
 
Uranus at 19.194 AU from the sun, with an orbital inclination of 0.77 deg. to the ecliptic plane, also has a 97.86 deg. polar inclination to the ecliptic as shown below.


View attachment 4001
Image Credit: NASA, ESA, CSA, STScI, with image processing by Joseph DePasquale (STScI)

The gas giant also experiences 42 years of sunlight and 42 years of darkness from its 84 year orbit around our sun.

___________ :coffee:


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History of observations from the Keck Observatory: Uranus

Keck Telescope historic photos of Uranus.jpg


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The Sombrero Galaxy - an infrared image


The Sombrero Galaxy in the IR.jpg

This galaxy's classification is unclear based on it's appearance 31.1 million light-years from our Milky Way Galaxy, and its diameter is about 49,000 light-years in diameter. It resides in the Virgo supercluster.

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