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First James Webb image
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First James Webb image
Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Fantastic. Look at the link and scroll to the first post. It shows what the Hubble was able to see for the same field compared to the James Webb. When I saw the James Webb photo, I saw the curved streaks. They are the result of gravitational lensing where light from very distant galaxies are bent when they pass by a massive object (sometimes a black hole) and their light is distorted into thin curved streaks. Einstein predicted this in his general theory of relativity, more than 100 years ago.
LarryAnalog- VPIClassic3-3DArm,Lyra Skala+MiyajimaZeroMono, 2xAmpex ATR-102,Otari MX5050B2,Merrill Trident Master Tape Pre,Herron VTPH-2A
Dig Rip-Pyramix,IzotopeRX3Adv,Mykerinos,PacMicroModel2
Dig Play-mchNADAC, LampiHorizon, Roon, HQP, Oppo105
Electronics-Doshi Pre,CJ MET1mchPre, Cary2A3monoamps
Speakers-AvantgardeDuosLR,3SolosC,LR,RR
Other-2x512Engineer/Marutani Symmetrical Power, AudioDiskVinylCleaner, Scott Rust Interconnects,
Music-2000R2Rtapes,50TBrips
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Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Jupiter
In a wide-field view, Webb sees Jupiter with its faint rings, which are a million times fainter than the planet, and two tiny moons called Amalthea and Adrastea. The fuzzy spots in the lower background are likely galaxies “photobombing” this Jovian view.
“This one image sums up the science of our Jupiter system program, which studies the dynamics and chemistry of Jupiter itself, its rings, and its satellite system,” Fouchet said. Researchers have already begun analyzing Webb data to get new science results about our solar system’s largest planet.
Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Massive Mosaic Filled With Galaxies , see them all at https://ceers.github.io/ceers-first-images-release
JWST has taken the first epoch of observations for our CEERS Survey and it is currently the largest image taken by the telescope to date! These data include NIRCam and MIRI imaging, covering near-infrared to mid-infrared wavelengths in the EGS field - a small patch of sky near the handle of the Big Dipper. We have produced a color image mosaic of all of our Epoch 1 data, which we share below, with several highlights and additional information. Epoch 1 covers less than half of our total survey area on the sky and already the images have led to new discoveries and an unexpected, but not unwelcome, abundance of never-before-seen galaxies. We hope you enjoy exploring these images as much as we have enjoyed studying them, and be sure to open the high-resolution ones to zoom in - the sheer number of galaxies we have captured so far is awe-inspiring!
From https://www.extremetech.com/extreme/...-with-galaxies
In the images, the CEERS team has identified some of the most interesting objects in Epoch 1. Here’s what makes each one notable.- A spiral galaxy at a redshift of z = 0.16. The resolution of the JWST imaging reveals a large number of blue star-forming clumps and star clusters.
- A chance alignment of a bright galaxy at a redshift z = 1.05 with several smaller galaxies forming an arc in the sky when viewed from JWST.
- An interacting system of galaxies at z = 1.4, dubbed the “Space Kraken” by the CEERS team.
- Two interacting spiral galaxies at z = 0.7. The arrow points to a supernova discovered with these JWST images.
- Another spiral galaxy, also at z = 0.7, again highlighting JWST’s ability to resolve small-scale features even for modestly distant galaxies.
- A chance alignment of a z = 0.63 galaxy with a tidal tail, and a grouping of red galaxies at z = 1.85.
Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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A detailed image of the Orion Nebula
Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Venus
Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Jupiter has rings? GET OUT! Really?! Never could have imagined. Some of the above photos look like artist renderings not like photos at all. Incredible. Wouldn’t these make for a sensational planetarium presentation?Turntable: TW Acustic TT with Ref motor & controller; Tri-Planar Arm; Ortofon Windfeld-Ti Cartridge, Harmonix-Combak platter mat & weight; PS Audio Stellar Phono Preamp; KLAudio Ultrasonic Record Cleaner.
Digital: Bluesound Vault-2 Music Server & Streamer
Amplification: VTL 6.5 preamp Series II, Pass Labs 150.8 Amp
Loudspeakers: Piega C711 Loudspeakers
Isolation: Symposium Osiris Rack; Symposium Platforms and Roller Blocks and grade 2.5 Balls
Misc: Acoustic Revive RR-888 Low Frequency Pulse Generator, Synergistic Research 12 UEF SE Line Conditioner, Level 3 HC AC Cord and Level 3 Atmosphere power cords, Synergistic Carbon fiber wall plates, Synergistic Research Orange Outlet, Furutech NCF Booster Braces, Audio Art Ref IC, synergistic Research Atmosphere X Euphoria Level 3 Balanced ICs, Synergistic Research Euphoria Level 3 Speaker Cables, Synergistic Research Cable Risers.
Sennheiser HDV 650 Headphone Amp; Sennheiser HD800s Headphones.
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Saturn's rings and tilt could be the product of an ancient, missing moon
https://phys.org/news/2022-09-saturn...ient-moon.htmlAnalog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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Neptune like never seen before
Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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With Triton as well
Analog: VPI Aries 3, custom suspension & platter interface || Magnetically stabilized JMW 10.5i || Ortofon A90, Verismo || Modded & fully shielded Pass XP-25 || VPI SDS speed controller || Magnum Dynalab MD-90SE/105 Digital: Spectral 4000SV Amplification: Spectral DMC-30SV || DMA-500AR Speakers: Custom MartinLogan Cabling: Shielded MIT Oracle 50ic,MA-X,90.1,Shunyata Alpha v2 Other: Shunyata Everest & Sigma/Delta cords; Isodamp, mumetal, 3M AB5100, Dynamat, Copper foil; Vishay diodes, resistors; Mundorf coils & capacitors
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