#infrared space telescope

[blueiscoool]

Spitzer Telescope

These bright young stars are found in a rosebud-shaped (and rose-colored) nebulosity known as NGC 7129. The star cluster and its associated nebula are located at a distance of 3300 light-years in the constellation Cepheus.

The Spitzer Space Telescope, formerly the Space Infrared Telescope Facility (SIRTF), was an infrared space telescope launched in 2003. Operations ended on 30 January 2020.

[aspaceinthecosmos]

new webb image(s) alert! 19 galaxies imaged in mid and near infrared light

i’m just blown away by the detail in these images- jwst never ceases to amaze me.

you can find the full resolution images of each of these galaxies in the official release here - i highly recommend looking through each of them, they’re STUNNING.

[spacetelescopescience]

To celebrate the James Webb Space Telescope's second year of science, let’s look back at one of its first images, the Cartwheel Galaxy. This near- and mid-infrared image shows the areas where stars develop after a high-speed collision about 400 million years ago: https://bit.ly/3WfJYW2

[without-ado]

Saturn and its moons l Webb

[thepastisalreadywritten]

With the addition of Saturn, the James Webb Space Telescope has finally captured all four of our Solar System's giant worlds.

JWST's observations of the ringed planet, taken on 25 June 2023, have been cleaned up and processed, giving us a spectacular view of Saturn's glorious rings, shining golden in the darkness.

By contrast, the disk of Saturn is quite dark in the new image, lacking its characteristic bands of cloud, appearing a relatively featureless dim brown.

This is because of the wavelengths in which JWST sees the Universe – near- and mid-infrared.

These wavelengths of light are usually invisible to the naked human eye, but they can reveal a lot.

For example, thermal emission – associated with heat – is dominated by infrared wavelengths.

When you're trying to learn about what's going on inside a planet wrapped in thick, opaque clouds, studying its temperature is a valuable way to go about it.

Some elements and chemical processes emit infrared light, too. Seeing the planets of the Solar System in wavelengths outside the narrow range admitted by our vision can tell us a lot more about what they have going on.

Saturn

As we saw last week, when we clapped eyes on the raw JWST Saturn images, the observations involved filters that dimmed the light of the planet, while allowing light from the rings and moons to shine brightly.

This is so a team led by planetary scientist Leigh Fletcher of the University of Leicester in the UK can study the rings and moons of Saturn in more detail.

They hope to identify new ring structures and, potentially, even new moons orbiting the gas giant.

The image above shows three of Saturn's moons, Dione, Enceladus and Tethys, to the left of the planet.

Although dim, the disk of the planet also reveals information about Saturn's seasonal changes.

The northern hemisphere is reaching the end of its 7-year summer, but the polar region is dark. An unknown aerosol process could be responsible.

Meanwhile, the atmosphere around the edges of the disk appears bright, which could be the result of methane fluorescence, or the glow of trihydrogen, or both. Further analysis could tell us which.

Jupiter

Jupiter was the first of the giant planets to get the JWST treatment, with images dropping in August of last year – and boy howdy were they stunning.

The spectacular detail seen in the planet's turbulent clouds and storms was perhaps not entirely surprising.

However, we also got treated to some rarely seen features: the permanent aurorae that shimmer at Jupiter's poles, invisible in optical wavelengths, and Jupiter's tenuous rings.

We also saw two of the planet's smaller, lesser-known moons, Amalthea and Adrastea, with fuzzy blobs of distant galaxies in the background.

"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," said astronomer Thierry Fouchet of Paris Observatory in France, who co-led the observations.

Neptune

Observations of Neptune arrived in the latter half of September 2022.

Because Neptune is so very far away, it tends to get a little neglected; you're probably used to seeing, if anything, the images taken by Voyager 2 when it flew past in 1989.

JWST's observations gave us, for the first time in more than 30 years, a new look at the ice giant's dainty rings – and the first ever in infrared.

It also revealed seven of Neptune's 14 known moons, and bright spots in its atmosphere.

Most of those are storm activity, but if you look closely, you'll see a bright band circling the planet's equator.

This had never been seen before and could be, scientists say, a signature of Neptune's global atmospheric circulation.

Uranus

Uranus is also pretty far away, but it's also a huge weirdo. Although very similar to Neptune, the two planets are slightly different hues, which is something of a mystery.

Uranus is also tipped sideways, which is challenging to explain too.

JWST's observations, released in April 2023, aren't solving these conundrums.

However, they have revealed 11 of the 13 structures of the incredible Uranian ring system and an unexplained atmospheric brightening over the planet's polar cap.

JWST has a lot to say about the early Universe; but it's opening up space science close to home, too.

As its first year of operations comes to an end, we can't help but speculate what new wonders will be to come in the years ahead.

Top: Jupiter - Neptune / Bottom: Uranus - Saturn

Credit: NASA

[wayti-blog]

"This stunning new mosaic of images from the NASA/ESA/CSA James Webb Space Telescope showcases the nearby star-forming cluster, NGC 1333."

"These data constitute the first deep spectroscopic survey of the young cluster, and have identified brown dwarfs down to planetary masses using the observatory’s Near-Infrared Imager and Slitless Spectrograph (NIRISS). The first results from this survey have been accepted for publication in the Astronomical Journal."

source

[thefirststarr]

SPACEMAS DAY 17 ✨🪐🌎☄️☀️🌕

The Ring Nebula (M57), is more complicated than it appears through a small telescope. The easily visible central ring is about one light-year across, but this remarkable exposure by the James Webb Space Telescope explores this popular nebula with an exposure in infrared light. Strings of gas, like eyelashes around a cosmic eye, become evident around the nebula in this digitally enhanced featured image in assigned colors. These long filaments may be caused by the shadowing of knots of dense gas in the ring from energetic light emitted within. The Ring Nebula is an elongated planetary nebula, a type of gas cloud created when a Sun-like star evolves to throw off its outer atmosphere to become a white dwarf star. The central oval in the Ring Nebula lies about 2,500 light-years away toward the musical constellation Lyra.

Image Credit & Copyright: NASA, ESA, CST, JWST

[viridare]

NASA Hubble Space Telescope - An Infrared View of Saturn

[kimlion13]

Crab Nebula, taken by the James Webb Space Telescope’s NIRCam (Near-Infrared Camera) & MIRI (Mid-Infrared Instrument)

Published by NASA 10/30/23

[ton-618-ton-618]

2024 April 3

A nebula is shown that appears like a firework. Radial filaments connect a glowing halo to a star in the center that appears as a blue dot.

Unusual Nebula Pa 30

Image Credit: NASA, ESA, USAF, NSF;

Processing: G. Ferrand (U. Manitoba), J. English (U. Manitoba), R. A. Fesen (Dartmouth), C. Treyturik (U. Manitoba);

Text: G. Ferrand & J. English

Explanation: What created this unusual celestial firework? The nebula, dubbed Pa 30, appears in the same sky direction now as a bright "guest star" did in the year 1181. Although Pa 30's filaments look similar to that created by a nova (for example GK Per), and a planetary nebula (for example NGC 6751), some astronomers now propose that it was created by a rare type of supernova: a thermonuclear Type Iax, and so is (also) named SN 1181. In this model, the supernova was not the result of the detonation of a single star, but rather a blast that occurred when two white dwarf stars spiraled together and merged. The blue dot in the center is hypothesized to be a zombie star, the remnant white dwarf that somehow survived this supernova-level explosion. The featured image combines images and data obtained with infrared (WISE), visible (MDM, Pan-STARRS), and X-ray (Chandra, XMM) telescopes. Future observations and analyses may tell us more.

[blasteffect]

These two stunning images show the same cosmic object, located 160,000 light-years away, captured by the Hubble Space Telescope.

The blue image highlights near-infrared and visible light, while the red image covers near-ultraviolet to infrared light.

Astrophysicists believe the first generation of stars ejected matter, which, due to the cluster's high density, couldn't escape its gravity.

Credit: NASA

[boanerges20]

NGC7293 Helix Nebula in Acuarius In Infrared. Spitzer Telescope/ NASA. Procesed: Judy Schmidt.

[breadandblankets]

rip Duke Thomas you would have loved the Spaceship Spitzer podcast

[your-local-future-milf]

Does the internet want this edit? I made it :D

[thepastisalreadywritten]

Comet NEOWISE rising over the Earth just before dawn as seen from the International Space Station. ☄️

—

C/2020 F3 (NEOWISE) or Comet NEOWISE is a long period comet with a near-parabolic orbit discovered on 27 March 2020 by astronomers during the NEOWISE mission of the Wide-field Infrared Survey Explorer (WISE) space telescope.

[wayti-blog]

Striking new Webb image showing alignment of bipolar jets confirms star formation theories

(Credit: NASA, ESA, CSA, STScI, K. Pontoppidan (NASA's Jet Propulsion Laboratory), J. Green (Space Telescope Science Institute))

"For the first time, a phenomenon astronomers have long hoped to image directly has been captured by the NASA/ESA/CSA James Webb Space Telescope's Near-InfraRed Camera (NIRCam). In this stunning image of the Serpens Nebula, the discovery lies in the northern area of this young, nearby star-forming region.

The astronomers found an intriguing group of protostellar outflows, formed when jets of gas spewing from newborn stars collide with nearby gas and dust at high speeds. Typically, these objects have a variety of orientations within one region. Here, however, they are all slanted in the same direction, to the same degree, like sleet pouring down during a storm."

"So, just how does the alignment of the stellar jets relate to the rotation of the star? As an interstellar gas cloud collapses in on itself to form a star, it spins more rapidly. The only way for the gas to continue moving inward is for some of the spin (known as angular momentum) to be removed.

A disk of material forms around the young star to transport material down, like a whirlpool around a drain. The swirling magnetic fields in the inner disk launch some of the material into twin jets that shoot outward in opposite directions, perpendicular to the disk of material."

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