ESA Hubble and Webb Space Telescopes

ESA Hubble and Webb Space Telescopes

Research Services

Official ESA account for the #Hubble Space Telescope and the James #Webb Space Telescope.

About us

Official ESA account for the #Hubble Space Telescope and the James #Webb Space Telescope. Find us on esahubble.org and esawebb.org

Website
https://esahubble.org/
Industry
Research Services
Company size
11-50 employees
Headquarters
Baltimore
Type
Nonprofit

Locations

Employees at ESA Hubble and Webb Space Telescopes

Updates

  • 🆕 The NASA/ESA/CSA James Webb Space Telescope has imaged a cold exoplanet 12 light-years away! 🔴 Astronomers had previously taken indirect measurements of the star Epsilon Indi A ⭐ which hinted at a giant planet ‘tugging’ on it. They then observed the exoplanet directly with Webb. 🔴 Previously imaged exoplanets tend to be the youngest, hottest exoplanets, still radiating much of the energy from their formation. As they cool and contract, they become fainter, with most of their emission in the mid-infrared. 🔴 With its #MIRI and its large mirror, Webb is well-equipped for imaging colder exoplanets! 🔴 This planet, Epsilon Indi Ab, is one of the coldest exoplanets directly detected 🥶 and more similar to Jupiter than any other imaged yet – so it provides a rare opportunity to study the atmospheres of true solar system analogues. Read more about it here: https://ow.ly/gRB950SJ0J9 #WebbSeesFarther 📷 ESA/Webb, NASA, CSA, STScI, E. Matthews (Max Planck Institute for Astronomy)

    • This image shows the exoplanet Epsilon Indi Ab. Blue scale-like features are visible in the background, with the host star’s light being blocked by a black circle in the centre of the image (indicated by a dashed-line and white star visual overlaid on the image). The exoplanet is visible on the left as a bright orange circle.
  • Our ESA/Hubble Picture of the Week features an island universe! 🏝️ NGC 3430 is a spiral galaxy which lies 100 million light-years from Earth. That it is such a fine spiral may be why it ended up as part of the sample that Edwin Hubble used to define his classification of galaxies. In 1926, Hubble wrote a paper classifying 400 galaxies by their appearance. The study of galaxies was in its infancy then, and Hubble referred to them as ‘extragalactic nebulae’ in his paper. Once it became clear that they were very different from nebulae, the favoured term became ‘island universe’. NGC 3430 may look as if it still deserves that name, but today we simply call it another galaxy 🌌 Read more: https://ow.ly/zrPP50SHTO8 📷 ESA/Hubble, NASA,C. Kilpatrick

    • A spiral galaxy with three prominent arms wrapping around it, and plenty of extra gas and dark dust between the arms. There are shining blue points throughout the arms and some patches of gas out beyond the galaxy’s edge, where stars are forming. The centre of the galaxy also shines brightly. It is on a dark background where some small orange dots mark distant galaxies.
  • 🆕 This artist’s concept shows how WASP-39 b could look 🔵 based on observations from telescopes including the NASA/ESA/CSA James Webb Space Telescope. WASP-39 b is a hot, puffy gas giant orbiting a star slightly smaller than the Sun. It is tidally locked, with one side always facing its star, so it has a terminator (boundary) where there is eternal sunrise and sunset 🌅 Using a transmission spectrum of WASP-39 b from Webb’s #NIRSpec, astronomers confirmed a temperature difference between morning and evening, with the evening appearing hotter by 200°C. Read more about it here: https://ow.ly/Kqum50SBqKF #WebbSeesFarther Artist's impression: NASA, ESA, CSA, R. Crawford (STScI)

    • Illustration of a planet, zoomed in on the planet’s dayside/nightside boundary. The planet encompasses takes up the full image. At the bottom left, the image is dark, depicting the nightside covering the planet in a dark shadow. In the right side of the image, the planet has a fuzzy orange-pink atmosphere with hints of longitudinal wispy cloud bands. The right upper corner is bright, where the star (not illustrated) shines.
  • Our ESA/Hubble Picture of the Week features the dwarf irregular galaxy NGC 5238. Its blobby appearance belies a complex structure which has been the subject of much astronomical research. NGC 5238 is theorised to have had a recent close encounter with another galaxy – the evidence for this is the tidal distortions of NGC 5238’s shape, the kind produced by two galaxies pulling on each other. The culprit was likely to be a satellite galaxy that was devoured by NGC 5238. Traces of it might be found by examining the stars in NGC 5238 ⭐ a task for which the NASA/ESA Hubble Space Telescope is perfectly suited! Read more: https://ow.ly/yetZ50SBc7T 📷 ESA/Hubble , NASA, F. Annibali

    • A dwarf irregular galaxy. It appears as a cloud of bluish gas, filled with point-like stars that also spread beyond the edge of the gas. A few glowing red clouds sit near its centre. Many other objects can be seen around it: distant galaxies in the background, four-pointed stars in the foreground, and star clusters that are part of the galaxy - shining spots surrounded by more tiny stars.
  • 🆕 A penguin portrait to mark the second science anniversary of the NASA/ESA/CSA James Webb Space Telescope 🎉 🔴 This duo of interacting galaxies – the Penguin and the Egg 🐧🥚 – are locked in a cosmic dance, and will merge into a single galaxy over hundreds of millions of years. 🔴 The Penguin was once spiral-shaped. Now, its centre gleams like an eye and its arms resemble a beak, head, backbone, and tail. The Egg pulls its thinner areas of gas and dust, causing them to crash in waves and form stars. 🔴 The Egg’s compact shape, however, remains largely unchanged. As an elliptical galaxy, it is filled with ageing stars ⭐ and has much less gas and dust that can be pulled away to form new stars. 🔴 The detail in this image – the haze joining the Penguin and the Egg, and the distant galaxies – is a testament to the sensitivity and resolution of Webb’s infrared instruments. 🔴 In the top right of the image is a quite edge-on young galaxy, teeming with new, blue stars. Since the galaxy’s stellar population is so young, it ‘vanishes’ in Webb's mid-infrared light view. 🔴 Webb’s operations over the last two years have helped astronomers make discoveries about other worlds, the lives of stars, the early Universe, and galactic evolution – helping solve longstanding mysteries, and producing beautiful images like this one! Read more about it here: https://ow.ly/6bcR50SAoFc #WebbSeesFarther 📷 NASA, ESA, CSA, STScI

    • Two interacting galaxies known as Arp 142. At left is NGC 2937, nicknamed the Egg for its appearance. At right is NGC 2936, nicknamed the Penguin for its appearance. The latter’s beak-like region points toward and above the Egg.
  • The Draco dwarf galaxy, as seen by the NASA/ESA Hubble Space Telescope 🐲 This image shows three different perspectives of the Draco dwarf spheroidal galaxy, which is located 250,000 light-years from Earth. Hubble observed the galaxy over 18 years. This helped astronomers build an accurate 3D map of the movement of the stars within it 🌠 and shed light on dark matter – the Universe’s invisible ‘glue’. Read more: https://ow.ly/ajRF50SzxBj 📷 NASA, ESA, Digitized Sky Survey, Roeland van der Marel (STScI)

    • At left is the main image: a wide-field view of the galaxy from the Digitized Sky Survey. Many yellow, blue-white, and white stars are dispersed across the black background of space. A faint brown oval surrounds the central area of the image. Within this area are two small graphic overlays: a square and a diamond. These two small overlays correspond to the two magnified views at right, as seen by the Hubble Space Telescope. The small square in the main image corresponds to the top right square. The small diamond in the main image corresponds to the bottom right square. The magnified view at top right shows a large white circle with four diffraction spikes in the top left. Small white specks and orange dots are scattered across the black background. A large spiral galaxy is seen face-on at top right. The magnified view at bottom right shows small white specks and orange dots scattered across the black background.
  • The NASA/ESA Hubble Space Telescope has found evidence for an intermediate-mass black hole (IMBH) in Omega Centauri! 🕳️ 🔴 IMBHs are the ‘missing link’ in black hole evolution, with only a few IMBH candidates ever discovered. If they exist, how common are they? How do they form? And can they grow into supermassive black holes? 🔴 Omega Centauri is the largest and brightest globular cluster in the sky. It is distinct from other globular clusters as it rotates relatively quickly, appears flattened, and is almost as massive as a small galaxy. 🔴 Astronomers tracked stars in Omega Centauri using hundreds of Hubble images, and discovered seven stars that shouldn’t be there 🌠 they are moving so fast they should have escaped the cluster forever. 🔴 The most likely explanation is that the gravity of a massive object is keeping them close – an IMBH with a mass at least 8200 times that of our Sun. Read more: https://ow.ly/qiTH50SyCXP 📷 ESA/Hubble, NASA, M. Häberle

    • A globular cluster, appearing as a highly dense and numerous collection of shining stars. Some appear a bit larger and brighter than others, with the majority of stars appearing blue and orange. They are scattered mostly uniformly, but in the centre they crowd together more and more densely, and merge into a stronger glow at the cluster’s core.
  • Distance or dust? 🤔 Our ESA/Hubble Picture of the Week features the galaxy NGC 3810, which was host to a Type Ia supernova in 2022. 🔴 Type Ia supernova are used to measure astronomical distance. These supernovae have a very consistent brightness 💥 so we can tell how far away they are from how dim they appear. 🔴 But this is complicated by intergalactic dust between Earth and the supernova – how much of the reduction in brightness is distance, and how much is dust? 🔴 The NASA/ESA Hubble Space Telescope can help by photographing the same supernova in ultraviolet light (blocked by dust) and infrared light (not blocked by dust)! Some of the data used to make this image of NGC 3810 were focused on its 2022 supernova. Read more: https://ow.ly/cB6J50SwGJ0 📷 ESA/Hubble, NASA, D. Sand, R. Foley

    • A spiral galaxy seen almost face-on. Large spiral arms whirl out from its centre, filling the scene. They glow faintly blue from the stars within, with some small bright patches of blue and pink marking areas of star formation. They are overlaid with thin filaments of dark reddish dust that block light. The galaxy’s centre shines brightly white.
  • 🆕 Webb brings you a jewelled ring! Our ESA/Webb Picture of the Month features the gravitational lensing of a quasar! 🔍 🔴 RX J1131-1231 lies six billion light-years from Earth in the constellation Crater. Its curious portrait was captured by the NASA/ESA/CSA James Webb Space Telescope’s #MIRI 🔴 It is one of the best lensed quasars ever discovered – the foreground galaxy smears the image of it into a bright arc and creates four images of the object, giving the appearance of a jewelled ring 💍 🔴 Lensing allows us to study regions close to the black hole in distant quasars. Measurements of the X-ray emission from quasars indicates how fast the central black hole is spinning, providing clues about how black holes grow. 🔴 Observations suggest that the black hole in this quasar has grown via mergers, rather than pulling in material from many different directions. Read more about it here: https://ow.ly/X1iw50SvL4E #WebbSeesFarther 📷 ESA/Webb, NASA, CSA, A. Nierenberg

    • A small image of a galaxy distorted by gravitational lensing into a dim ring. At the top of the ring are three very bright spots with diffraction spikes coming off them, right next to each other: these are copies of a single quasar in the lensed galaxy, duplicated by the gravitational lens. In the centre of the ring, the elliptical galaxy doing the lensing appears as a small blue dot. The background is black and empty.

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