Pic of the Week: Eyeing the Ring Nebula

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Image (Credit): The Ring Nebula as captured by the JWST. (ESA/Webb, NASA, CSA, M. Barlow (University College London), N. Cox (ACRI-ST), R. Wesson (Cardiff University))

This week’s image comes from the Jame Webb Space Telescope’s (JWST) Near-Infrared Camera (NIRCam). It shows the Ring Nebula, which is approximately 2,500 light-years away. It looks like a heavenly eyeball. with an Earth-colored iris.

Here is more on the image from NASA:

The NASA/ESA/CSA James Webb Space Telescope has observed the well-known Ring Nebula with unprecedented detail. Formed by a star throwing off its outer layers as it runs out of fuel, the Ring Nebula is an archetypal planetary nebula. Also known as M57 and NGC 6720, it is both relatively close to Earth at roughly 2,500 light-years away. This new image provides unprecedented spatial resolution and spectral sensitivity. For example, the intricate details of the filament structure of the inner ring are particularly visible in this dataset. There are some 20,000 dense globules in the nebula, which are rich in molecular hydrogen. In contrast, the inner region shows very hot gas. The main shell contains a thin ring of enhanced emission fromcarbon-based molecules known as polycyclic aromatic hydrocarbons (PAHs). Roughly ten concentric arcs are located just beyond the outer edge of the main ring. The arcs are thought to originate from the interaction of the central star with a low-mass companion orbiting at a distance comparable to that between the Earth and the dwarf planet Pluto. In this way, nebulae like the Ring Nebula reveal a kind of astronomical archaeology, as astronomers study the nebula to learn about the star that created it.

Pic of the Week: Dusty Spiral Arms of NGC 1087

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Image (Credit): NGC 1087 as captured by the Hubble Space Telescope. (Space Telescope Science Institute and Gladys Kober, NASA/Catholic University of America)

This week’s image comes from the NASA/ESA Hubble Space Telescope.  It is an image of the grainy-textured, colorful barred spiral galaxy NGC 1087, which is about 80 million light-years away.

Here is more about the galaxy from NASA:

It has a diameter of 87,000 light-years and a very small nucleus, or center. The galaxy’s dust lanes, seen in dark red, help define its spiral structure. NGC 1087’s stellar bar – the elongated, bright-white structure at the galaxy’s center – is also shorter compared to other barred galaxies. Typically, in barred galaxies, the gravity of the center pulls in large quantities of gas, causing a burst of star formation followed by a slow decay. Uniquely, NGC 1087 shows signs of new star formation, making it of special interest to scientists.

British astronomer William Herschel discovered NGC 1087 in 1785. The galaxy sits just south of the celestial equator, making it visible from both hemispheres. In 1995, astronomers discovered a Type II supernova within this galaxy. Type II supernovae occur when a massive star uses all of its nuclear fuel and its iron core collapses, then explodes. Named 1995V, it is the only supernova ever seen in this galaxy.

In this new ultraviolet, visible, and near-infrared light image from NASA’s Hubble Space Telescope, the dark red streaks are cold molecular gas, the raw material from which stars form. The spots of bright pink signal areas where new stars are forming, characterized by the presence of ionized hydrogen, oxygen, and sulfur. The bluer regions hold hot, young stars formed earlier in the lifetime of this galaxy. Hubble observed NGC 1087 to study the connection between young stars and cold gas, and especially to determine what happens to gaseous regions after stars are formed within them.

Pic of the Week: Herbig-Haro 211

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Image (Credit): Herbig-Haro 211 as captured by the JWST.

This week’s image is from the James Webb Space Telescope (JWST). It shows a colorful and expansive Herbig-Haro 211, with a Herbig-Haro (HH) being “…luminous regions surrounding newborn stars, formed when stellar winds or jets of gas spewing from these newborn stars form shock waves colliding with nearby gas and dust at high speeds.”

NASA explains what we are seeing:

This image of HH 211 from NASA’s James Webb Space Telescope reveals an outflow from a Class 0 protostar, an infantile analog of our Sun when it was no more than a few tens of thousands of years old and with a mass only 8% of the present-day Sun (it will eventually grow into a star like the Sun).

Infrared imaging is powerful in studying newborn stars and their outflows, because such stars are invariably still embedded within the gas from the molecular cloud in which they formed. The infrared emission of the star’s outflows penetrates the obscuring gas and dust, making a Herbig-Haro object like HH 211 ideal for observation with Webb’s sensitive infrared instruments. Molecules excited by the turbulent conditions, including molecular hydrogen, carbon monoxide, and silicon monoxide, emit infrared light that Webb can collect to map out the structure of the outflows.

The image showcases a series of bow shocks to the southeast (lower-left) and northwest (upper-right) as well as the narrow bipolar jet that powers them. Webb reveals this scene in unprecedented detail — roughly 5 to 10 times higher spatial resolution than any previous images of HH 211. The inner jet is seen to “wiggle” with mirror symmetry on either side of the central protostar. This is in agreement with observations on smaller scales and suggests that the protostar may in fact be an unresolved binary star.

Pic of the Week: Shackleton Crater

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Image (Credit): Shackleton Crater on the lunar surface. (Mosaic created by LROC and ShadowCam teams with images provided by NASA/KARI/ASU)

This week’s image shows the Shackleton Crater located at the Moon’s South Pole. To create what you see above, an image from NASA’s Lunar Reconnaissance Orbiter Camera (LROC) was combined with another image from ShadowCam, a NASA instrument on board a KARI (Korea Aerospace Research Institute) spacecraft called Danuri,

Here is more information from NASA concerning the two cameras:

LROC can capture detailed images of the lunar surface but has limited ability to photograph shadowed parts of the Moon that never receive direct sunlight, known as permanently shadowed regions. ShadowCam is 200-times more light-sensitive than LROC and can operate successfully in these extremely low-light conditions, revealing features and terrain details that are not visible to LROC. ShadowCam relies on sunlight reflected off lunar geologic features or the Earth to capture images in the shadows.

ShadowCam’s light sensitivity, however, renders it unable to capture images of parts of the Moon that are directly illuminated, delivering saturated results. With each camera optimized for specific lighting conditions found near the lunar poles, analysts can combine images from both instruments to create a comprehensive visual map of the terrain and geologic features of both the brightest and darkest parts of the Moon. The permanently shadowed areas in this mosaic, such as the interior floor and walls of Shackleton Crater, are visible in such detail because of the imagery from ShadowCam. In contrast, the sunlit areas in this mosaic, like the rim and flanks of the crater, are a product of imagery collected by LROC.

Pic of the Week: Cosmic Smokescreen

Posted on by onespaceman2000
Image (Credit): NGC 6530 as captured by the NASA/ESA Hubble Space Telescope. (ESA/Hubble & NASA, ESO, O. De Marco)

This week’s image is from the Hubble Space Telescope. It shows a fantastic array of colors from a portion of NGC 6530, which is about 4,350 light-years from Earth.

Here is more about this image from the European Space Agency (ESA):

A portion of the open cluster NGC 6530 appears as a roiling wall of smoke studded with stars in this image from the NASA/ESA Hubble Space Telescope…The cluster is set within the larger Lagoon Nebula, a gigantic interstellar cloud of gas and dust. It is the nebula that gives this image its distinctly smokey appearance; clouds of interstellar gas and dust stretch from one side of this image to the other.

You can also watch this short video that pans over the cluster.