Starship Asterisk*

Image Credit: ESA/Hubble, A. Riess et al., J. Greene

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Meet NGC 5728, a spiral galaxy around 130 million light-years from Earth. This image was captured using Hubble’s Wide Field Camera 3 (WFC3), which is extremely sensitive to visible and infrared light. Therefore, this image beautifully captures the regions of NGC 5728 that are emitting visible and infrared light. However, there are many other types of light that galaxies such as NGC 5728 can emit, which WFC3 cannot see.

In this image, NCG 5728 appears to be an elegant, luminous, barred spiral galaxy. What this image does not show, however, is that NGC 5728 is also a monumentally energetic type of galaxy, known as a Seyfert galaxy. This extremely energetic class of galaxies are powered by their active cores, which are known as active galactic nuclei (AGNs). There are many different types of AGNs, and only some of them power Seyfert galaxies. NGC 5728, like all Seyfert galaxies, is distinguished from other galaxies with AGNs because the galaxy itself can be seen clearly. Other types of AGNs, such as quasars, emit so much radiation that it is almost impossible to observe the galaxy that houses them. As this image shows, NGC 5728 is clearly observable, and at optical and infrared wavelengths it looks quite normal. It is fascinating to know that the galaxy’s centre is emitting vast amounts of light in parts of the electromagnetic spectrum that WFC3 just isn’t sensitive to! Just to complicate things, the AGN at NGC 5728’s core might actually be emitting some visible and infrared light — but it may be blocked by the dust surrounding the galaxy’s core.

Image Credit: ESO/Yuri Beletsky (LCO)

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The low twilight Sun highlights the clouds hanging over the Chilean Atacama landscape in this Picture of the Week, bathing the scene in deep, fiery red light. The image is dominated by the Purico Complex, a clump of volcanic mountains whose highest peak reaches a whopping 5703 metres in elevation! A single vehicle is visible on the remote road below, kicking up a stream of opaque dust in its wake, and towards the left of the image is a cluster of buildings...and a single antenna.

This is the ESO-operated Atacama Pathfinder Experiment (APEX), one of the highest telescopes in the world. APEX is designed to work at submillimetre wavelengths between infrared light and radio waves, which are key to revealing some of the coldest, dustiest, and most distant objects in the Universe. Over the years, it has explored a wide range of astronomical phenomena, probing the wild early lives of today’s most massive galaxies, studying matter torn apart by a supermassive black hole, and mapping the plane of the Milky Way.

Because submillimetre radiation from space is heavily absorbed by water vapour in the Earth's atmosphere, it is best to observe it from high altitudes — hence APEX’s location. The experiment can be found at an altitude of 5100 metres, up on the Chajnantor plateau in Chile’s Atacama Desert. This desert is one of the driest places on Earth, and as such offers unsurpassed views of the cosmos. The site is also home to the Atacama Large Millimeter/submillimeter Array (ALMA), the world's largest ground-based facility for observations in the millimetre/submillimetre regime. ALMA’s 66 high-precision antennas are not visible in this image; they are scattered across the plateau behind the photographer.

Image Credit: ESA/Hubble and NASA, R. Cohen

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This sparkling starfield, captured by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3) and Advanced Camera for Surveys (ACS), contains the globular cluster ESO 520-21 (also known as Palomar 6). A densely packed, roughly spherical collection of stars, it lies close to the centre of the Milky Way, where interstellar gas and dust absorb starlight and make observations more challenging.

This absorption by interstellar material affects some wavelengths of light more than others, changing the colours of astronomical objects and causing them to appear redder than they actually are. Astronomers call this process “reddening”, and it makes determining the properties of globular clusters close to the galactic centre — such as ESO 520-21 — particularly difficult.

ESO 520-21 lies in the constellation Ophiuchus, near the celestial equator. Ophiuchus was one of the 48 constellations which appeared in the writings of the second-century Egyptian astronomer Ptolemy, all of which are among the 88 constellations officially recognised by the International Astronomical Union today. Not all the constellations proposed by astronomers throughout history have survived, however — forgotten or obsolete constellations include Felis (the Cat), Rangifer (the Reindeer), and even Officina Typographica (the Printer’s Workshop).

Image Credit: R. Lucchesi/ESO

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In this Picture of the Week, taken by drone, you can see nearly all of the telescopes at ESO’s La Silla Observatory snaking along the top of the 2400-metre saddle-shaped mountain and into the distance. One for the La Silla family album!

La Silla is located on the outskirts of Chile’s Atacama Desert, far from human-made light pollution in an area famed for its dark, clear skies. It was ESO’s first observatory, inaugurated in 1969, and remains at the forefront of astronomy today, with around 300 scientific papers using observations from La Silla telescopes published every year.

The most prominent telescope in this image is the ESO 3.6-metre telescope, home to the world's foremost exoplanet hunting instrument: the High Accuracy Radial velocity Planet Searcher, or HARPS. Thanks to the observations made with HARPS, astronomers have worked out that there are likely billions of rocky planets in the temperate zones around red dwarfs in the Milky Way, worlds that could potentially be home to life outside the Solar System.

Click to view full size image 1 or image 2

Credit: ESA/Hubble and NASA, A. Nota, C. Britt

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This Picture of the Week showcases new views of the dual nature of the star AG Carinae, which was the target of the NASA/ESA Hubble Space Telescope’s 31st anniversary image in April 2020. This new perspective was developed thanks to Hubble’s observations of the star in 2020 and 2014, along with others captured by the telescope’s WFPC2 instrument in 1994. ...

The first image showcases the details of the ionised hydrogen and ionised nitrogen emissions from the nebula (seen here in red). In the second image, the blue demonstrates the contrasting appearance of the distribution of the dust that shines of reflected stellar light. Astronomers believe that the dust bubbles and filaments formed within and were shaped by powerful stellar wind.

This giant star is waging a tug-of-war between gravity and radiation to avoid self-destruction. The star is surrounded by an expanding shell of gas and dust — a nebula — that is shaped by the powerful winds emanating from the star. The nebula is about five light-years wide, equal to the distance from here to our nearest star, Alpha Centauri.

AG Carinae is formally classified as a Luminous Blue Variable because it is hot (blue), very luminous, and variable. Such stars are quite rare because there are not many stars that are so massive. Luminous Blue Variable stars continuously lose mass in the final stages of their life, during which a significant amount of stellar material is ejected into the surrounding interstellar space, until enough mass has been lost that the star has reached a stable state. ...

Credit: P. Horálek & J. C. Casado / ESO

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Looking at this photo might make you feel a little topsy-turvy! This Picture of the Week captures both the Northern and Southern Hemisphere at once — the whole night’s sky in one mind-bending image — something that would be impossible to see in real life.

To create this image, photographers Petr Horálek and Juan Carlos Casado took two pictures at observatories located at the same latitudes in the Northern and Southern Hemispheres. The top half is a photo taken at the Instituto de Astrofísica de Canarias’ Roque de los Muchachos Observatory in La Palma in the Canary Islands, 29 degrees north of the equator, whilst the bottom half was taken at ESO’s La Silla Observatory in Chile’s Atacama Desert, 29 degrees south of the equator. When digitally stitched together, they create a continuous sweeping view of the night’s sky.

One of the most noticeable features in this picture is the eerie white glow radiating out vertically from its centre. This is the zodiacal light, a phenomenon caused by dust that pervades our Solar System scattering sunlight, which is only visible in areas with extremely dark skies free from light pollution. Shining brightly in the beam of the Northern Hemisphere Zodiacal Light is the planet Venus.

The bottom image shows several of the telescopes at La Silla, including the ESO 1-metre Schmidt telescope in the foreground. The reflective mirror seen upside-down in the top image is part of the Cherenkov Telescope Array (CTA), a group of gamma-ray telescopes observing some of the most energetic phenomena in the universe. A second array will be installed in the southern hemisphere close to ESO’s Paranal Observatory, via an agreement between CTA Observatory and ESO.