Grains of cosmic dust streaked through night skies in early May. Swept up as planet Earth plowed through the debris streams left behind by periodic Comet Halley, the annual meteor shower is known as the Eta Aquarids. This year, the Eta Aquarids peak was visually hampered by May's bright Full Moon, though. But early morning hours surrounding last May's shower of Halley dust were free of moonlight interference. In exposures recorded between April 28 and May 8 in 2022, this composited image shows nearly 90 Eta Aquarid meteors streaking from the shower's radiant in Aquarius over San Pedro de Atacama, Chile. The central Milky Way arcs above in the southern hemisphere's predawn skies. The faint band of light rising from the horizon is Zodiacal light, caused by dust scattering sunlight near our Solar System's ecliptic plane. Along the ecliptic and entrained in the Zodiacal glow are the bright planets Venus, Jupiter, Mars, and Saturn. Of course Mars itself has recently been found to be a likely source of the dust along the ecliptic responsible for creating Zodiacal light.

Source: NASA

Charon is 1,214 kilometers (754 miles) across. That's about 1/10th the size of planet Earth but a whopping 1/2 the diameter of Pluto itself, and makes it the largest satellite relative to its parent body in the Solar System. Still, the moon appears as a small bump at about the 1 o'clock position on Pluto's disk in the grainy, negative,telescopic picture inset at upper left. That view was used by James Christy and Robert Harrington at the U.S. Naval Observatory in Flagstaff to discover Charon in June of 1978.

A darkened and mysterious north polar region known to some as Mordor Macula caps this premier high-resolution view. The portrait of Charon, Pluto's largest moon, was captured by New Horizons near the spacecraft's closest approach on July 14, 2015. The combined blue, red, and infrared data was processed to enhance colors and follow variations in Charon's surface properties with a resolution of about 2.9 kilometers (1.8 miles).

Source: NASA

his tantalizing trio of galaxies sometimes called the Draco Group, is located in the northern constellation of Draco, the Dragon all found within this single telescopic field of view that spans a little more than the width of the full moon.

A mere 390 light-years away, Sun-like stars and future planetary systems are forming in the Rho Ophiuchi molecular cloud complex, the closest star-forming region to our fair planet. The James Webb Space Telescope's NIRCam peered into the nearby natal chaos to capture this infrared image at an inspiring scale.

An increase in surface activity is expected because our Sun is approaching solar maximum in 2025. However, last month our Sun sprouted more sunspots than in any month during the entire previous 11-year solar cycle -- and even dating back to 2002. The featured picture is a composite of images taken every day from January to June by NASA's Solar Dynamic Observatory. Showing a high abundance of sunspots, large individual spots can be tracked across the Sun's disk, left to right, over about two weeks. As a solar cycle continues, sunspots typically appear closer to the equator. Sunspots are just one way that our Sun displays surface activity -- another is flares and coronal mass ejections (CMEs) that expel particles out into the Solar System. Since these particles can affect astronauts and electronics, tracking surface disturbances is of more than aesthetic value. Conversely, solar activity can have very high aesthetic value -- in the Earth's atmosphere when they trigger aurora.

If our Sun were part of this star cluster, the night sky would glow like a jewel box of bright stars. This cluster, known as M53 and cataloged as NGC 5024, is one of about 250 globular clusters that survive in our Galaxy. Most of the stars in M53 are older and redder than our Sun, but some enigmatic stars appear to be bluer and younger. These young stars might contradict the hypothesis that all the stars in M53 formed at nearly the same time. These unusual stars are known as blue stragglers and are unusually common in M53. After much debate, blue stragglers are now thought to be stars rejuvenated by fresh matter falling in from a binary star companion. By analyzing pictures of globular clusters like the featured image taken by the Hubble Space Telescope, astronomers use the abundance of stars like blue stragglers to help determine the age of the globular cluster and hence a limit on the age of the universe. M53, visible with a binoculars towards the constellation of Bernice's Hair (Coma Berenices), contains over 250,000 stars and is one of the furthest globulars from the center of our Galaxy.

Source: NASA

This shows the Messier 16 Eagle Nebula region of the sky in true color, without the use of any filter. This region is most often captured in narrowband. You can see the wings of the eagle spanning in rich hydrogen alpha gas, and the bright stars lighting up the famous Pillars of Creation.

Source: Antoine Grelin

I have a Nikon D7100 and I am in love with my 35mm 1.8/f prime. On the crop sensor it gives such a natural image that I find myself using it over anything else. I am in the market for a new wide angle lens, something in the 12mm range, though.

Deep in the South constellation Apus lies a truly spectacular field of nebulosity. Not far from the South Celestial Pole (at declination -80º), this nebula is very rarely captured, especially in full colour. This image shows a region catalogued by Steve Mandel and Michael Wilson in early 2000s as the 9th and last entry to their "Catalogue of Unexplored Nebulae" [1]. This pioneering project identified the interstellar clouds in optical light, before only known to professional astronomers through infrared surveys. Mandel named the nebulae Integrated Flux Nebula, or IFN, a name that is frequently quoted in amateur astrophotography, but seldomly used in professional astronomy, where "galactic cirrus" is preferred.

The Galactic Cirri are veils that surround our galaxy – made of dust and gas in the interstellar space. It was first noticed on optical glass plates recorded at Palomar Observatory and subsequently cataloged by B. T. Lynds, in 1965. In the 2000s, Steve Mandel noticed faint cirrus in deep, wide field photographs near the North Celestial Pole, and labelled the nebulosity as the IFN, or the Integrated Flux Nebula. [2] It has incredibly low surface brightness, at ~22-28 mag/arcsec² (fainter than the darkest sky background on Earth), thus it is not easy to capture!

Source: Gabriel Santos

A spiral galaxy with a small central bar, M66 is a member of the Leo Galaxy Triplet, a group of three galaxies about 30 million light years from us. The Leo Triplet is a popular target for relatively small telescopes, in part because M66 and its galactic companions M65 and NGC 3628 all appear separated by about the angular width of a full moon. The featured image of M66 was taken by Hubble to help investigate the connection between star formation and molecular gas clouds. Clearly visible are bright blue stars, pink ionized hydrogen clouds -- sprinkled all along the outer spiral arms, and dark dust lanes in which more star formation could be hiding.

Source: NASA

The growth of this community continues to amaze me. We've made this the premier Space-related sub on Lemmy and continue to bring in new user's at a huge pace. There's a continued increase in user contribution as well and it's great seeing the different celestial objects or image types that different users prefer.

Please continue to post and comment so we can continue to make this an exciting and welcoming community.

Also, if you're new here, know that this is a friendly place that you should feel comfortable joining. Please remember to share your suggestions, I want this community to be active and reflect what the user's want it to be.

Thanks and continue being awesome.