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SciGleam, Buenos Aires, 1102, Sanaa (2026)

01/06/2026

The Headphones Nebula in Lynx

The Headphones Nebula is a planetary nebula discovered in 1939 by Rebecca Jones and Richard Emberson. Located in the constellation Lynx about 1600 light years from Earth, this faint and uniquely shaped nebula represents the final evolutionary stage of a dying Sun like star, casting off its outer layers into space. This image was captured using a Celestron 8 inch HD Edge telescope and a ZWO 2600mc camera, built from 24 exposures of 600 seconds for a total of 4 hours at Starfront Observatories.

SciGleam Highlights

A rare planetary nebula with a distinctive shape that gives it the Headphones nickname

Located about 1600 light years away marking the late life stage of a Sun like star

Long exposure imaging reveals faint structure and delicate outer shells

Credit Bob Rossiter

01/06/2026

Hydrogen Symphony in Monoceros

A rich field of glowing hydrogen emission in Monoceros reveals the delicate structure of ionized gas spread across a star forming region. The soft red glow and layered detail bring out the quiet power of interstellar hydrogen shaped by nearby hot stars.

SciGleam Highlights

A hydrogen rich emission scene in Monoceros

Shows the glow of ionized gas in a star forming region

A fine example of subtle structure revealed through deep exposure imaging

Credit Piotr Czerski

01/06/2026

Orion Nebula M42 in Orion

The Orion Nebula also known as Messier 42 is one of the closest and most studied star forming regions in the night sky located about 1300 light years away in the constellation Orion. This vast cloud of glowing gas and dust is a stellar nursery where new stars are actively forming and illuminating their surroundings with intense radiation.

At its heart lies the Trapezium Cluster a group of hot young stars that energize the nebula and shape its intricate structure. Bright filaments dark dust lanes and expanding gas reveal the dynamic processes of star birth making the Orion Nebula a cornerstone object for understanding how stars and planetary systems form.

SciGleam Highlights

A nearby stellar nursery about 1300 light years away in Orion

Home to the Trapezium Cluster which powers the nebula glow

A key region for studying star and planet formation in real time

Credit Robert Gendler

31/05/2026

Comet C2025 R3 Over West Virginia Skies

In the quiet predawn hours of April 10 2026 Comet C2025 R3 was captured rising above the horizon at Calhoun County Park West Virginia. This icy visitor reveals a delicate glow and subtle tail structure as sunlight begins to interact with its coma, offering a fleeting glimpse of a traveler from the outer Solar System. The image was taken using a 135mm Rokinon lens paired with a ZWO 2600mc color camera.

SciGleam Highlights

A rare capture of Comet C2025 R3 during its early morning above the horizon

Shows the faint coma and developing tail shaped by solar radiation

Represents a short lived celestial event preserved through astrophotography

Credit Bob Rossiter

31/05/2026

Heart of the Lagoon Nebula

The heart of the Lagoon Nebula reveals a glowing region of gas and dust shaped by powerful young stars. This deep sky view captures the bright energy and intricate structure at the core of one of the sky’s most beautiful stellar nurseries.

SciGleam Highlights

A vivid look into the central region of the Lagoon Nebula

Shows active star formation within glowing interstellar gas

A rich scene of texture color and cosmic structure

Credit Jason Marriott

31/05/2026

Wizard Nebula NGC 7380 in Cepheus

The Wizard Nebula also known as NGC 7380 is an emission nebula about 7200 light years away in the constellation Cepheus. It surrounds a young open star cluster around 4 million years old where hot massive stars flood the region with ultraviolet radiation causing the surrounding hydrogen gas to glow with rich red light.

Spanning roughly 100 light years this active stellar nursery appears about the size of the full Moon in the sky. The complex structure of gas and dust reveals ongoing star formation shaped by radiation and stellar winds. It was first discovered by Caroline Herschel in 1787 and remains a striking example of how young stars illuminate and sculpt their birth clouds.

SciGleam Highlights

A glowing emission nebula about 7200 light years away in Cepheus

Powered by a young cluster of stars around 4 million years old

Ionized hydrogen gas produces the vivid red glow of active star formation

Credit Nicolas Rolland

30/05/2026

Bodes Galaxy and the Cigar Galaxy in a Sea of Integrated Flux Nebula

M81 known as Bodes Galaxy and M82 the Cigar Galaxy appear surrounded by faint wisps of Integrated Flux Nebula, a delicate glow of interstellar dust illuminated by the combined light of stars across the Milky Way. Though nearly invisible to the naked eye, this diffuse structure becomes visible through long exposure astrophotography, revealing a hidden layer of our cosmic environment. This image was captured using a 135mm Rokinon lens with a ZWO 2600mc pro at f2.0, built from 150 exposures of 120 seconds for a total integration time of 5 hours.

SciGleam Highlights

Showcases M81 and M82 embedded within the faint and rarely seen Integrated Flux Nebula

Reveals interstellar dust illuminated by the collective light of the Milky Way

Demonstrates the power of long exposure imaging to uncover extremely low brightness structures

Credit Bob Rossiter

30/05/2026

M81 and M82

M81 and M82 are a famous galaxy pair in Ursa Major, often seen together in wide field astrophotography. M81 is a graceful spiral galaxy while M82 is a vibrant starburst galaxy shaped by intense activity and interaction between the two systems.

SciGleam Highlights

A classic interacting galaxy pair in Ursa Major

M81 shows a bright spiral structure with a prominent core

M82 stands out as an active starburst galaxy with dramatic dust and gas detail

Credit Ján Gajdoš

Slovakia

30/05/2026

Butterfly Galaxies in Virgo

These two galaxies lie about 60 million light years away in the constellation Virgo and are beginning to collide and merge. Their close encounter is slowly reshaping both systems and will eventually produce a single giant elliptical galaxy much like the fate expected for the Milky Way when it meets Andromeda. Known as the Siamese Twins for their striking visual closeness their cores are separated by about 20,000 light years.

SciGleam Highlights

A pair of interacting galaxies in Virgo about 60 million light years away

Their close encounter is driving a future merger into one giant elliptical galaxy

The visually close cores make this one of the sky’s most striking galaxy pairs

Credit Gemini North Telescope NSF NOIRLab

29/05/2026

The Sunflower Galaxy M63 in Canes Venatici

M63 the Sunflower Galaxy was discovered by Pierre Mechain in 1779 and later confirmed by Charles Messier. Located about 27 to 30 million light years from Earth in the constellation Canes Venatici near the Big Dipper, this grand spiral galaxy spans roughly 100000 light years and contains an estimated 400 billion stars, making it similar in scale to our Milky Way. This image was captured using a Celestron 8 inch HD Edge telescope paired with a ZWO 2600mc camera, built from 17 exposures of 600 seconds for a total integration time of 2 hours and 50 minutes under a first quarter Moon.

SciGleam Highlights

A massive spiral galaxy comparable in size to the Milky Way with hundreds of billions of stars

Captured under moonlit conditions demonstrating strong imaging capability and detail

Reveals the textured spiral structure that gives M63 its sunflower like appearance

Credit Original capture and processing by Bob Rossiter

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