A Night of Celestial Capture: The Constellation Vulpecula

A photographic series from the Death Valley Observatory in the dark skies of Amargosa Valley, using the Seestar S50.

It has no first-magnitude stars and no pattern that leaps out at you. It is a modest constellation, laid out between Cygnus and Sagitta, right in the heart of the summer Milky Way. And that is exactly what makes it a treasure: to see it well, you need genuinely dark skies. From Amargosa Valley, under a Bortle 1 sky, the Little Fox stops being shy.

For this series, I pointed my Seestar S50 at its named stars—those carrying a Flamsteed or variable-star designation—and let each one pose for a few minutes. The result is not a set of spectacular nebulae, but something more intimate: portraits of individual stars, each with its true color, its temperature written in light, and its own small story.

α Vulpeculae — Anser, the Fox and the Goose

Exposure: 8 minutes of integration.

Visual and artistic analysis

The image is a rich, deep star field on an ink-black background—the signature of a Bortle 1 sky. In the lower right, a warm-toned star dominates, somewhere between orange and amber, clearly larger and brighter than its neighbors thanks to the "bloating" its light produces. Beside it, a small group of stars keeps it company, and higher up shines a prominent white star. The contrast of colors—the protagonist's amber against the blue-white of the background stars—is the true spectacle of this shot.

Astronomical and scientific context

Identification. This is Anser (Alpha Vulpeculae, α Vul), whose name means "goose" in Latin. The star preserves the memory of the constellation's original name, given by Johannes Hevelius in the 17th century: Vulpecula cum Ansere, "the little fox with the goose." It is the brightest star in the constellation, at magnitude 4.44.

What it is and where it is. Anser is a red giant of spectral type M1 III, located about 291 light-years away. It has exhausted the hydrogen in its core and swelled to roughly 43 times the Sun's radius; it shines with more than 400 solar luminosities despite having a mass similar to our own. Its relatively cool surface (around 3,700 K) is what gives it that orange hue.

Scale and perspective. Anser forms an optical double with the star 8 Vulpeculae, an orange giant separated by just 7 arcminutes in the sky. It's a trick of perspective: 8 Vul lies much farther away, at about 457 light-years. They are not bound by gravity; they only line up from our vantage point.

Revealing fact. Anser probably was not born in the Milky Way. It belongs to the so-called Arcturus stream, a group of stars thought to have come from a small dwarf galaxy devoured by our galaxy billions of years ago. With nearly 11 billion years behind it, this star is a traveler from another stellar realm, now woven into our own.

4 Vulpeculae — the quiet orange giant

Exposure: 5 minutes of integration.

Visual and artistic analysis

Against a somewhat sparser field, with slight vignetting at the edges, a warm-colored star stands out at the center, golden-orange. Near the top edge, a very close pair of stars catches the eye, also in warm tones—a wink for the curious observer. The background mixes white and amber points, giving the whole an autumnal atmosphere.

Astronomical and scientific context

Identification. 4 Vulpeculae, at magnitude 5.16. It is so faint that it can only be seen with the naked eye under truly dark skies like those of Amargosa.

What it is and where it is. It is an orange giant of type K0 III, about 260 light-years away. It sits in the "red clump" phase: an evolved star that is now steadily burning helium in its core. It has grown to about 11 times the Sun's radius and has a surface temperature of around 4,760 K, hence its color.

Physical processes. At about 2.6 billion years old, 4 Vulpeculae is a star of "advanced middle age": after leaving the main sequence, it swelled and cooled. Its orange color is the portrait of a star that has already lived a good deal.

Curious fact. It has a very faint companion (magnitude 11.36) separated by about 19 arcseconds. It is a challenge even for large telescopes, and it shows how a single naked-eye star can conceal an entire system.

9 Vulpeculae — the blue spinning top

Exposure: 2 minutes of integration.

Visual and artistic analysis

This is the shortest exposure of the series, and it shows: the field is sparser, dominated by warm-toned stars on deep black. At the center shines the protagonist, clean and white, surrounded by a modest swarm of orange points. A sober, almost minimalist composition.

Astronomical and scientific context

Identification. 9 Vulpeculae, magnitude 5.01.

What it is and where it is. A blue-white giant of type B8 III, about 560 light-years away, with a surface at around 12,000 K—more than twice as hot as the Sun.

Physical processes. Its classification includes an "n" that stands for "nebulous" lines: it is a fast rotator, spinning at about 185 km/s at its equator. That dizzying rotation broadens the lines in its spectrum and slightly flattens the star, like a spinning top stretched by its own motion.

Curious fact. At only about 185 million years old, 9 Vulpeculae is a young, hot star burning its fuel in a hurry. Blue stars like this one live fast and die young compared to our Sun.

12 Vulpeculae — the star that wraps itself in a ring

Exposure: 9 minutes of integration.

Visual and artistic analysis

An elegant, not overly crowded field. At the center reigns a clearly blue-white star—cooler in tone than warm—wearing that soft halo that betrays its brightness. Up and to the left, an isolated orange star adds chromatic contrast. The whole composition breathes, with plenty of black space between the points.

Astronomical and scientific context

Identification. 12 Vulpeculae, which also carries a variable-star designation: V395 Vulpeculae. Its brightness varies slightly, between magnitude 4.78 and 4.97.

What it is and where it is. It is a Be star of type B2.5V, about 630 light-years away. At nearly 19,000 K in surface temperature and about 7 solar masses, it is one of the hottest and most massive stars in this series.

Physical processes. The "e" suffix (for emission) is the key: spinning at about 195 km/s, 12 Vulpeculae flings material off from its equator and surrounds itself with a disk of gas—a decretion disk—that emits light of its own. That disk appears and disappears over the years, and it is what makes its brightness vary.

Revealing fact. Be stars are among the most dynamic of the "normal" stars: they don't explode, but they actively shed their own matter. We are watching a star in the very act of losing weight.

13 Vulpeculae — the third brightest and its companion

Exposure: 7 minutes of integration (framed on the B component).

Visual and artistic analysis

One of the loveliest compositions in the series. Two blue-white stars stand out against the field: one in the upper half and another toward the center, both wearing the same clean, cool halo. The background, sprinkled with amber points, frames this luminous pair like two beacons in the night.

Astronomical and scientific context

Identification. 13 Vulpeculae, the third brightest star in the constellation (magnitude 4.64 for the primary component).

What it is and where it is. The primary star, 13 Vul A, is a blue-white giant of type B9.5 III, about 339 light-years away. It forms a genuine binary system with a fainter companion (13 Vul B), and both are gravitationally bound at a very similar distance from us.

Physical processes. With an almost pure white color, 13 Vul A has a surface temperature of about 10,000 K. It is a star that has already left the main sequence and swelled to about four times the size of the Sun.

Curious fact. The orbit between A and B is enormously long: estimated at more than 600 years per revolution. By the time these two stars complete a single orbit, more than twenty human generations will have passed on Earth.

15 Vulpeculae — the star with chemical spots

Exposure: 4 minutes of integration.

Visual and artistic analysis

A balanced, serene composition. At the center shines a white-blue star, and just above it a small companion of the same cool tone keeps it company, like a note and its echo. The field, of medium density, has a pleasant scattering of background stars.

Astronomical and scientific context

Identification. 15 Vulpeculae, with the variable-star designation NT Vulpeculae. It is the nearest named star in the entire constellation.

What it is and where it is. A white star of type A4 III, about 243 light-years away, with a surface at around 7,700 K and a little over twice the Sun's mass.

Physical processes. 15 Vulpeculae is a variable of the Alpha² Canum Venaticorum type: a chemically peculiar star with a strong magnetic field that concentrates certain elements into "spots" on its surface. As the star rotates, those spots move in and out of our view, and its brightness changes slightly.

Revealing fact. Stellar magnetism can paint a star's surface unevenly, like chemical continents. What we see as a steady point of light is, in reality, a surface with its own geography rotating before us.

16 Vulpeculae — the most eccentric orbit

Exposure: 12 minutes of integration (the longest in the series).

Visual and artistic analysis

With the longest exposure, this field is rich and deep. At the center shines a white star; below and to the left, a clearly blue companion; and to the right, an isolated orange star. That trio of colors—white, blue, and amber—against a dense background makes this one of the most chromatically complete shots of the set.

Astronomical and scientific context

Identification. 16 Vulpeculae, combined magnitude 5.79, right at the limit of naked-eye visibility.

What it is and where it is. It is a binary system whose primary star is of type F2 III, about 222 light-years away, with a surface at around 6,900 K, a little hotter than the Sun.

Physical processes. The extraordinary thing about 16 Vulpeculae is its orbit. The two stars take about 1,200 years to circle one another, following an ellipse of eccentricity 0.93—one of the most elongated stellar orbits known. They draw very close and then swing far apart, in an exceedingly slow, sweeping waltz.

Curious fact. An eccentricity of 0.93 means that, at the farthest point of their dance, the stars are dozens of times more distant than at the nearest. It's the difference between nearly brushing past each other and losing sight of one another entirely.

17 Vulpeculae — the blue newborn

Exposure: 6 minutes of integration.

Visual and artistic analysis

A clean, well-populated field. The protagonist, at the center, is an unmistakable blue-white, accompanied by a small blue companion just below. Around it, a uniform tapestry of background stars with scattered warm touches.

Astronomical and scientific context

Identification. 17 Vulpeculae, magnitude 5.08.

What it is and where it is. A blue-white main-sequence star, type B3 V, about 480 light-years away. Its surface burns at more than 15,600 K and its mass is around 6 times the Sun's.

Physical processes. Its intense blue color is pure heat: it emits much of its light in the ultraviolet. It shines with more than 500 solar luminosities despite its modest size, because temperature, raised to the fourth power, sends luminosity soaring.

Revealing fact. 17 Vulpeculae is astonishingly young: only about 11 million years old. When its light set out 480 years ago, the 16th century was unfolding on Earth; but the star itself, on a cosmic scale, is practically a baby fresh out of its parent cloud.

21 Vulpeculae — a star's heartbeat

Exposure: 4 minutes of integration.

Visual and artistic analysis

The framing shows marked vignetting at the edges, which frames the field like a window. At the center, a clean, well-defined white-blue star presides over a medium-density background of stars in varied tones.

Astronomical and scientific context

Identification. 21 Vulpeculae, with the variable-star designation NU Vulpeculae, magnitude 5.19.

What it is and where it is. A white star of type A7, about 313 light-years away, with a surface at around 7,700 K. It is a very fast rotator, spinning at more than 220 km/s.

Physical processes. 21 Vulpeculae is a variable of the Delta Scuti type: it physically pulsates, expanding and contracting in cycles of a few hours, which makes its brightness fluctuate slightly. It is, quite literally, a star that beats.

Curious fact. The pulsations of Delta Scuti stars allow astronomers to "listen" to their interiors through asteroseismology, in much the same way a seismologist studies the interior of the Earth from its tremors.

22 Vulpeculae — the eclipse of a yellow giant

Exposure: 5 minutes of integration.

Visual and artistic analysis

In this rich, deep field, the protagonist, toward the center-left, shows a warm tone—between yellow and golden white—that sets it apart from most of its neighbors. Up and to the right, a prominent white star provides a counterpoint. The contrast between the protagonist's gold and its neighbor's white is subtle and elegant.

Astronomical and scientific context

Identification. 22 Vulpeculae, also known as QS Vulpeculae, magnitude around 5.2.

What it is and where it is. It is an eclipsing binary system located about 1,490 light-years away—among the most distant in the series. It is made up of a yellow bright giant (type G9, about 96 times the Sun's radius) and a hot blue companion star of type B8.

Physical processes. It is a system of the Zeta Aurigae / Algol type: from our perspective, the two stars eclipse one another each time one passes in front of the other, with an orbital period of about 249 days. When the yellow giant covers the small blue star, the total brightness of the system drops.

Revealing fact. During these eclipses, the light of the blue star passes through the outer layers of the yellow giant just before it is hidden. By analyzing that filtered light, astronomers can "sample" the giant's atmosphere, layer by layer, as if taking an X-ray of it.

QR Vulpeculae — the X-ray star

Exposure: 5 minutes of integration.

Visual and artistic analysis

A dense, heavily populated field, typical of the heart of the summer Milky Way. In the lower center shines the protagonist, blue-white, over a carpet of countless background stars in tones ranging from white to amber. It is one of the shots that best conveys the sensation of gazing into the interior of our galaxy.

Astronomical and scientific context

Identification. QR Vulpeculae (also cataloged as HD 192685 and HR 7739). Its brightness varies between magnitude 4.60 and 4.80. It was recognized as a variable in 1982 and received its QR Vul designation in 1985.

What it is and where it is. It is a Be star of type B3, with a companion of type A7, located about 1,000 light-years away. Its surface burns at around 18,700 K and, like a good Be star, it spins fast (about 160 km/s) and surrounds itself with a disk of gas.

Physical processes. QR Vulpeculae is a variable of the Gamma Cassiopeiae type: a select group of Be stars that, unusually for stars of this kind, emit intense and erratic X-rays. The exact origin of that emission remains a matter of scientific debate—one of those questions astronomy has not yet fully closed.

Curious fact. That such an apparently quiet naked-eye star should in fact be a variable X-ray source reminds us that the sky hides extreme physics behind every point of light. The Little Fox keeps, among its modest stars, genuine open riddles.

Coda: the sky's thermometer

Lined up together, these eleven stars tell a story no nebula could tell better: that of color as temperature. From the cool amber of Anser and 4 Vulpeculae, through the intermediate white of the type-A stars, to the burning blue of 12 and 17 Vulpeculae, each portrait is a direct reading of the heat of a surface tens or hundreds of light-years away.

And there is more: giants swelling at the end of their lives, newborns only millions of years old, stars that pulse, that spin until they shed their own matter, that eclipse one another, or that emit X-rays for reasons we don't fully understand. All of that lives in a constellation most people have never looked at, in a corner that reveals itself only under truly dark skies.

That, perhaps, is the best lesson of the Little Fox: the modest is not the insignificant. It's enough to look patiently—and with a sky black enough—to discover that even the humblest constellation is full of wonders.

All images were captured with a Seestar S50 from Amargosa Valley, Nevada, under Bortle 1 skies.

AUGUST 2026: DARK PILLARS & THE PERSEID METEOR SHOWERS!

August is here, and it’s bringing one of the most anticipated skywatching events of the entire year! As your Solar System Ambassador, I am thrilled to introduce the August 2026 Astrophotography Challenge. This month, we have a brilliant open cluster, a famous dark pillar of dust, and the king of annual meteor showers!

🎯 August Targets: Open Cluster M29: A bright, compact star cluster nestled deep in Cygnus the Swan, shining through the rich star fields of the Milky Way.

Elephant's Trunk Nebula (IC 1396A): A striking dark pillar of dense gas and dust embedded within the larger emission nebula IC 1396. A true masterpiece for deep-sky imagers!

🌟 BONUS TARGET - METEOR SHOWER: Perseid Meteor Shower! Reaching its peak on the night of August 12–13, this is the best meteor shower of the year, boasting up to 100 meteors per hour under ideal conditions!

🗓️ Timing & Conditions: Prime Imaging Window: August 8 – 16.

Moon Watch: Perfect timing! We have optimal ~20% Moon Illumination, giving us dark skies ideal for tracking fainter meteors and deep-sky details!

💡 Ambassador Tips for August: M29 Location: Look right in the heart of the Cygnus Milky Way to frame this neat star cluster.

Elephant's Trunk Filters: IC 1396A shows its finest structural detail when using narrowband H-alpha filters.

Perseids Setup: Use a wide-angle lens on a sturdy tripod, set long exposures (15–30 seconds), and point towards the northeast after midnight for your best chance at catching fireballs!

Clear skies and happy imaging! 🔭🌵

JULY 2026: THE COSMIC CONTINENT & A CELESTIAL TRIO!

We are moving right into the heart of summer and peak Milky Way season! As your Solar System Ambassador and EOP, I am thrilled to introduce the July 2026 Astrophotography Challenge. This month, we have an amazing contrast between deep dark dust lanes, a massive emission nebula, and a beautiful planetary conjunction!

🎯 July Targets:

• Pipe Nebula (Barnard 59, 65-67, 78): A massive dark nebula complex in Ophiuchus. It forms a perfect silhouette against the bright backdrop of the Milky Way core.

• North America Nebula (NGC 7000): The "Cosmic Continent." This iconic emission nebula in Cygnus is a summer classic, glowing with rich crimson light.

• 🌟 BONUS TARGET - CELESTIAL TRIO: Moon, Mars & Pleiades Conjunction! Early in the month on July 11, keep an eye out for a beautiful close alignment. It is perfectly visible to the naked eye and offers an amazing nightscape photo opportunity!

🗓️ Timing & Conditions:

• Prime Imaging Window: July 10 – 17.

• Moon Watch: We have optimal dark skies with ~20% illumination, giving you the perfect canvas to pull out the faint details of the Milky Way core.

💡 Ambassador Tips for July:

• Framing the Pipe: The Pipe Nebula needs a wide-field setup to fully capture its shape silhouetted against the dense stellar background of the Milky Way.

• NGC 7000 Structure: The North America Nebula shows its finest details and contrast when paired with an H-alpha filter.

• Dark Nebula Secret: Unlike bright targets, dark nebulae often show up best with shorter, carefully stacked exposures to avoid bloating the surrounding stars.

• Summer Comfort: Take advantage of these warm summer nights—they are absolutely perfect for spending hours out under the stars imaging!

How to Enter: Post your best July images to our Facebook group! Include your gear setup and make sure to tag your posts with our official hashtags. Let's see some summer magic!

Clear skies and happy imaging! 🔭🌵

IN CASE YOU MISSED IT: NASA’s June Moon Base Update is wild!

If you haven’t been tracking the latest updates, the blueprint for a permanent human presence on the Moon is officially moving into overdrive. NASA just dropped the June wrap-up, and the strategy is clear: more missions, more partners, and a relentless drive toward the lunar South Pole.

Here is the quick breakdown of what’s happening right now:

🚀 The Big Moves

NASA just awarded 4 new landing missions to 3 major commercial partners (a massive ~$560M combined investment):

• Astrobotic: 2 missions (Peregrine variant)

• Firefly Aerospace: 1 mission (Blue Ghost lander)

• Intuitive Machines: 1 mission (Nova-C lander)

🌙 The 3-Phase Strategy

• Phase 1 (Through 2029): Getting to the Moon reliably. Over 20+ robotic missions are planned to scout the South Pole and test key tech. First robotic landing target? 2026!

• Phase 2 (2029–2032): Setting up the grid. Think permanent power, navigation, and communications.

• Phase 3 (2032+): Full-on habitats, advanced logistics, and cargo return to Earth.

🔑 Game-Changing Tech: Meet "Promise"

Imagine a nuclear-powered (RTG) cousin of the Mars Curiosity/Perseverance rovers, but built for the Moon. Named "Promise", this rover will be capable of exploring permanently shadowed regions where solar power can't reach.

💡 The Philosophy: "Many Shots on Goal"

Space is hard. NASA is embracing a "learn from every mission" mindset—embracing both successes and setbacks to buy down risk, just like the Mercury → Gemini → Apollo days. (This includes working closely with Blue Origin as they refine their New Glenn/Endurance lander plans for 2027).

Bottom line: We aren't just visiting the Moon this time. We are building a permanent home base. 🧑‍🚀🌕

🔗 Read the full breakdown: nasa.gov/moonbase 📅 Stay tuned for Moon Base Update #3 next month!

#NASAMoonBase #Artemis #LunarExploration #SpaceNews #MoonBase #NASA #ReturnToTheMoon #SpaceExploration

A Night of Celestial Capture: M8 — The Lagoon Nebula

Deep within the shadows of Sagittarius, where the Milky Way thickens into a river of starlight, lies a region that seems to breathe with its own pulse. The Lagoon Nebula, M8, is not just a glowing cloud of gas; it is a living stage, a cosmic workshop where matter reshapes itself and light carves pathways through primordial dust.

Every time you point a telescope toward this region, something shifts. It’s not only the image that appears on the screen or in the eyepiece; it’s the feeling of witnessing a process that began thousands of years before the word “astronomy” even existed. The light we capture today began its journey when ancient civilizations were raising monuments to the sky, unaware that millennia later we would still be searching for meaning in the same stars.

M8 is a nebula that invites contemplation. Its reddish glow, dark filaments, and luminous cavities seem to tell a layered story: the story of stars being born, of stellar winds sculpting the gas, of past explosions leaving visible scars in its structure. It reminds us that the universe is not static; it is dynamic, turbulent, creative.

Capturing it in an image is an attempt to freeze a single moment within an eternal process. It is holding still one heartbeat of a stellar nursery that never stops moving. And yet, every photograph reveals something new—a detail previously overlooked, an unexpected contrast, a texture that feels almost organic.

Below is the detailed description of this capture of M8, a window into one of the most fascinating natural laboratories in our galaxy.

General Description: The image presents a bright and extensive nebula, with a diffuse and filamentous appearance. The composition is rich in detail and shows an irregular distribution of cosmic gas and dust, creating a stunning visual landscape. A remarkable depth is seen, with denser regions that seem to stand out and others that fade into the darkness of space. Structure and Shapes: The main structure of the nebula is complex, with dark filaments that intertwine with brighter, more colorful regions. Arcs and veins of gas are observed that appear to undulate, suggesting turbulent movements. The general shape is irregular and amorphous, without obvious symmetry, giving it a natural and organic appearance. There are subtle spiral structures, but they are not as defined as in a spiral galaxy. Color Palette:

• Red: The red color dominates in many areas of the nebula, indicating the presence of ionized hydrogen (Hα). This color is characteristic of regions where gas is being excited by radiation from young stars.

• Blue/Cyan: Blue or cyan regions suggest the presence of ionized oxygen ([O III]), another common element in emission nebulae.

• Green/Yellow: A mixture of red and blue can create green or yellow hues, which usually indicate a combination of ionized hydrogen and oxygen.

Darkness: Dark areas, where gas and dust are denser, absorb light and create striking contrasts. Notable Elements:

• Bright Core: There is a very bright central core that appears to be the source of the light emission. It could correspond to a group of hot and massive stars. Dark Filaments: Dark filaments are particularly notable, as they create a sense of depth and complexity. Regions of Intense Brightness: Regions of intense brightness can be identified that suggest areas of active star formation.

Dark Filaments: Dark filaments are particularly notable, as they create a sense of depth and complexity. Regions of Intense Brightness: Regions of intense brightness can be identified that suggest areas of active star formation.

• Artifacts: I have not been able to identify artifacts in the image.

Notable Elements: Bright Core: There is a very bright central core that appears to be the source of the light emission. It could correspond to a group of hot and massive stars. Dark Filaments: Dark filaments are particularly notable, as they create a sense of depth and complexity. Regions of Intense Brightness: Regions of intense brightness can be identified that suggest areas of active star formation. Artifacts: I have not been able to identify artifacts in the image.

ASTRONOMIC AND SCIENTIFIC CONTEXT Object Identification: The object you have captured is the Lunar Nebula, also known as the Lagoon Nebula. Its technical designation is M8 (in the Messier catalogue) and its catalog name NGC 864. What is it and where is it?: M8 is an emission nebula located in the constellation Sagittarius. It is located about 5,200 light years from Earth. It is a star-forming region, meaning it is a place where new stars are born. Cosmic gas and dust collapse under the influence of gravity, forming accretion disks around young stars. Physical Processes: The nebula is being ionized and illuminated by a group of young, massive stars, known as the star cluster NGC 864. These stars emit ultraviolet radiation that excites the hydrogen and oxygen atoms present in the gas, causing them to emit visible light. Stellar winds and radiation from these stars are also sculpting the nebula, creating its complex structures. Scale and Perspective: The Lunar Nebula is relatively large, with a diameter of approximately 120 light years. This makes it slightly larger than the full Moon in the sky. Despite its size, it is very far from us, which is why it appears small in the night sky. The bright stars seen near the nebula are stars that belong to our own galaxy, the Milky Way, and are located between us and the nebula. Curious or Revealing Fact: The Lunar Nebula is one of the brightest and easiest to observe emission nebulae in the night sky. The light we see from M8 came from there more than 5,200 years ago, which means we were seeing it as it was seen during the construction of the Giza pyramids in Egypt.

A New Era of Lunar Exploration: An Inspiring Story

In these times of unprecedented advances in technology and science, space remains one of the greatest frontiers of exploration, one that has captured the minds of generations. With each new dawn, we find ourselves standing at the threshold of a new golden age of space exploration. Just as the Apollo astronauts inspired millions with their footprints on the Moon, today we continue to dream big and look toward the future.

And this Tuesday, June 9, that future gained names and faces: NASA officially announced the crew of Artemis III, the mission that in 2027 will rehearse in Earth orbit some of the most complex operations ever attempted in recent human spaceflight, paving the way for Artemis IV to carry us, in 2028, to the lunar South Pole.

The Four Chosen (and a Fifth Guardian)

The Artemis III crew reflects the very best humanity can offer when it brings together talent, discipline, and vocation:

Randy Bresnik (NASA), commander. A veteran of three spaceflights, a retired U.S. Marine Corps colonel, and a test pilot with more than 7,000 hours in 95 types of aircraft. Since 2018, he has overseen the development and testing of the systems that will fly on Artemis missions. Few people on the planet know the spacecraft he will now command better than he does.

Luca Parmitano (ESA), pilot. And here is the news that makes history: for the first time, a European Space Agency astronaut has been assigned to an Artemis mission. Parmitano, a colonel in the Italian Air Force and a test pilot, was the first Italian — and only the third European — to command the International Space Station. His assignment as pilot reflects the depth of European expertise in human spaceflight and his extensive operational experience in high-pressure situations.

Frank Rubio (NASA), mission specialist. A physician, a U.S. Army aviator, and the holder of the American record for the longest single-duration spaceflight: 371 days in orbit. If anyone understands what human endurance in space truly means, it's him.

Andre Douglas (NASA), mission specialist. For Douglas — an engineer with a doctorate in systems engineering and a former Coast Guardsman with experience in search and rescue operations — this will be his first spaceflight. He already served on the backup crew for Artemis II, and now it's his turn to walk through the door himself.

Named as backup crew member was Bob Hines, pilot of the Crew-4 mission to the International Space Station, who will train alongside the four prime crew members, ready to fill any seat should the need arise.

An Orbital Choreography Without Precedent

So what exactly will Artemis III do? Although the mission will not land on the Moon, it will likely be the most ambitious dress rehearsal in the history of space exploration.

The SLS (Space Launch System) rocket will launch the Orion spacecraft and its four crew members from NASA's Kennedy Space Center in Florida into low Earth orbit. Once there, Orion will demonstrate for the first time its rendezvous and docking capabilities with test versions of the two commercial lunar landers currently in development: Blue Origin's Blue Moon and SpaceX's Starship.

The plan is a true odyssey of precision. First, Blue Origin's test lander — capable of remaining in orbit for several weeks — will launch and await the crew. Then, SLS will send the astronauts aboard Orion, which will rendezvous in space with the Blue Origin lander and spend about two days docked to it, conducting tests and technology demonstrations that will include the crew entering the lander itself. With that phase complete, Orion will undock and await SpaceX's Starship, spending roughly a day connected to it for additional checkouts and testing.

Finally, Orion and its crew will return home, splashing down in the Pacific Ocean, where a team from the U.S. Navy and NASA will recover the astronauts. In total, the crew is expected to remain in space for about two weeks, with the exact mission length determined in real time based on launches, rendezvous, and docked operations.

Every system interface, every line of software, every propulsion and communications system between Orion and the landers will be put to the test. It's the difference between dreaming of returning to the Moon and knowing, with engineering certainty, that we can do it.

Europe at the Heart of Artemis

The Artemis program is a testament to the shared commitment of international agencies like ESA and NASA to push our frontiers beyond the known. For the first time, a European astronaut has been assigned to one of these missions, marking an era in which Europe doesn't merely participate — it plays a crucial role in humanity's return to our natural satellite.

And the European contribution goes far beyond a seat on the spacecraft. ESA's European Service Module is, quite literally, what gives Orion life: it provides propulsion, power, water, and air for the crew. As a European, born in Madrid, I confess this news strikes a special chord in me. Seeing Europe take its place at the very heart of the Artemis program is a reminder that space exploration, at its best, knows no exclusive flags: it is a project of all humanity.

The Road to 2027 Is Already Underway

As I write these lines, the work is moving forward at a steady pace. This summer, engineers will connect Orion's crew module to its service module and integrate the spacecraft's docking system, which will fly for the first time. Heat shield testing continues, with individual blocks undergoing ultrasonic inspections. SLS technicians are integrating the engine section with the rest of the core stage ahead of installing the four RS-25 engines, and with all the solid rocket booster segments now at Kennedy Space Center, rocket stacking is also set to begin this summer.

Meanwhile, Blue Origin and SpaceX are building the test articles for their respective lunar landers, with NASA working hands-on alongside both companies through every phase of design, development, and evaluation. The crew, for their part, begin training immediately — both on Orion's systems and by assisting in the development of the landers that will one day carry human beings back to the lunar surface.

All of this builds on the extraordinary foundation of Artemis II, the mission that in April carried four astronauts around the Moon and reignited global excitement for exploration. Those astronauts lit the torch; now they pass it to Randy, Luca, Frank, and Andre.

More Than Technology: The Human Spirit

The success of Artemis III will symbolize not only a technological achievement, but the human spirit itself: international collaboration, the passion to discover the unknown, and the shared vision that drives us forward. Because the final destination of this journey is not just the Moon. Every test, every docking, every lesson learned on these missions is a stepping stone toward the goal that defines this new golden age: sending the first human beings to Mars.

NASA Administrator Jared Isaacman summed it up with an image that perfectly captures the moment we are living through:

"Think about how many spacecraft, all of which will eventually carry human beings, will be in orbit at the same time — from Dragon, Shenzhou, Soyuz, possibly Starliner, Starship, and Blue Origin landers. This seems like the beginning of the future that we imagined as children."

And he's right. For the first time in history, the sky above our heads is beginning to resemble the one we used to draw in our school notebooks: a sky filled with spacecraft, with many flags, with human beings living and working beyond the Earth.

In moments like these, it's easy to feel inspired and full of hope. As our space leaders remind us, exploration is not just about achieving technical milestones; it's also about carrying the aspirations of an entire generation and building a legacy for those who come after us — just as the Apollo astronauts did for so many of us.

So, as the sun sets over our planet Earth and we contemplate the vastness of the universe — as I will tonight, like so many other nights, under the dark skies of the Nevada desert — let us remember that each one of us is part of this thrilling journey to the stars.

It is a never-ending story in which we are all protagonists.

JUNE 2026: SUMMER SHOWPIECES & SOLAR MAXIMUM PEAK!

Summer has officially arrived, and the skies are heating up! As your Solar System Ambassador and EOP, I am thrilled to introduce the June 2026 Astrophotography Challenge. This month, we balance a classic galactic showpiece and an ancient star cluster with a spectacular, high-energy daytime target!

🎯 June Targets:

• Lagoon Nebula (M8): The ultimate "Summer Showpiece." This giant emission nebula is incredibly bright, vibrant, and a joy to image as it rises out of the southern horizon.

• Globular Cluster (M92): Often overshadowed by its neighbor M13, this "Compact Beauty" is one of the oldest ancient star clusters in the northern sky and a fantastic technical target.

• 🌟 BONUS TARGET - SOLAR MAXIMUM: Solar Maximum Peak Activity! From June 20–30, we are entering an expected peak of Solar Cycle 25! It is the perfect time to turn your safe solar scopes toward our star. ⚠️ SAFETY FIRST: NEVER look directly at the Sun! Use proper, certified solar filters only!

🗓️ Timing & Conditions:

• Prime Imaging Window: June 11 – 18.

• Moon Watch: Dark Skies are back with ~20% illumination, providing prime dark windows as the stunning Summer Milky Way continues to rise.

💡 Ambassador Tips for June:

• Lagoon Framing: M8 looks spectacular in wide-field setups—try framing it with the nearby M20 (Trifid) for an epic summer mosaic!

• M92 Magnification: To really resolve the dense, bright core of this ancient cluster, swap in a focal extender or use higher magnification.

• Solar Dynamics: For solar imaging, H-alpha filters will beautifully reveal massive surface prominences and flares. Keep your cameras ready at night too, and watch for potential auroras triggered by this peak solar activity!

• Shorter Nights: Remember, the summer solstice means shorter nights, so plan your deep-sky imaging tracks carefully to maximize your integration time!

How to Enter: Share your best June captures in our Facebook group! Whether you are tracking sunspots by day or capturing deep-sky hydrogen clouds by night, we want to see your work. Include your equipment specs and tag your posts with our official hashtags!

Clear skies and happy imaging! 🔭🌵

An Honor and a Privilege: Closing My Chapter as Vice President of the LVAS Education Outreach Program

This is, quite possibly, the hardest post I have ever written on this blog.

This month I submitted my resignation as Vice President of the Education Outreach Program of the Las Vegas Astronomical Society, a position I have had the honor of holding since 2018.

Thank You for the Trust

I want to start with what matters most: gratitude. This position is not inherited or handed out; it is decided by election every two years. Receiving the vote of confidence of the association's members, election after election, throughout all these years, has been one of the greatest honors of my life. Every vote was a reminder of the responsibility I carried — and of the affection of this community.

Thank You to the Volunteers

To every volunteer who has been part of this program: thank you from the bottom of my heart. Nothing we accomplished would have been possible without you. Every star party, every event at libraries, parks, and schools, every telescope set up under the desert sky carries your fingerprints. You are, and always will be, the soul of this program.

Thank You, Stephen

I want to give a very special mention to Stephen Alan Bock, the Vice President who came before me. In 2018, Stephen gave me something money can't buy: the confidence in myself to begin this adventure. Without that push, none of this would have happened. Thank you, my friend.

A Road I Never Imagined

When I became a member of this association back in 2012, I never thought or imagined that I would have the opportunity to serve the Southern Nevada community in this way. From 2018 until today it has been many years, many nights, many faces lit up while looking through a telescope for the first time. It has been an honor and a privilege, followed by an extraordinary experience I will carry with me always.

The Why

Since this blog is my most personal space, I want to share the why in more detail.

A series of radical changes in my life, both professional and personal, have brought me to this crossroads. The biggest of them: I am part of the group building Nevada's first telescope farm, Death Valley Observatories, in Amargosa Valley. A project of this magnitude demands constant effort and a daily presence — not to mention the distance from Las Vegas. Between the farm and the city lie desert, miles, and hours that no longer allow me to support the program properly and with the dedication it deserves. And this program, and this community, deserve nothing less than full dedication. Out of respect for both, I am taking this step.

And why there, in the middle of the desert? Because in Death Valley, the night sky offers infinitely more than just darkness — it offers clarity, depth, and time.

• New Moon? Chances are high for clear skies: this region has among the lowest cloud cover in the United States.
• Photographing galaxies? Average atmospheric seeing here ranks among the finest nationwide, giving sharper, steadier views.
• Hunting faint molecular clouds? Sky darkness reaches 21.97 mag/arcsec² — close to the natural limit of Earth's night sky.
• Worried about optics fogging? Don't be: with some of the lowest humidity levels on the planet, your equipment stays clear all night.
• And surrounded by unobstructed horizons, every night offers more usable hours to explore the cosmos.

In the end, I am not stepping away from the mission — I am stepping closer to the sky. Everything I learned and lived at the LVAS comes with me into this new chapter.

This Is Not Goodbye

I will remain connected to the association as a member. I will remain under the same sky, looking up, sharing the same sense of wonder that has been with me since I was a child.

And speaking of that wonder: I want to thank my mother, who at age six sparked in me a love for the universe, and my sisters, patient and enthusiastic companions through so many nights under the stars. Everything I have done in these years was born from that support and that love.

Thank you for everything, Las Vegas Astronomical Society.

It has been an honor and a privilege.

Clear skies,

The Moon is back in play! And this time… we’re going there to stay.

Something happened to me today that I haven't felt in years: my lunar excitement returned.

And yes, I know that sounds like a cliché. But anyone who has followed space exploration over the last few years knows exactly what I’m talking about: promises, renders, slipping deadlines… Until today, when everything changed.

That spark I had as a child—when I used to imagine bases on other worlds—suddenly reignited. And it’s all thanks to NASA’s conference regarding the Moon Base program.

Because this time, they didn't talk about vague intentions.

They didn't talk about "someday."

They didn't show pretty renders with no attached dates.

No.

Today, they presented a real plan—complete with clear phases, contracted vehicles, scheduled missions, and a direct objective:

to establish a permanent human presence on the Moon.

And honestly… I was starting to lose faith.

But this restored my pride, my happiness, and the sense that we are entering a new era.

A program that finally has momentum and direction.

Moon Base is divided into three phases, and the first one is already underway:

• 25 launches
• 21 landings
• 4 tons of cargo delivered to the lunar South Pole

All of this between now and 2029. It’s a pace we haven't seen since the 1960s.

And the best part? Every mission contributes something; every vehicle tests a new capability; every landing paves the way for the next.

For the first time in decades, we aren't just improvising. We are building.

Vehicles already on the way (and that have me completely fascinated)

The conference was a flurry of announcements, but these are my favorites:

Blue Origin Mark 1 Endurance

The lander that will inaugurate Moon Base One.

Privately developed, robust, and designed to deliver cargo to the Shackleton Connecting Ridge in 2026.

Astrobotic Griffin

A cargo-hauling behemoth capable of carrying over 500 kg—including the FLEX rover.  The New LTV Rovers

This is where I got truly excited:

Astrolab CLV‑1 → Compact, autonomous, teleoperated, or crewed. 200 km range. 200 km! That is four times the range of any previous lunar or Martian rover.

Lunar Outpost Pegasus → Lightweight, rugged, ready for early missions. Designed to explore, map, and prepare the terrain for the base.

These vehicles aren't just conceptual prototypes. NASA has already signed the contracts. They are already under construction.

Lunar Drones: The Part That Feels Like Science Fiction

The announcement of the Moonfall system absolutely blew my mind. Hopping drones capable of:

• Exploring dark craters
• Mapping with centimeter-level resolution
• Searching for subsurface ice
• Surviving the lunar night
• Serving as communication relays
• And Firefly’s carrier spacecraft will deploy several at once, covering vast areas of the South Pole.

This means we will have constant communication—something we have never had on the Moon before. And that changes everything.

The Lunar South Pole: The New Continent to Discover

What excites me most is *what* we are going to explore. The South Pole is an extreme and mysterious place:

• Craters reaching –400°C
• Mountains illuminated almost year-round
• Ice deposits that could sustain human life
• Terrain that is virtually unknown

(Side note: in the entire history of humanity, we have accumulated only 80 hours of lunar spacewalks. Eighty. Over six decades.)

In the coming years, we could multiply that figure several times over. We are going to see:

• Spacewalks in regions never before trodden
• Rover traverses spanning hundreds of kilometers
• Deep exploration of eternally dark craters
• Installation of the first power and communication systems

And they haven't forgotten the most important thing: astronaut health. Pressure, radiation, decompression... they are investigating every detail to ensure this isn't a reckless adventure, but a safe exploration.

It’s hard not to get excited.

International Cooperation… and a Silent Race

Moon Base is not an isolated project. NASA has made it clear that it will be an international effort:

• Europe
• Korea
• Japan
• Commercial partners
• Universities
• New nations yet to join

But it is also true that China is advancing rapidly with its plans for a lunar base in the 2030s. It is not a hostile race, but it is, indeed, a competition of visions. And that—far from concerning me—I find fascinating. Humanity advances furthest when there is more than one player pushing forward.

An Extraordinary Time to Be Alive

Today, I regained something I thought I had lost: the faith that we would see a lunar base within our lifetime.

• And not just a base. A complete ecosystem:
• Landers
• Rovers
• Drones
• Constant communication
• International cooperation
• In-depth exploration of the South Pole
• And, above all, human footsteps that will mark a new era

The Moon is back in play. And this time, we aren't going just to visit. We are going to stay.

Thought of the Day: The Files Are Out. Now What?

On May 8, 2026, the U.S. government released decades of classified UAP files to the public. For many, this was a bombshell. For me, it felt like the first drop of a very long rain—a rain we’ve been promised, denied, and ridiculed about for more than eighty years. After decades of “nothing to see here,” suddenly there is something to see, and we’re being told it’s real. But only a drop at a time.

I’ve been fascinated by this topic for years—not because I believe in little green men, but because the questions it raises are some of the deepest a human being can ask. Who are we? Are we alone? And if we are not alone, what does that actually mean for how we live?

After sitting with these files, the whistleblower testimonies, the old myths, and the new theories, I find myself not with answers, but with better questions. And I think that’s exactly where we should be right now. The discomfort of not knowing is, in a strange way, the most honest place to stand.

Looking at the possibilities emerging from all of this, I can see at least four broad scenarios—and none of them are comfortable.

First, beings that mean us harm. Whether we call it slavery, resource extraction, or something darker dressed in the language of ancient demons, the result is the same: an encounter that leaves us diminished, injured, or afraid. What makes this narrative dangerous is how easily it can be weaponized. When a public figure calls these phenomena “demons from hell,” I don’t just hear a warning—I hear the opening notes of a crusade. And a crusade does not negotiate, does not distinguish between varieties of intelligence, and rarely ends with the best of us in charge.

Second, beings that offer help with hidden conditions. They arrive with gifts—technology, healing, protection from the other group—but the gifts come with a leash. Sign here, trust us, accept our framework, and we will save you. The chain might not be made of iron. It might be made of silk, woven from every solution we are desperate for. The danger isn’t invasion; it’s dependency. It’s waking up generations later to find we have forgotten how to solve our own problems, how to be our own civilization.

Third, beings that are simply passing through, indifferent to our existence entirely. They are here for a reason that has nothing to do with us. They are not hostile; they are not saviors. They are travelers on a highway, and we are a stone by the roadside they have never thought to notice. This might be the quietest wound of all. Not that we are threatened, not that we are enslaved, but that something ancient and wise is right next to us—and we will never know what being alive meant to them. A locked library floating through our skies, forever silent.

Fourth, something from beyond our dimension of reality, leaking into ours in ways we are only beginning to perceive. Perhaps they are observing an experiment. Perhaps our universe is a kind of simulation, and they are the programmers checking in on the runtime. Perhaps their “leak” is not even intentional—just a natural law we don’t yet understand. This possibility reminds us how young our science still is, and how much of what we call impossible is simply not yet measured.

What strikes me most, looking at these four possibilities, is what is missing from our public conversation. I hear no powerful voice saying, “They are here to say hello.” I hear no serious official exploring the possibility that some of these intelligences might be curious observers, not demons or manipulators. The loudest narratives are the ones that push us toward fear, dependency, or crusade—and that should make us deeply suspicious. Who benefits when we are herded into only threat-based interpretations?

But here is what I keep coming back to, and what I want to offer you as a place to stand: regardless of which scenario turns out to be true, or which mix of them, or something we haven’t yet imagined—we are still human. The best and worst of us is still ours. We are still the ones who choose, every day, whether to be cruel or kind, curious or closed, generous or grasping. No outside force, however ancient or advanced, changes that responsibility. That’s not naivety. It’s a refusal to let our moral center be held hostage by a revelation we did not ask for.

I don’t know if God made us, or if we are a beautiful accident of evolution, or if we are part of a design so vast we cannot see its edges. And I don’t need to know that to know that we are capable of looking for the best in ourselves. Not a perfect version, not a hall-of-fame version—just the version that faces uncertainty without immediately reaching for a sword or signing away its soul.

I invite you to explore these ideas with me. Not to arrive at certainty, but to sit with the uncertainty together. To ask better questions. To notice which narratives make us afraid and which ones make us curious. And to figure out—while we wait for the universe to reveal itself, drop by drop—what kind of humans we want to be.

MAY 2026: SUMMER NEBULAE & THE BLUE MICROMOON!

The nights are getting warmer, and the galactic core is climbing higher! As your Solar System Ambassador and EOP, I am thrilled to introduce the May 2026 Astrophotography Challenge. This month, we are diving into deep-sky remnants and a very rare lunar event!

🎯 May Targets:

• Trifid Nebula (M20): Known as the "Three-Lobed Beauty," this stunning object is a rare combination of an emission, reflection, and dark nebula all in one.

• Crab Nebula (M1): The famous remnant of a supernova observed nearly a thousand years ago. It’s a complex pulsar wind nebula that serves as a fantastic technical challenge.

• 🌟 BONUS CELESTIAL EVENT: The Blue Micromoon! On May 31, we will witness the smallest full moon of 2026 as it reaches apogee. Because it is the second full moon in a single month, it earns the "Blue Moon" title!

🗓️ Timing & Conditions:

• Prime Imaging Window: May 12 – 19.

• Moon Watch: We have an excellent ~20% illumination window mid-month, providing the dark skies needed for prime nebula photography.

💡 Ambassador Tips for May:

• Trifid Color: Use an H-alpha filter to really bring out the deep reds and vibrant colors of M20.

• Crab Detail: M1 shows its best structure when using an OIII filter.

• Micromoon Challenge: Take a photo on May 31 and compare its size to your previous moon shots—you’ll really see the 14% difference!

• Look South: The Milky Way is rising, so keep an eye on the southern horizon for these summer targets.

How to Enter: Share your captures in our Facebook group! Whether you're chasing the pulsar in the Crab or measuring the Micromoon, we want to see your results. Include your gear details and use our hashtags!

Clear skies and happy imaging! 🔭🌵