Pro camera techniques for bagging your best-ever astro photos

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Astrophotographer, film-maker and night-sky conservationist Josh Dury uses photography and film-making as a way to promote conservation and highlight the effects of light pollution.

Based in south-west England, Dury has traveled across the world taking photos of dark skies, with favorite subjects including the Milky Way, the Northern Lights, meteor showers and the Winter Circle – Orion, Taurus and Gemini.

Pro techniques for super astro shots

Josh reveals his go-to setup for astrophotography: a Sony A7S II, a Sigma 14mm F1.8 Art lens, a sturdy aluminum tripod and head by Slik, and an RGBS LCD Shutter Release.

Josh reveals his go-to setup for astrophotography: a Sony A7S II, a Sigma 14mm F1.8 Art lens, a sturdy aluminum tripod and head by Slik, and an RGBS LCD Shutter Release.

“Firstly,” says Dury, “set up your camera on a tripod with a geared head, so you can easily adjust for right ascension [which corresponds to longitude] or declination [latitude] – with astrophotography, you don’t want to consider a particular angle only to find that your equipment limits you.

“Next, look at the camera’s rear screen and check that it reflects the image you have projected in your mind.

“Now, using an intervalometer, take an interval image every three or four seconds – the amount of images required depends on the nature of the shot: for a Milky Way, you will need at least 20-30 frames to stack during editing.

“One of the most vital things to do is to balance out the signal-to-noise ratio; that’s why a camera that works well at higher ISO values, coupled with a wide-angle lens with a large aperture to let lots of light in, is essential.

“Depending on the nature of the shot, an acceptable ISO range is 800-21,000.”

You won’t go wrong if you…

Astrophotographer Josh Dury on location with is camera kit

Astrophotographer Josh Dury on location with is camera kit

“Plan ahead and know what your subject is going to be. If you want to take lots of different shots on the night – of the Milky Way, star trails and the moon – then you need to plan carefully for every scenario.”

“The most important aspect of landscape astrophotography is the weather. You need a clear sky, otherwise you won’t get the detailed shots you need. There must be no cloud interference whatsoever.”

“Allow for an appropriate amount of time to capture what you need. At least a couple of hours will be fine for the Milky Way but for star trails with definition, you’re looking at up to three hours or longer.”

josh dury astro tips image 2

josh dury astro tips image 2

josh dury astro tips image 3

josh dury astro tips image 3

“Be aware of light pollution. Shooting anywhere near towns or cities is a no-go because of all the light shining up. Check light pollution maps – you need to be anywhere between five and 10 miles away.”

“Take plenty of layers of clothing. You want astrophotography to be fun, and not have to struggle when the temperatures drop at night. Pack coats, hats and plenty of pairs of socks, because your feet will feel it first.”

“Recce the routes to your location so you can plan them beforehand and know what you’ll need to put up with along the way. Be conscious of health and safety and let someone know where you’re going and when – just in case.”

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James Webb’s John Hancock | WJCT News

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Get ready for incredible astrophotography from the James Webb Space Telescope! Look for its unique signature – diffraction spikes in the shape of James Webb’s John Hancock. With six strong spikes and two horizontal ones, you’ll recognize Webb’s distinct telescope everywhere. Get ready to gawk at celestial wonders!

Transcript:

The James Webb Space Telescope will be the source of incredible astrophotography for decades to come. Gawk, but mind your drool, please.

But how can we tell Webb’s images from other amazing telescopes? Afterall, incredible observatories around the world have snapped some beauties.

Well, Webb has a signature that you could look for.

You might say, James Webb… has a John Hancock.

So what is this signature?

Well – ever seen an image of space and notice that the stars have thin spikes coming off em? Often they look like plus signs. These are called diffraction spikes.

And they’re complete artifacts of the telescope.

See, when light from a point source enters a telescope, the edges of the mirrors diffract light, so different shaped mirrors make different diffraction spikes.

And, the arms that help hold the telescope together also diffract the light.

Based on Webb’s unique design, it has six strong spikes and two lesser, horizontal ones. It’s Webb’s very own. Once you notice it, you’ll recognize its handwriting everywhere.



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Observación del cometa Nishimura desde ciudad

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Este miércoles 30 de agosto puse el despertador un poco antes de lo normal con la intención de observar el cometa Nishimura desde ciudad, algo casi de locos aunque no es la primera vez que observo un cometa desde casa a pesar de la contaminación lumínica.

Tenía ya preparado el telescopio en el salón desde la noche anterior, que estuve observando un rato Saturno, y también me llevé la Canon para hacer alguna foto. Encendí el telescopio, el Mak127 sobre la AZ-GTi, y alinee con las estrellas Castor y Betelgeuse. Recientemente actualicé el firmware de la montura para ponerla en modo altacimutal ya que apenas la uso en ecuatorial, y en esta postura el buscador del tubo quedaba siempre en una posición muy incómoda (con firmware EQ el tubo se monta a la derecha del brazo).

Con el ojo puesto en el ocular de 32 mm me puse a escudriñar el cielo por la zona donde se suponía que estaba el cometa pero no dí con él. Tras sopesarlo y teniendo en cuenta que el tiempo corría en mi contra (el amanecer astronómico estaba a pocos minutos) decidí meter las coordenadas que encontré en heavens above en el mando. Inicialmente no vi nada pero en cuanto moví un poco el telescopio reparé en una pequeña mancha gris difusa. Usando un poco de visión indirecta salí de dudas, efectivamente ahí estaba el cometa C/2023 P1 Nishimura.

Se encontraba situado entre 3 estrellas, justo en el borde derecho del triángulo, próximas a 28 Cnc. Rondaría la magnitud 7.5. Como tal era visible únicamente la coma, no había núcleo ni cola. Sin duda la contaminación lumínica me privaba de detalles pero no voy a quejarme. No todos los días uno es capaz de observar un cometa desde casa. Lo que más me fascina es que ese cuerpo lleva vagando por el espacio cientos de miles de años y solo lo podemos ver durante un breve tiempo.

nishimura astrocid
Cometa Nishimura fotografiado por Rodrigo Martínez @astrocid

Recientemente he leído que nuevos cálculos han indicado que este cometa tiene un periodo de unos 519 años y que no se trataría de un cometa interestelar como se pensó en un principio. También se especula con que en realidad lo que estemos viendo sean los restos que quedan de un cometa que fue mayor años atrás y que ha ido desintegrándose con sus repetidas aproximaciones al Sol. Incluso se especula que pueda ser el causante de la lluvia de estrellas Sigma-hídridas.

Para poder observar algún detalle más me cubrí la cabeza con un paño negro que tengo para observación visual que siempre ayuda algo cuando estás en zonas con claridad. Tras dejar que mis ojos se acostumbraran a la oscuridad durante unos minutos ya me costaba menos encontrar el cometa y podía verlo con visión directa. Incluso me dió la sensación de poder apreciar algo de cola pero ya no se si era producto de mi imaginación.

Durante los próximos días el cometa estará más y más bajo en el horizonte y aunque cada día estará un poco más brillante será más difícil de observar por su proximidad al Sol. Además la meteorología va a empeorar durante los próximos días y la llegada de una DANA nos va a impedir observar por aquí este cometa durante los próximos 4 o 5 días.



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Nuevo impacto registrado en Júpiter

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De nuevo Júpiter ha sufrido el impacto de un objeto de grandes dimensiones, posiblemente un asteroide o un cometa. El evento fue registrado por varios telescopios a las 16:45 UT del 28 de agosto.

En las imágenes se puede apreciar un súbito aumento de brillo en una zona del planeta, un breve destello que solo se puede explicar por la colisión con otro objeto celeste. No es la primera vez que esto sucede, ya hemos visto con anterioridad eventos similares por lo que hay múltiples telescopios capturando constantemente imágenes del planeta y monitorizando si se producen destellos similares.

En esta ocasión el proyecto OASES (Organized Autotelescopes for Serendipitous Event Survey) y PONCOTS (Planetary Observation Camera for Optical Transient Surveys) publicaron una alerta sobre el evento y fueron varios los astrónomos aficionados, muchos de ellos japoneses, que confirmaron haberlo capturado.

El gran tamaño y la masa de Júpiter producen una gran atracción gravitatoria para estos cuerpos menores de nuestro sistema solar. En ocasiones sus órbitas son modificadas y en otras, como ésta, les pone en rumbo de colisión.

Por el momento se desconocen más detalles sobre el tamaño y órbita del objeto que chocó contra Júpiter.

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James Webb Telescope drops another out-of-this-world photo of distant spiral galaxy

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Another awe-inspiring magical image of deep space has been captured by the James Webb Space Telescope (JWST). Released on August 29, the latest high-resolution photo shows us a glimpse of a spiral galaxy that is found 27 million light years away from Earth in the Canes Venatici constellation.

Known as the Whirlpool Galaxy, or Messier 51a, it has been a central focal point for astronomers and astrophotographers for years (it was first discovered in 1773) but has never before has it been viewed in such fine detail.

The most recent image shows a red whirlpool galaxy with protruding spirals and a bright bluish-white core. While you might not be able to get such a high resolution even with the best cameras for astrophotography, this bedazzling galaxy is sometimes visible from Earth.

• Check out the best telescopes for astrophotography so you can capture stunning photos of the night sky from your back garden

Image of the M51 galaxy from James Webb Telescope

Image of the M51 galaxy from James Webb Telescope

Taken using the JWST main near-infrared camera (NIRcam) and a mid-infrared instrument (MIRI), the two separate photos have been combined into a composite to create a truly out-of-this-world galactic portrait. These incredibly advanced camera systems capture the infrared light that the eye cannot see and decode the data to create images scientists can study to unlock the secrets of our universe. It’s thought that the shape of M51 is due to its close proximity to the nearby dwarf galaxy NGC 5195 and its spiraling arms are formed through its strong gravitational influence.

Up until now, the clearest image we had of the M51 galaxy was taken by the Hubble Telescope in 2011 but it was nowhere near as in-depth and detailed as the JWST offering. The actual image has been colorized so we can distinguish areas of ionized gas created by recently formed star clusters (the orange and yellow buts) while the darker areas represent empty cavities necessary for the galaxy to maintain its spiral shape.

Image of M51 galaxy by James Webb Telescope

Image of M51 galaxy by James Webb Telescope

This latest image is part of a body of research known as Feedback in Emerteging Extragalactic Star Clusters or for east, FEAST. Since the James Webb telescope is 100 times more powerful than the Hubble Telescope, it enables scientists and astronomers to discover even more about deep space. The European Space Agency commented, “Webb is opening a new window into the early stages of star formation and stellar light as well as the energy of reprocessing gas and dust”.

Not only do these images enable us to develop a deeper understanding, but they are signs that the instruments onboard the JWST are still fully functional following some concern there have been some technical issues. While the NIRcam image and the MIRI image offer two different perspectives of the same galaxy, the combined composite offers exaggerates the remarkable wonders of this “grand spiral staircase sweeping through space” – a term that NASA has used to describe it.

Image of M51 galaxy taken by James Webb telescope

Image of M51 galaxy taken by James Webb telescope

Also check out the best telescopes for kids or the best telescopes for beginners

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Nikon Z8 review | Live Science

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Key specifications

Type: Mirrorless
Sensor: 45.7MP full frame
Lens mount: Nikon Z
ISO range: 64-25,600 (exp 32-102,400)
Viewfinder: Electronic, 3.69m dots
Video capability: 8K 60p / 4K 120p
Weight: 2lbs 0.1oz
Size: 56.7 x 46.5 x 32.7 inches
Memory card: 2x CFexpress B

The Nikon Z8 is referred to by Nikon as both “a baby Z9” and “the true successor to the Nikon D850”. That’s high praise indeed, with the Z9 being the company’s cutting-edge, flagship mirrorless camera, and the D850 being widely regarded as the finest DSLR ever made. 

Both labels are wholly accurate, though, as the Nikon Z8 lives up to every inch of the hype. With 45.7MP resolution, 8K 60p video and up to 120fps burst shooting, this can handle almost anything you throw at it; its continuous shooting speed and ferocious autofocus obviously make it one of the best wildlife cameras on the market, but it’s also an absolute powerhouse for anything from astrophotography to portraiture. 

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iPhone 15 Pro Max vs. Galaxy S24 Ultra camera face-off — which flagship could win?

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People would agree that cameras are what separates the good phones from the best phones. That’s what makes an iPhone 15 Pro Max vs. Galaxy S24 Ultra camera face-off intriguing on so many levels, thanks in part to how they could be in line for the best camera phones around when they’re officially released.

Apple’s Wonderlust event is full steam ahead now that the September 12 date is official, and it’s where we’ll most likely be introduced to its iPhone 15 lineup — including the highest-end model of the bunch in the iPhone 15 Pro Max. Whether Apple decides to call it that, or perhaps switch the name to the iPhone 15 Ultra moniker, there’s no denying that this high-end phone is going to be accompanied by new cameras that could help it dethrone the Galaxy S23 Ultra, the current camera phone king.

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Blue supermoon: How to see it in the Kansas City area | KCUR

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Amateur astronomers and idiom lovers will both have reason to rejoice this week: It’s the once in a blue moon when an actual blue moon will rise in the sky.

And it’s not just any blue moon. It’s a rare blue supermoon. The Earth’s lunar sidekick will seem extra big and bright as it reaches its fullest stage on Wednesday.

We won’t see this particular lunar twofer again until 2037, so here’s what you need to know to make the most of it.

First things first: What is a supermoon?

A perigean full moon, better known as a supermoon, happens when the moon is full during the closest point in its orbit around Earth.

According to NASA, the moon’s typical orbit ranges between 226,000 and 251,000 miles from Earth, but variances can bring it a bit closer or farther away. Only the closest three or four approaches each year qualify as supermoons.

The last supermoon fell earlier this month, on Aug. 2, inspiring photographers from all over the world to document the big and bright spectacle, from New York’s moody skyline to light-filled late night soccer matches in South Africa.

Yet the supermoon coming up this week will be even bigger and brighter — the biggest and brightest of 2023 — because the moon will be “exceptionally close” to Earth at 222,043 miles, according to The Old Farmer’s Almanac — nearly 17,000 miles closer than average.

This means it’ll appear “about 8% larger than a normal full moon and 15% brighter than a normal full moon,” according to Dave Teske, the lunar topographic studies coordinator for the Association of Lunar and Planetary Observers.

And while that might not make a hugely discernible difference to the naked eye, it’ll still be a sight to behold.

As Teske put it, “It’ll be big and bright and beautiful.”

But it’s not just a supermoon. It’s a blue supermoon

While the term “supermoon” references the moon’s orbit in relation to Earth, a blue moon has to do with frequency. Confusingly, it doesn’t have anything to do with color, either (though there was one time when a blue moon actually turned blue).

The moon takes 27.3 days to orbit the Earth, but because of how the sun’s light hits the celestial body, it takes 29.5 days to complete its lunar cycle from one new moon to the next. So it’s rare for us on Earth to see two full moons in the span of a single month. When we do, we call it a “blue moon.”

The term “blue moon” is also used in some circles to describe the third of four full moons in an astrological season.

And the idiom “once in a blue moon” is used to describe a rare but nonetheless recurring event. But according to NASA, blue moons aren’t actually all that rare, recurring every 2.5 years or so.

A blue supermoon, however, happens far less frequently. The last blue supermoon was in December 2009, and the next one won’t be until January 2037, NASA reports.

When and where can I see it?

This year’s blue supermoon will officially turn full at 9:36 p.m. ET on Aug. 30, according to Space.com, but to the naked eye, it’ll look just as full from Tuesday night to Friday morning, with the shaded strip appearing so narrow as to be virtually imperceptible.

And, if it’s an especially big moon you’re after, consider catching the moonrise in the east or moonset in the west. Experts say this is when foreground objects combine with a low-hanging moon to create the “moon illusion” — the time when the moon tends to look the largest.

(You can check the local rising and setting times for your area using the U.S. Navy’s Moonrise calendar).

Anyone looking to take in more detail of the lunar surface could use binoculars, a telescope, or an astrophotography lens. But astronomers like Teske say those tools aren’t necessary for a moving experience.

“Get out there and observe it. Just enjoy the beautiful view of the moon,” he said. “Really think about what you’re seeing out there.”

After all, this isn’t just a hunk of rock orbiting the Earth about a quarter of a million miles away. It could be the next frontier.

Just in the last week, the Indian Space Agency successfully landed a spacecraft on the moon’s south pole, where frozen water craters could fuel future missions. Japan’s space agency, JAXA, nearly launched a moon lander (but postponed the moonshot due to strong winds).

And the private company SpaceX paired with NASA to dock a crew of astronauts at the International Space Station, in order to perform experiments that might one day make it easier to travel to the moon and back.

“We’re doing things with the moon now that are building this slow and steady public interest,” said Noah Petro, a research scientist with NASA’s Goddard Space Flight Center.

Petro said that the value of supermoons like these is that they “allow us to take a moment and revel, and enjoy that nearest neighbor and space.”

“It’s not so far away that we can’t see it. It’s effectively right there in our backyard,” he added.

One note of caution: This moon could bring an elevated risk for flooding

But those looking to observe the moon from a beach should consider checking conditions first.

The close proximity of the moon means that for several days this week, the range of tides will be greater than normal.

The moon will exert 48% more tidal force during the spring tides of Aug. 30 compared with two weeks earlier, according to Space.com. Higher tides could get more high, which could cause some coastal flooding.

That risk will be especially heightened along the gulf coast of Florida, where Hurricane Idalia is expected to make landfall early Wednesday.

NPR’s Dustin Jones contributed reporting.

Copyright 2023 NPR. To see more, visit https://www.npr.org.



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It’s big! It’s bright! It’s a rare blue supermoon! Here’s how to check it out

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Amateur astronomers and idiom lovers will both have reason to rejoice this week: It’s the once in a blue moon when an actual blue moon will rise in the sky.

And it’s not just any blue moon. It’s a rare blue supermoon. The Earth’s lunar sidekick will seem extra big and bright as it reaches its fullest stage on Wednesday.

We won’t see this particular lunar twofer again until 2037, so here’s what you need to know to make the most of it.

First things first: What is a supermoon?

A perigean full moon, better known as a supermoon, happens when the moon is full during the closest point in its orbit around Earth.

According to NASA, the moon’s typical orbit ranges between 226,000 and 251,000 miles from Earth, but variances can bring it a bit closer or farther away. Only the closest three or four approaches each year qualify as supermoons.

The last supermoon fell earlier this month, on Aug. 2, inspiring photographers from all over the world to document the big and bright spectacle, from New York’s moody skyline to light-filled late night soccer matches in South Africa.

Yet the supermoon coming up this week will be even bigger and brighter — the biggest and brightest of 2023 — because the moon will be “exceptionally close” to Earth at 222,043 miles, according to The Old Farmer’s Almanac — nearly 17,000 miles closer than average.

This means it’ll appear “about 8% larger than a normal full moon and 15% brighter than a normal full moon,” according to Dave Teske, the lunar topographic studies coordinator for the Association of Lunar and Planetary Observers.

And while that might not make a hugely discernible difference to the naked eye, it’ll still be a sight to behold.

As Teske put it, “It’ll be big and bright and beautiful.”

But it’s not just a supermoon. It’s a blue supermoon

While the term “supermoon” references the moon’s orbit in relation to Earth, a blue moon has to do with frequency. Confusingly, it doesn’t have anything to do with color, either (though there was one time when a blue moon actually turned blue).

The moon takes 27.3 days to orbit the Earth, but because of how the sun’s light hits the celestial body, it takes 29.5 days to complete its lunar cycle from one new moon to the next. So it’s rare for us on Earth to see two full moons in the span of a single month. When we do, we call it a “blue moon.”

The term “blue moon” is also used in some circles to describe the third of four full moons in an astrological season.

And the idiom “once in a blue moon” is used to describe a rare but nonetheless recurring event. But according to NASA, blue moons aren’t actually all that rare, recurring every 2.5 years or so.

A blue supermoon, however, happens far less frequently. The last blue supermoon was in December 2009, and the next one won’t be until January 2037, NASA reports.

When and where can I see it?

This year’s blue supermoon will officially turn full at 9:36 p.m. ET on Aug. 30, according to Space.com, but to the naked eye, it’ll look just as full from Tuesday night to Friday morning, with the shaded strip appearing so narrow as to be virtually imperceptible.

And, if it’s an especially big moon you’re after, consider catching the moonrise in the east or moonset in the west. Experts say this is when foreground objects combine with a low-hanging moon to create the “moon illusion” — the time when the moon tends to look the largest.

(You can check the local rising and setting times for your area using the U.S. Navy’s Moonrise calendar).

Anyone looking to take in more detail of the lunar surface could use binoculars, a telescope, or an astrophotography lens. But astronomers like Teske say those tools aren’t necessary for a moving experience.

“Get out there and observe it. Just enjoy the beautiful view of the moon,” he said. “Really think about what you’re seeing out there.”

After all, this isn’t just a hunk of rock orbiting the Earth about a quarter of a million miles away. It could be the next frontier.

Just in the last week, the Indian Space Agency successfully landed a spacecraft on the moon’s south pole, where frozen water craters could fuel future missions. Japan’s space agency, JAXA, nearly launched a moon lander (but postponed the moonshot due to strong winds).

And the private company SpaceX paired with NASA to dock a crew of astronauts at the International Space Station, in order to perform experiments that might one day make it easier to travel to the moon and back.

“We’re doing things with the moon now that are building this slow and steady public interest,” said Noah Petro, a research scientist with NASA’s Goddard Space Flight Center.

Petro said that the value of supermoons like these is that they “allow us to take a moment and revel, and enjoy that nearest neighbor and space.”

“It’s not so far away that we can’t see it. It’s effectively right there in our backyard,” he added.

One note of caution: This moon could bring an elevated risk for flooding

But those looking to observe the moon from a beach should consider checking conditions first.

The close proximity of the moon means that for several days this week, the range of tides will be greater than normal.

The moon will exert 48% more tidal force during the spring tides of Aug. 30 compared with two weeks earlier, according to Space.com. Higher tides could get more high, which could cause some coastal flooding.

That risk will be especially heightened along the gulf coast of Florida, where Hurricane Idalia is expected to make landfall early Wednesday.

NPR’s Dustin Jones contributed reporting.

Copyright 2023 NPR. To see more, visit https://www.npr.org.



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August’s Blue Moon, the biggest full moon of 2023, rises this week

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On Wednesday, Aug. 30, you’ll no doubt hear the mainstream media proclaiming that on that night we will have an opportunity to witness a “supermoon.” It’s a term, or more specifically, a branding, of relatively recent origin. It originated not from astronomy, but astrology; first coined by an astrologer, who arbitrarily defined it as “a full moon which occurs with the moon at or near (within 90-percent of) its closest approach to Earth in a given orbit (perigee).” 

Indeed, at 12 noon ET on that fifth Wednesday of August, the moon will arrive at perigee, its closest point in its orbit relative to Earth at 221,942 miles (357,181 km) away. And 9 hours and 36 minutes later, the moon will officially turn full. Although a full moon theoretically lasts just a moment, that moment is imperceptible to ordinary observation, and for a day or so before and after, most will speak of seeing the nearly full moon as “full”: The shaded strip is so narrow, and changing in apparent width so slowly, that it is hard for the naked eye to tell whether it’s present or which side it is. 

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