Monthly Archive September 16, 2021

When is a camera worth buying?

September 16, 2021 Comments Off on When is a camera worth buying? By admin

When is an instrument worth buying.

It’s not an easy question to answer.

There are a lot of cameras that are worth a lot, but not all are equally important.

There is a huge difference between buying an iPhone or a DSLR.

When you are shopping for a camera, there are a few things to keep in mind.1.

Quality: Many cameras are made with great quality, but they have their shortcomings.

Some cameras have an amazing autofocus or excellent low-light capabilities.

But, many cameras suffer from poor color reproduction.

Some are not well-suited for outdoor scenes, or some have a limited number of shooting modes.2.

Price: If you’re going to spend a lot more than the average, then the price tag should be the first thing you look at.

It might not be a camera that will bring in much cash, but you should be able to afford it.3.

Availability: If a camera is available at a great price, then it might be worth the extra money.

But some cameras will never be available, and you might want to look at a cheaper alternative.4.

Features: A camera should have a few features that will help you make the most of it.

That’s why it’s important to consider what other features the camera has.

The Canon EOS 7D has a great low- light performance, excellent color reproduction, and a large range of shooting options.

But it has a number of other issues that make it a bad camera for the price.

In the table below, we’ve ranked the most important factors that affect the price of an instrument.

They range from good quality to poor quality, from a wide range of cameras to a few specific cameras that have very specific needs.1) Optical performance and optics qualityThe most important factor to consider is the quality of the lens.

Is it a prime lens or an autofocused lens?

Most lenses have the same performance.

A prime lens is a lens that has the highest optical resolution.

A typical prime lens has a resolution of 10 million dots.

Autofocus lenses have a smaller optical resolution and are much more expensive than a prime.

If the image quality is great, then you should go with a prime, but if it’s not, then go with an autfocal lens.2) Resolution of the sensor: A lens with a high resolution will have a much higher dynamic range than a lens with lower resolution.

So, the higher the resolution, the better the dynamic range.

A lot of digital cameras have a resolution that is around 2-3 times that of a regular camera, so a camera with a higher resolution has a higher dynamic- range.3) Size and weight: A large sensor means that the camera will weigh more, which means you’ll have to take more shots.

So a large camera with low resolution will require you to shoot in slow motion, while a smaller camera with higher resolution will work better in slow-motion.

A medium sized camera will work well in low-angle shots, while larger cameras will work best in high-angle.4) Depth of field: Depth of focus is the ability of a lens to accurately focus on an object.

If a lens has good depth of field, then that lens will be sharp.

If not, you will have to get a better lens for that specific object.5) Size of the aperture: A smaller lens will produce a narrower field of view.

A smaller aperture means that a larger number of objects will be in focus.

For example, a 25mm lens will allow you to get much more detail in the details of a building, while an 80mm lens gives you a much wider field of focus.6) Lens aperture: The aperture is the aperture that gives the camera a specific focal length.

A f/1.4 lens will give you a f/4 aperture, while any f/2 lens will provide you with a f of 1.7.

A lot of lenses have very narrow an f/5.6 lens, which makes it hard to focus.

A few of the best lenses have f/11.5 and f/16 lenses.

The f/3.5 lens will work very well for shooting low-contrast subjects.7) Resolution: If the sensor resolution is very good, then this is a good thing.

If it’s good, the lens will not be as good.

It will have less sharpness.

A good sensor resolution will also mean that you can get a lot less noise in the image.

A small sensor with low sensor resolution can produce noise at low light levels.8) Aperture ring: The focus ring is a piece of plastic on the camera that controls the focusing.

It moves as the lens moves, and it can move up and down.

The ring can be damaged if you drop it, but it is not a major problem.9) Focus speed: Focus speed is the

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How to get better at klein optical objects

September 15, 2021 Comments Off on How to get better at klein optical objects By admin

Posted June 02, 2018 06:18:18 klein optics are among the most widely used optical instruments in the world.

They are used in many different fields of astronomy, including: Astrophysics: They provide optical elements for the Hubble Space Telescope, making it possible to observe faint galaxies and other objects.

Astronomy: They can detect small asteroids, comets, and even asteroids of other planets in the solar system.

Astronautics: They help determine the size of objects like asteroids or comets by measuring their orbital velocities.

Physical Sciences: They are the main building blocks of all materials used in modern science.

Chemistry: They make it possible for chemical reactions to take place more quickly.

Astronomerics: Klein optics have been used in astronomy since the 19th century and were originally used in telescopes to study light.

Today, they are used for astronomy, astrophysics, astronomy and other fields.

They can be used to measure the properties of objects or to image the planets.

They have become a part of everyday life in many parts of the world because they are very reliable, and because of their simple design, there is no need to buy expensive optical instruments.

If you’re looking for an inexpensive alternative to buying expensive optical instrument, klein telescopes can be a good option for you.

You can learn how to use one of the best klein spectrometers.

This article is part of a series about optics, and you can read the rest of this article.

klein optic instruments klein (also called a “synthetic”) optical instruments are used to create images of the object.

They usually consist of a pair of mirrors, a camera and a telescope.

The mirror, called a diaphragm, is attached to the mirror of the mirror-less instrument.

The camera is mounted on a tripod, and the telescope is mounted to the lens of the instrument.

In order to take a good picture of the target object, the telescope must be focused at the object and the diaphram is rotated to achieve a “sharp focus”.

When the telescope focuses at an object, it magnifies the image.

This sharp focus produces the image on the telescope’s screen.

The image on a klein telescope consists of a small number of dots.

A larger number of individual dots are called magnitudes.

klons are also used in astronomical photography, which is when you focus the camera at an astronomical object, and when you look at a single dot.

These dots are often called magnifications.

kleines can be useful for observing a variety of objects, such as galaxies, planets, stars and other stars.

If your telescope is designed with an optical system, it can be easier to use.

However, if you have a camera with a small aperture, it may be harder to use a telescope with a large aperture.

Most modern telescopes are designed with a relatively large aperture, and it is easier to focus on objects with larger magnifications, because the camera’s lens is focused at a small distance.

klenow lenses are usually used for telescopes with a fixed focus, so that the telescope will focus on the object without needing to be focused in a particular direction.

kleen lenses are used with fixed-focus optical instruments to provide images of distant objects that are closer than the object being photographed.

For example, if a telescope is fixed-focal, you can use a kleen lens to take an image of the stars in Orion.

However it is not necessary to have the telescope fixed-lens.

You will need to use either a klenows or a klens if you are photographing objects that do not have fixed focus.

You may also be able to use both, such that both images are of the same object.

If the object is not fixed-focused, it is possible to use the kleen to take images of planets and other celestial objects.

You cannot use a lens with a larger diameter than your telescope’s focal length.

klene lenses are lenses that have a smaller diameter than the diameter of the telescope.

A klene lens has a focal length of 1/2 the telescope focal length, and its lens is designed to focus at a distance of about 1.5 times the diameter.

A typical klenew lens will have a focal depth of 1.4 times the telescope field.

A conventional klenene lens will focus at the focal length specified by the telescope manufacturer.

klées are usually designed with fixed focal lengths, and are used instead of a kleine lens.

The lens has an aperture that is 1.2 times the focal diameter of your telescope.

This aperture allows the lens to focus accurately on the target.

If both the eyepiece and the eyeline are fixed, you will need a klée lens.

If a fixed eyepieces is used, you need a fixed-end eyepoint, which has a fixed length and can

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How to watch the best sports and the most memorable moments of the past 10 years

September 14, 2021 Comments Off on How to watch the best sports and the most memorable moments of the past 10 years By admin

The Irish people will get their first glimpse of the game at the 2018 Rugby World Cup in Ireland, with the Irish Rugby Union (IRFU) setting up the first-ever video stream from the game.

In 2018, Ireland won the Rugby World Championship with a 13-16 victory over France.

They were then knocked out of the tournament by Italy in the quarter-finals, with both teams coming from the same side of the Atlantic.

In 2019, they beat New Zealand and Fiji in the semi-finals before beating Wales in the final.

Ireland beat France again in the 2017 Rugby World Finals, and then beat Italy in a dramatic encounter in the 2019 World Cup final.

It is understood that the IRFU will have the ability to provide live video coverage from the 2018 tournament as well as from the 2019 event, as part of a partnership with ITV.

The video stream will be available on ITV’s WatchESPN app, and will be powered by the company’s proprietary technology.

The Irish Rugby union has been in talks with the ITVs WatchESPN platform for the last few years, with ITV currently running live coverage of the 2018 World Cup.

In an exclusive interview with The Irish Sun, the IRU chief executive, Brian Cowen, said the IRB would be delighted to take on the responsibility of providing a unique and comprehensive video stream of the sport’s best games.

“We’ve got a great team behind us at the IRWU and they’re incredibly dedicated and professional,” Cowen said.

“It will be great to be able to provide our viewers with a comprehensive look at the rugby of the world’s greatest sporting nation.”

WatchESPN has a great portfolio of sports content, and we look forward to bringing that content to Irish fans as part the IRVU’s exclusive video platform.

“The IRFU has been keen to see how the technology would work in conjunction with its own content and social media platforms.”

I’m sure that in the future, with our technology and the fact that we are now the official video streaming partner of the IRFU, we’ll be able get a great deal more coverage,” Cowens said.

The IRB will also be able provide a unique look at their matches, with an online scoreboard and live video stream, which will be a vital part of the match day experience.

The game will be played at the same time as the Irish Super League season and will kick off on February 10, 2019.

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How to build your own telescope from scratch

September 13, 2021 Comments Off on How to build your own telescope from scratch By admin

In this article by The Verge’s Matt Young, we take a look at the science and engineering behind building a telescope that’s actually pretty cool.

It’s called a photonic aperture, and it’s not just a fancy name.

The idea behind photonic telescopes is to build something that can shoot light at the sky that is at least as good as, or even better than, the optical telescopes in your garage.

And for a good reason: photonic optics can create images that are much sharper than the best optical telescopes.

That’s because, unlike optical telescopes, which are made up of light and are typically mounted to a glass or metal housing, photonic instruments are made out of a metal lens, so light from the light source bounces off of the lens and gets refracted in the lens to produce a picture.

To put that in perspective, the difference between the refractive index of glass and that of a glass tube is about 40.

That means that the refraction in a lens is less than one part in a million.

But that doesn’t mean that the optical tube is actually less sharp than the lens.

It just means that light coming from the source will be less affected by refraction than light coming off of a mirror.

That helps to give a much more detailed picture.

And that’s what makes the Photonic Astrophotography (PA) telescope, a pair of optics mounted to the side of the telescope, particularly useful.

The optics are built around a single lens that’s about 1.3 millimeters thick and is mounted on a base that’s 2 millimeters wide.

That makes the PA telescope nearly twice as wide as the largest optical telescopes on the market.

That width also means that it can fit a lot of instruments.

As Young writes: If you have a large enough telescope and the right instruments, you can actually get a lot out of it.

For example, if you’re a student in physics, you could use it to test your theories of gravitational waves, which could potentially lead to a discovery that could revolutionize how we understand the universe.

And you could also use it for astrophotography.

Aperture optics The PA telescope is equipped with an array of 16 lenses, each about 3.5 millimeters across.

That allows it to produce images that look a little bit like the real thing.

In fact, you’ll notice that the PA telescopes lens is actually very similar to the one that NASA uses to look at distant objects.

The PA optics are mounted on two metal housings that are connected by a small metal tube.

The tubes are made of steel and the tube is made of aluminum, which is much more durable than steel.

That tube also houses a pair a pair small mirrors that can magnify the image that’s being produced by the PA optics.

The mirrors are also a little bigger than the mirrors used in optical telescopes because they’re larger in diameter.

The size of these mirrors is important, because they help direct light towards the optics and away from the telescope.

The aperture optics are made from a single tube that is about 1 millimeter thick and can be mounted on either a glass, or metal, housing.

The tube is a very thin piece of aluminum with a hole drilled in the middle to connect it to the housing.

So, when the PA Telescope is mounted, the tube itself is the only part of the housing that is connected to the telescope by a connection.

The other pieces are made in a way that makes them easily removable from the housing and can easily be replaced when they’re no longer needed.

That thin, flexible tube allows the optics to be attached to the PA housing without the need for any special hardware.

There’s also a pair the PA optical instruments, which consist of a lens and a pair, or a series of mirrors.

The lens and the mirrors are made by using two different types of materials, each of which has a specific optical characteristics.

For instance, the glass lens is a light-emitting diode that has a wavelength of about 100 nanometers.

That wavelength is much longer than that of the light that the photonic lens produces.

It has the ability to produce very bright, high-contrast images, while the mirrors on the PA instruments are also capable of producing very bright and bright images.

The photonic lenses also have a number of optical properties that are important for imaging objects in the sky.

One of those optical properties is called refractive efficiency.

That tells you how much light gets reflected by a surface.

Refraction is what causes the colors of a light that is reflected from a surface to appear different than the colors that it actually was.

That also means the PA lenses and the optical instruments are much better at focusing light on objects in deep space.

As a result, the PA instrument can get a very clear image even in the presence of a lot more light.

Because the PA mirrors and the optics are light-absorbing, the light coming into the telescope doesn’t cause any visible distortion or d

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The next generation of solar imaging telescope is coming from Axios

September 13, 2021 Comments Off on The next generation of solar imaging telescope is coming from Axios By admin

Axios reporters are reporting that the next generation, the next Genop telescope will use an array of 12 high-precision optical instrument bases that will allow it to track and image the entire night sky.

Axios says the Genop will be built with a focus on providing the best possible imaging experience to all users.

The Genop should also allow users to do more detailed research, by tracking the motions of objects in the night sky, and then creating detailed maps of those motions.

The instrument bases will allow the Genops ability to provide a “broad range of images to the users, while retaining the precision necessary for detailed analysis,” Axios said.

Genop is also expected to offer users the ability to analyze the motion of stars and galaxies.

The next Genops will also offer “a robust and robust array of high-resolution optical imaging,” the Axios report said.

The Axios Genop has been named one of the best optical telescopes in the world by the American Astronomical Society and the National Optical Astronomy Observatory, according to the news outlet.

It has a $1.5 billion price tag.

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Argentina to host England in friendly

September 12, 2021 Comments Off on Argentina to host England in friendly By admin

Buenos Aires (AP) Argentina is set to host the first of three World Cup qualifiers for the 2019 FIFA World Cup in 2019.

The first game of the three will take place on Sept. 15 at Estadio Azteca.

The third will take the place of the Argentina-Uruguay friendly in May 2020.

Argentina defeated Uruguay in the World Cup opener, 2-0, but lost 1-0 in extra time to eventual winners Uruguay in extra-time in the semifinal.

The final will be played on Sept, 29 at Estado de los Angeles, and will be hosted by Argentina’s coach Luis Enrique, who is expected to take charge of the game.

Argentina plays the winner of those two games in the quarterfinals.

Argentina beat Ecuador 2-1 in the 2018 Copa America, the last time Argentina was to host a World Cup qualifier.

[FIFA] The Definitive Guide to FIFA 15’s [Optical] Lab

September 11, 2021 Comments Off on [FIFA] The Definitive Guide to FIFA 15’s [Optical] Lab By admin

article From the moment the game launches on December 8, gamers can grab a guide to all the new equipment available in FIFA 15.

As we get closer to release, we’ll be sharing more on all the latest tech, tricks, and tips.

Today, we’re looking at a new optical instrument, the Optical Laboratory.

This new optical tool allows players to create a variety of different shots, and also allows for a new way to look at the camera.

Here’s how it works.

When you click on the optical lab, a pop-up window appears to the right of the main menu.

From here, you can pick a lens from the available categories.

You’ll be able to zoom in and out on the lens you want, or even rotate the camera to focus on any point in the scene.

You can also change the focus of the lens and position it to any part of the scene in the real-time.

Once you’re done with all that, click the camera button and the camera will automatically rotate and zoom to the selected lens.

In this tutorial, we used the Canon 60D lens for this shot.

To get the full-sized image from this lens, we selected the same focal length as the Canon 55-300mm zoom lens.

Once zoomed in, the lens will automatically change focus and position, and the lens itself will automatically appear in focus, allowing us to capture the perfect shot.

It’s also possible to add additional elements to your shots.

To do this, we made a small adjustment to the lens’ focal length, and then rotated it until we got a focus point at which we could capture a photo.

Now, the best part about this new tool is that it allows players a variety for how they can use it.

It allows you to shoot as many different angles as you want.

We shot this shot using the Canon 5D Mark III, which had an 85mm lens.

We chose the 45-300 mm lens to get a shot of the player as he is running away from the ball.

You could also create your own angle-of-view shot with the 45mm lens, but we prefer the 70-200mm lens because it’s sharper.

In the end, the only downside to this tool is the limited options.

However, it’s certainly a cool new addition to the game and we’ll update this guide with more information on it.

For more info on how to use this new Optical Lab, check out the video above.

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You’re Not the Only One who Likes Optical Instruments

September 11, 2021 Comments Off on You’re Not the Only One who Likes Optical Instruments By admin

You’re not the only one who likes optical instruments, even if you’re one of the many people who are completely convinced that it’s the most exciting thing that’s going to happen to astronomy in the next decade or two.

It’s just not true, of course, and if you believe in the magic of optical instruments in general, you have no business believing that their potential is limitless.

If you’re a serious professional astronomer, however, you might think you’re an expert on the subject, and the answer is no.

You’re wrong, and your views are a huge contributor to a very narrow and unhelpful set of beliefs about astronomy.

Here are ten common misconceptions about optical instruments and how they’re useful, and why they’re so hard to dispel.

Optical instruments don’t perform well in cold environments They’ve got all the hallmarks of a useful optical instrument: a strong lens, high resolution, a focal length, an aperture and a resolution that makes the instrument look like a telescope, to name a few.

They also have a very long focal length range, and can be used to detect faint objects or objects that you can’t see, like faint dust and ice.

That’s why they make good instruments for detecting galaxies or planets.

But for many other things, such as measuring the temperature of gas or dust, they’re useless.

Even though the instrument can detect light, it can’t detect anything.

That is, even though you can see it, it won’t emit light.

So it’s useless for detecting ice or gas that might exist at the temperature you’re looking for.

But optical instruments do perform better in warm environments.

They use a lot of energy to heat the lens and to drive a lens to focus, but the heat from the lens is converted to light in the optical system.

So the lens will be focused more accurately when the ambient temperature is higher, even when you’re at a very, very low altitude.

The image of a telescope on a hilltop in the Alps.

(Photo by Daniel J. Tissot) But when you use a telescope to focus a telescope with a small telescope, you’ll need a larger lens.

And the smaller the lens, the more energy you need to focus the telescope, because the lens needs to move faster than the telescope.

The energy required to focus an optical telescope can be calculated as: Where a is the aperture, f is the focal length of the telescope and L is the magnification of the lens.

For example, if you have a 5 mm telescope, the optical power required to make the image of the moon is about 1.5 times that of a 1.2-m telescope, and so you’ll use about one-third of the power of a 5-mm telescope to make an image of that moon.

But if you use the same lens with a 30 mm telescope and a 1 mm aperture, the image will be 1.8 times larger, because you’ll have to use twice as much energy to focus that telescope.

So you’ll get the same image with a bigger lens, but it will be a bit smaller in size.

A telescope with 10-mm focal length requires a bigger aperture to make it focus at the same focal length as the lens used to focus it.

A 12 mm telescope requires a 20 mm aperture to focus at a similar focal length to the one used to make a 1-mm image.

The difference is that the smaller aperture produces more light, which makes the image more visible.

So a telescope that uses a smaller lens is useful for objects in the night sky that aren’t visible with a large telescope.

But that’s not the whole story.

Optical telescopes use lots of light to illuminate them If you have the same aperture, it will use a larger amount of light than a 10- or 12-mm lens.

The amount of sunlight falling on the telescope will be proportional to the aperture used, so you get a higher image quality when you have less light.

This is called the refractive index of light, or the refraction index, and it determines how much light falls on the image when you take the image.

So if you want a very bright image with good contrast, the higher the aperture is, the brighter you can get.

But even at very high magnifications, the telescope can’t use as much light as a 10 mm telescope.

You need a telescope of about 1/10 of a power.

A 2.2 megapixel camera lens with an aperture of 10 mm.

(Image courtesy of NASA) That’s not to say that you shouldn’t use a 10 or 12 mm lens for things like high-contrast objects like planets and stars.

But you can only get that kind of image quality with a lens that’s 1/20 the size of the one you’re using.

So don’t expect that you’ll see a star that’s only 1/30 of a wavelength at the highest magnification.

If that’s your thing, then you

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Which Optical Urethrotomies Are Safe and Effective?

September 10, 2021 Comments Off on Which Optical Urethrotomies Are Safe and Effective? By admin

By Brian A. FongUpdated May 18, 2019 12:05:16This article is not intended to replace the advice of your healthcare professional.

We urge you to seek advice from your healthcare provider if you have an eye injury or condition.

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Why do some objects glow so brightly when they pass through the Milky Way?

September 10, 2021 Comments Off on Why do some objects glow so brightly when they pass through the Milky Way? By admin

By MICHAEL R. KURTISThe faint glow that some objects emit as they pass by the Milkyway is due to a special type of optical spectroscopic instrument called an optical epicornot.

The name is a play on the words “excitation” and “epicentro” — the latter meaning “light” and the former “light emitted by a substance.”

The name may suggest that the objects’ brightness is due mainly to the light that passes through their optical lens.

In fact, the bright glow may be caused by an electrical current flowing through the material, the authors say.

The authors report the results in the May 24 issue of Nature.

“When light interacts with the atoms in the sky, the atoms can be excited by a certain voltage, and as that voltage is decreased the atoms lose their electrons,” says Dr. Kuznetsova, an associate professor of physics at the University of Arizona.

“As the atoms change from one excited state to another, they have a slight tendency to glow with an intensity.”

The researchers found that when a light source passes through the lens of an optical telescope, the intensity of the emitted light depends on the size of the light source, and its position relative to the telescope’s eyepiece.

As the light travels through the telescope, it becomes brighter as it moves closer to the lens, and dimmer as it travels farther away.

The light emitted by an object passing through the Hubble Space Telescope (HST) is typically around 20 to 30 times brighter than the light emitted from a similarly-sized object passing in front of the telescope.

“This phenomenon is called a refractive index,” Dr. Kurtskaya says.

“It tells you how big an object you are looking at.”

When an object passes through a telescope, light from the object’s source (light from the sky) bounces off the telescope to hit the telescope (light emitted from the telescope).

The reflected light bends as it passes through, creating a “refraction” effect.

Light can then be seen as a wave.

When the waves meet, they create an image of the object in the telescope that can be seen from Earth.

This phenomenon has long been known as the “Hubble effect,” but the researchers wanted to know why it was there.

“We’ve been looking for something like this since the 1920s, and it has never been seen,” Dr, Kurtsaya says.

The researchers looked at more than 200 Hubble images taken in different wavelengths.

The team used software to analyze the image data, and they then compared the Hubble data with other Hubble data sets.

“We found that the Hubble effect is very strong,” Dr Kurtsoda says.

The Hubble effect occurs when the light from an object is shifted so that it hits the telescope instead of the ground.

The result is a brighter image.

The researchers found a similar effect in the light of distant galaxies, where light from distant stars is shifted as well.

The effect is most pronounced near the center of the galaxy, which is where the light has the most influence.

“If you were looking at a small portion of the Milky Kingdom, you would probably be able to see it,” Dr Kuznetskaya says, but “in fact, you wouldn’t be able, unless you were standing on a very high mountain or a volcano.”

The scientists found that there is a strong correlation between the intensity and distance from the source.

The greater the distance from an observer, the greater the Hubble-effect, and the brighter the light.

The scientists also found that some distant galaxies have the Hubble effects even when the source is closer to Earth.

In the case of the Andromeda galaxy, for example, the light at the distance of about 30,000 light years is only 10 times brighter as compared to the nearby Andromeda galaxy.

“These effects are so strong that we can detect them at very close distances,” Dr Kratsosky says.

In other words, distant galaxies can be detected by the telescope and detected in infrared.

The results show that even the brightest objects are not the only ones to have the effect.

“It’s hard to tell what the source of this Hubble effect might be, but this Hubble data may be a clue,” Dr Krazetsky says, referring to the optical telescopes that are capable of seeing stars in the Milky and nearby galaxies.

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