Telescope Eyepieces: The Weakest Link

Do you have a new telescope, or are you considering buying a new one? Hopefully, you have chosen a telescope with the best specifications for your budget, but before you can truly get the best out of your wonderful new window on the cosmos, you need to have something even more important than the scope – Eyepieces!

A lot of people new to astronomy, or new to buying astronomy equipment tend to concentrate on telescopes and unfortunately overlook eyepieces, settling for the basic set of 2 or 3 that come with the new telescope.

Eyepieces are probably the most important part of your observing equipment, as they are at the heart of your setup and can make your observing experience fantastic or disastrous, or make an average telescope great or an excellent telescope bad.

The Basics

Eyepieces are the part you look through and are responsible for magnification of the objects you see through the telescope. They come in many different magnifications and types, but it’s not rocket science. You will soon learn what eyepieces work well for seeing different astronomical objects.

Telescope eyepieces are designed to fit into the focuser of the telescope. Depending on your telescope, they come in two sizes 1.25” or 2” and there is .965” which is an older size and pretty much obsolete, unless you have an old telescope. Most telescopes can be fitted with adapters so both eyepiece sizes can be used.

Magnification

The magnifying power of any eyepiece is a simple equation expressed in millimetres: Divide the focal length of the telescope by the focal length of the eyepiece and your answer is the amount of magnification. Long focal length eyepieces such as 32mm and 25mm are lower magnification, while lower numbers like 10mm and 5mm are magnifying powerhouses.

It is always good practice to start observing an object with a lower power eyepiece such as a 40mm and gradually build up to higher powered eyepieces such as 10mm or lower. The reason for this is the telescope, human eye, seeing conditions and object being observed are all variable. Starting off with a high power such as 4.7mm may be a struggle.

Fainter objects such as nebula and galaxies are usually seen better with lower powers and you can really ramp up the power with bright objects like the moon.

Below are rough guides and are dependent on the telescope you use:

2mm-4.9mm Eyepieces: These are very high magnification and very difficult to use unless seeing conditions are perfect and the object observed is very bright, like the moon.

5mm – 6.9mm Eyepieces: These are good on bright objects such as the moon and bright planets, but are still very high power and work best with steady seeing conditions.

7mm – 9.9mm Eyepieces: These are very comfortable high magnification eyepieces and are excellent for observing brighter objects, a must for any eyepiece collection.

10mm – 13.9mm Eyepieces: These work well for all objects including brighter nebula and galaxies a good mid/high range magnification.

14mm – 17.9mm Eyepieces: These are a great mid range magnification and will help resolve globular clusters, galaxy details and planetary nebulae.

18mm – 24.9mm Eyepieces: These will work nicely to show wide field and extended objects, great mid-range magnification for objects like galaxy clusters and large open clusters.

25mm – 30.9mm Eyepieces: These are wider field eyepieces for large nebula and open clusters. A good finder eyepiece for locating objects before moving to higher powers.

31mm – 40mm Eyepieces: These are excellent for extended views and large star fields and make excellent finder eyepieces before moving to higher powers.

Eye Relief

Eye relief is the distance from the last surface of an eyepiece at which the eye can obtain the full viewing angle. If a viewer’s eye is outside this distance, a reduced field of view will be obtained and viewing the image through the eyepiece can be difficult. Generally longer eye relief is preferred.

Eye Relief Credit: qwiki.com

Apparent Field of View

This is the apparent size of the image in the eyepiece and can range from about 35 to 100 degrees. Larger fields of view are more desired.

Apparent Field of View Credit: starizona.com

Types of Eyepiece

There are many different eyepiece types, some old and now obsolete, some simple and some advanced.

The different types of eyepiece are purely governed by the configuration of the glass and lenses inside the eyepiece. Some giving exceptional eye relief, wide fields of view, colour correction etc.

Some different brands of eyepiece include: Huygens, Ramsden, Kellner, Plössl, Orthoscopic and Kellner.

The most common and popular eyepiece type is the Plössl due to its good all round performance, good eye relief, approximate 50 degree field of view, pinpoint sharpness and good contrast. Plössl eyepieces are made by many manufacturers now, but there are excellent examples from manufacturers such as Meade and Televue.

Finally we have exotic eyepieces such as Super Wide and Ultra Wide which are usually 2” eyepieces, with higher powers up to around 4.7mm at 1.25” and are usually in the domain of the large Dobsonian or Newtonian telescope user, but are just at home on smaller telescopes such as refractors or Cassegrains.

These eyepieces sport amazing eye relief and huge “port hole” 80 – 100 degree views with fully loaded premium optics, which are very forgiving on telescopes with optical aberrations and other problems. They can make average or poor telescopes great, but there is a cost; an example of which is my 14mm Ultra Wide which cost £500 ($800) just for one eyepiece and I have a full set! Combined, my eyepieces are worth much, much more than the telescopes they are used on, but it’s worth it!

Eyepieces are the most important part of your observing equipment, choose them and use them well, which will help you enjoy observing through your telescope.

Asteroid Observing Alert

2011 GP59 imaged remotely from the GRAS Observatory. Credit: Ernesto Guido & Giovanni Sostero

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A newly discovered asteroid could provide one of the best recent viewing opportunities for amateur astronomers, according to the British Astronomical Association. “This is the best NEO close approach these past few years and is bright enough to be observed visually in large (>20cm., or 8-inch) aperture telescopes when on the night of Thursday 14th it will appear as a faint slow-moving star,” writes Richard Miles, the director of the BAA’s Asteroids and Remote Planets Section.

UPDATE: See a new picture of asteroid 2011 GP59 from Ernesto Guido & Giovanni Sostero taken on April 14, 2011, below.


2011 GP59 imaged remotely from the GRAS Observatory. Credit: Ernesto Guido & Giovanni Sostero

Guido & Sostero sent us a note that they imaged 2011 GP59 early on April 14, remotely from the GRAS Observatory (near Mayhill, New Mexico USA) through a 0.51-m, f/6.9 reflector + CCD.

“It’s a single unfiltered exposure of 600 seconds, showing 2011 GP59 as trail with brightness fluctuations clearly evident,” they said.

(end of 4/14 update)

2011 GP59 was discovered just a few days ago and will make its closest approach to the Earth on April 15 at 19h UT at 1.39 lunar-distances. But it will be brightest at an average magnitude of 13.2 around 00h UT on the night of April 14/15 when Miles says it will be very favorably placed in the sky for observers worldwide.
The asteroid is approximately 60 meters in diameter and appears to be rotating very quickly, about once every 7.35 minutes. Its oblong in shape and rotation will vary the object’s brightness every 4 minutes or so.

Miles reported that David Briggs observing with the Hampshire Astronomy Group’s 0.4-m instrument on the evening of April 11 commented, “This is probably the fastest rotator I’ve seen so far in that it completely disappears from view every 3 to 4 images.”

This object was discovered on the night of April 8/9 by the Observatorio Astronomico de Mallorca (OAM) using a 0.45-m f/2.8 reflector at their La Sagra facilities (J75) in Andalusia, Spain (see http://www.minorplanets.org/OLS/ ). The observers involved were S. Sanchez, J. Nomen, R. Stoss, M. Hurtado, J. A. Jaume and W. K. Y. Yeung.

Brian Skiff of Lowell Observatory has completed a lightcurve analysis which can be found at this link, and positions can be found using the Minor Planet Center’s ephemeris service at this link. You can also find more information on this object from the website of the Remanzacco Observatory in Italy.

The British Astronomical Association is also seeking observations of the Moon on Friday, April 15, between 19:00 and 21:00 UT, when the Aristarchus and Herodotus area of the Moon will match the same illumination, to within +/- 0.5 degrees, as that observed during the famous Transient Lunar Phenomena (TLP) seen by Greenacre and Barr from Flagstaff observatory back on Oct. 30, 1963.

TLPs are very short changes in the brightness of patches on the face of the Moon, which can last anywhere from a few seconds to a few hours and can grow from less than a few to a hundred kilometers in size. This phenomenon has been observed by hundreds of amateur and professional astronomers, but how and why this occurs is not understood. Some astronomers believe that they are the outcome of lunar outgassing, where gas is being released from the surface of the Moon, but most commonly astronomers think it could be an effect from Earth’s own atmosphere.

If you want to help understand TLPs and perhaps observe an event like this for yourself, the BAA Lunar Section is looking for high resolution monochrome, or especially color, images of this area during this time period,, which favors observers in Europe.

But you can check this website from the University of Aberystwyth for many locations around the world of when would be a good time to observe a TLP.

See more information about how to observe a TLP and how to report your observations at the BAA website.

Sources: BAA, BAA (again) University of Aberystwyth

How to find Saturn in the Sky this Weekend

If you want to find the planet Saturn in the sky this weekend, but aren’t sure where to look, this guide should help you.

Saturn is visible all night long at the moment and is quite easy to find, as it is just past opposition which makes it quite bright.

Credit: Adrian West

Find the constellation of Leo the Lion (high in the Southern sky at around 10pm) by looking for the backwards question mark asterism (red in the diagram), which is the head of Leo. Find the last 2 stars in Leo’s body and draw an imaginary line through these 2 stars, and arc to the left and down until you reach a bright yellowish star. This is Saturn.

If you continue drawing this imaginary line a little further you will find the bright bluish white star Spica, in the constellation of Virgo.

Right now, Saturn should be an easy target to spot with the naked eye, but looks great through binoculars and is truly amazing through any telescope.

Global Lunar Week – April 10 to 16, 2011

Lunar Week Logo Courtesy of Astronomers Without Borders

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In 2009, hundreds of thousands of people participated in one way or another with the International Year of Astronomy, and there’s no reason to let the excitement die! Astronomers Without Borders are celebrating the entire month of April as Global Astronomy Month and one of the focus points is just three days from arrival… Global Lunar Week!

” A week-long series of programs, from April 10 through 16, will be dedicated to the Moon during Global Astronomy Month to help people rediscover our closest companion in space.” says AWB. “Lunar Week takes place while the Moon is well-placed for observation in the evening sky. As the Moon’s phases and positions change during its orbit around the Earth, there will be Moon-themed star parties to observe the Moon by telescope and naked eye, educational programs, online observing events, competitions and a celebration of the Moon in different cultures.”

Astronomers Without Borders has a theme – One People * One Sky. For all of those who read Universe Today, we realize quickly how astonomy can bring together friends from different countries, different cultures and different time zones. Wouldn’t it be wonderful if we could all observe together?

The dream can come true…

Sander Klieverik from AstronomyLive is working with telescopes around the world to celebrate Global Lunar Week and bring the view right to you.

“The week will start with an amazing broadcast from the historic Chamberlin observatory of the Denver university (with the help of Prof. R. Stencel). It will start april 9th between 7-10pm local time (Denver), which is 01-04 GMT April 10th.” says Sander. “Our goal is to get as many telescopes pointed towards the Moon as possible. I hope that there will be a continuous view of the Moon somewhere from the globe the whole week.”

How can you participate? It’s easy! Just tune into the AstronomyLive Website and follow the instructions. “During the Lunar Week, AstronomyLive will host at least two broadcasts, currently scheduled 15th and 16th of April.” instructs Klieverik. “The first broadcast will take you on a journey across the 85% illuminated lunar surface, on the hunt for the most beautiful craters during this phase, the ´Crater hunt´. The craters at the terminator will receive special attention, the dark side of the moon that changes during the Moon phase. Please know that you will see a LIVE view of the Moon and not some Moon photo. The same accounts for the “Apollo Hop”.

Come one, come all… Lunatics are welcome!

Real-time Observatory Captures Stunning Recent Auroras

An image of the Aurora Borealis above Yellowknife, Northwest Territories, Canada, taken at 00:51 MDT on April 7, 2011. Credit: AuroraMAX

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The online observatory AuroraMAX, which offers live-streaming views of Canada’s northern lights, has seen an uptick in recent aurora activity, and the latest images the team has released are nothing short of stunning. The image above was taken early this morning, April 7, 2011. AuroraMAX is monitoring the intensity and frequency of the Aurora Borealis above their cameras in Canada in the years leading up to Solar Maximum, expected in 2013. In addition to nightly broadcasts of the aurora, AuroraMAX is helping demystify the science behind the phenomenon, as well as providing tips for seeing and photographing auroras.

See below for more recent views.

The Aurora Borealis above Yellowknife, Northwest Territories, Canada, taken at 00:25 MDT on April 5, 2011. Credit: AuroraMAX
The Aurora Borealis above Yellowknife, Northwest Territories, Canada, taken at 01:11 MDT on April 4, 2011 Credit: AuroraMAX
The Aurora Borealis above Yellowknife, Northwest Territories, Canada, taken at 03:10 MDT on March 31, 2011 Credit: AuroraMAX

Click each image to access AuroraMAX’s Twitpic page, where they frequently post images from their nightly observations.

And check out the AuroraMAX website for more information on how you can watch nightly webcasts of aurora activity.

Now is the Time for Observing Saturn in the Night Sky

A current view of Saturn (middle) and also at opositions from the last six years from present (left) clockwise to bottom left. Credit: Efrain Morales Rivera, Jaicoa Observatory, Aguadilla, Puerto Rico.

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April is Global Astronomy Month, and as a highlight, the “Lord of the Rings” is back prominently in the night sky! This past weekend, Saturn reached opposition, when it is closest to the Earth in its orbit. Opposition means Saturn is directly opposite the Sun in the sky, so it rises in the east at sunset and sets in the west at sunrise – meaning it will be in the sky all night long! Saturn is also the only planet visible before midnight in April. But the beautiful ringed planet will be looking even brighter that it has been for the past few months.

Special thanks to Efrain Morales Rivera for sending us this montage of Saturn images, showing a current view of Saturn in the middle and the ringed planet at oppositions from the last six years.

Around opposition there is a phenomenon known as the Seeliger Effect, which might actually be a couple of different effects combining to enhance the brightness of Saturn: Since the Earth is smack dab in the middle of the Sun and Saturn, sunlight is coming from directly behind us and directly at Saturn. And there’s also the phenomenon called coherent backscattering, which is where if you shine a beam of light at something that is made from a lot of separate particles (like Saturn’s rings) the light is reflected back with greater intensity from the direction directly opposite the beam. The middle image of Saturn in the montage above reveals brighter rings from the Seeliger Effect, as well as highlighting the ‘Serpent storm’ in the northern hemisphere.

You can read more about the Seeliger Effect on AstroBob’s website.

This is also a great time to try and see some of Saturn’s moons, too.

Astronomers Without Borders are sponsoring a special Saturn Watch event April 11-16. See their website for more information about “Saturn Watch” and activity suggestions.

Here are more Saturn resources.

There are also several other fun observing events for Global Astronomy Month:

On April 9 the Global Star Party will unfold as darkness sweeps around the Earth. This is the night to set up your telescopes and share the wonders of the sky with others.

From April 10 to 16 it’s Lunar Week, to turn your gaze turns toward Earth’s natural satellite, and take a close-up look the Moon’s craters and “seas”.

April 12th is Yuri’s Night — and a very special one too, as it is the 50th anniversary of the first human in space.


April 17 is SunDay, highlighting our very own star.

The month closes with the Lyrid Meteor shower. On April 21/22 get comfortable in something warm and spend
the night scanning the sky for meteors caused by debris left behind by Comet Thatcher.

See more on the Global Astronomy Month website.

You can hear a podcast about Dark Skies Month on the April 5th 365 Days of Astronomy podcast.

Kickstarting the Joy of Astronomy

Sidewalk astronomy back in 1921 in New York City. Credit: Wikipedia

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You’re probably familiar with Sidewalk Astronomy – where amateur astronomers set up telescopes on street corners or other public places to share free views through a telescope with those who might not otherwise have the chance. These are great opportunities for public education about astronomy and the Universe in which we live. We just got a note from a long-time sidewalk astronomer, Jay Horowitz, who has a plan to set up telescopes on A LOT of street corners. He wants to share telescope views of the skies with people all over the US. But he needs a little help to make his plan come to fruition.


“ I want to give thousands of people the opportunity to see firsthand the universe in which we live, turning young minds on to the power of science and sparking curiosity and awe in adults,” Jay wrote us in an email. And so, he has set up a Kickstarter page – and you might be familiar with this new “crowd sourcing” way to fund creative projects.

Kickstarter projects are efforts by people to do something they love, something fun, or at least something of worthwhile and of note. But they might not have the funds to do it. Kickstarter is an all-or-nothing funding method where projects must be fully-funded or no money changes hands.

Check out Jay’s Astronomy On The Road Kickstarter project, where his goal is to take science around the country in 2011 and 2012. He’s looking to raise money for a Schmidt-Cassegrain telescope, a solar telescope, and fuel for transporting the telescopes between locations. He and his group will provide free views of the skies in schools, libraries, and on city streets all over the United States.

“The telescopes will always be used for public education and will never be for private use, even down the road,” Jay said.

There are also some notable prizes for those who donate, including lunch with some of the big names in astronomy.

Jay’s Sidewalk Astronomy resume is impressive: he founded a successful sidewalk astronomy group in New York City and also volunteered as a telescope operator and educator at an observatory, and taught astronomy in the Dominican Republic.

Consider donating to this great project. You can also follow the project on Twitter.

Observing Alert – Nova Saggitarii 2011 #2

If you think you’re looking a a star studded field, you’d be right. But take a close look at the full size image done by Joe Brimacombe and you’ll see a faint circle with the latest of sky phenomena in its center – Nova Sagitarii 2011… #2!

According to the latest AAVSO press release done by Elizabeth Waagen, “We have been informed by the Central Bureau for Astronomical Telegrams (Central Bureau Electronic Telegram 2679, Daniel W. E. Green, ed.) that Koichi Nishiyama, Kurume, Japan, and Fujio Kabashima, Miyaki, Japan, report their discovery of a possible nova at magnitude 11.7 on two unfiltered CCD frames taken around March 27.832 UT. They confirmed the object on images taken on March 27.832 UT. After posting on the Central Bureau’s Transient Objects Confirmation Page (TOCP) webpage, the object was given the provisional name PNV J18102135-2305306.

Low resolution spectra taken March 28.725 UT by A. Arai, M. Nagashima, T. Kajikawa, and C. Naka, Koyama Astronomical Observatory, Kyoto Sangyo University, suggest that N Sgr 2011 No. 2 is a classical nova that is reddened by interstellar matter.”

At magnitude 12.5, one tiny star is hard to pick out of a huge field, especially when it’s so close to our galactic center. As Joe said, “It is quite close to the Cat’s Paw and Lagoon Nebulae, so the wide field image is neat even though its only a single 10 minute exposure.” For those of us who would take more than ten minutes just to find it, the celestial coordinates are: R.A. 18:10:21.35 Dec. -23:05:30.6. N Sgr 2011 No. 2 has been entered into VSX and assigned the identifier VSX J181021.3-230530. Finder charts for N Sgr 2011 No. 2 may be plotted by entering the coordinates above in the International Variable Star
Plotter
. Please report observations to the AAVSO International Database
as N SGR 2011 NO. 2.

It might be an early morning adventure, but then… Aren’t the skies always the darkest just before dawn?

Many thanks to Joe Brimacombe and AAVSO for waking us up!

Fancy doing a Messier Marathon this Weekend?

The Messier Catalog
The Messier Catalog Credit: SEDS

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If you are new to astronomy, you may ask “what is a Messier Marathon and how do I do one?”

Basically a Messier Marathon is an all night (Dusk til Dawn) observing session held around mid March/ early April every year, where an observer attempts to see all, or as many of the 110 Messier objects as listed by Charles Messier.

The Messier list includes: Nebulae, Galaxies, Star clusters, Supernovae and many other deep sky objects. All of the objects in the Messier list are observable with small amateur telescopes and many of the objects are observable with binoculars.

The reason why Messier marathons take place from mid March to early April is because this is when all of the objects are visible in one evening. Other times of the year aren’t suitable as some of the objects will be in daylight or below the horizon etc.

You don’t have to be an astronomy ace or a seasoned astronomer to do a Messier marathon, but you will need a good telescope to see all of the objects. You don’t even need to do a full Messier marathon as many people do half marathons and depending on your location, or when you observe, you may not be able to see all 110 objects as there is a very tight window of opportunity and higher latitude observers do lose a couple of objects below the horizon.

Timing is key to enable you to see as many of 110 messier objects as possible. Many astronomers put tables and even star charts on the internet to help observers see as many objects as possible.

Observing starts at dusk and ends after dawn and on average each object gets about 5 minutes of observing time before you have to move onto the next one. There can be a short respite half way through the observing session for food and rest, but this depends on the order and success of the objects you are viewing?

Before starting your night of viewing Charles Messier’s wonders, make sure you have all your equipment ready, are dressed warm as it will get cold, have all your charts and viewing tables ready. It also helps to have a hot drink and something nice to eat.

The best dates this year for doing a Messier Marathon have passed and the sky was drenched with the glow of the full moon, but we still have early April. Good luck.

Charles Messier (26 June 1730 – 12 April 1817) was a French astronomer most notable for publishing an astronomical catalogue consisting of deep sky objects such as nebulae and star clusters that came to be known as the 110 “Messier objects”. The purpose of the catalogue was to help astronomical observers, in particular comet hunters such as himself, distinguish between permanent and transient objects in the sky.

Why are Dobsonian Telescopes a Favorite Among Amateur Astronomers?

Dobsonian Telescope
The Meade 16" LightBridge

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Welcome to the scary and expensive world of buying your first, or replacing your old telescope!

I am asked all the time “What telescope should I buy” or “What telescope do I need to see X with?” Nine times out of ten, I recommend a Dobsonian Telescope.

So what is a Dobsonian telescope and why are they so good? Read on to find out why.

A Dobsonian is simplicity in itself; a simple set of optics on a simple mount. But don’t be fooled by this simplicity. Dobsonian telescopes are incredibly good and are great for amateurs and professional astronomers alike. They are also very economical compared to other telescopes.

The optical part of the telescope or OTA (Optical Tube Assembly) is the same as a Newtonian reflector telescope. It consists of a primary parabolic mirror and a flat secondary mirror in an open ended tube, with a focuser for an eyepiece set on the side. Light enters the tube, reflects off of the primary mirror at the base and is then focused onto the smaller flat secondary mirror and then finally, into an eyepiece. Simple!

Credit Skywatcher.net

The benefit of this type of optical arrangement is the telescopes light gathering ability. The more light gathered, equals more fainter objects to be seen. A light bucket!

Dobsonian/Newtonian telescopes have a big advantage over telescopes with lenses such as refractors and Cassegrain telescopes, as mirrors are a lot cheaper to make than lenses. Plus they can be a lot bigger!

Both Dobsonian and Newtonian telescopes are measured by the size of the diameter of their primary (big) mirror. Dobsonian sizes range from starter scopes of 6 inches up to 30 inches, but common sizes are 8 to 16 inches in diameter. They can be many times larger and less expensive to produce than scopes with lenses.

The second part of a Dobsonian telescope is the mount. As with the optical part the mount is just as simple, if not more so! A basic manual mount which supports the optical tube and can be manually moved by hand in the Altitude (up/down) and Azimuth (left/right) axis.

The mount is usually made from wood or metal with bearings and support for the two axis of movement. More so lately, some manufacturers have put GoTo systems with motors on some Dobsonian mounts. Personally I think it’s a bit over kill for a Dobsonian, as finding objects manually by star hopping or other manual methods helps you learn the sky better and can be fun.

Dobsonian

Resist the urge to spend lots of money on small computerized scopes that will eventually never get used, as they can be too complicated or you may not see much through them apart from the brightest objects such as the Moon. A Dobsonian is a great all-around telescope, and are available in almost all telescope stores. Some people make their own homemade Dobsonian scopes too!

Due to the nature of the Alt-Az mount, Dobsonians are not suitable for long exposure astro imaging. For that you will need an equatorial mount, which will track the stars equatorially. You may have some success with webcam imaging with some of the GoTo Mounts though.

Skywatcher 10 inch Dobsonian Credit sherwoods-photo.com

Dobsonian telescopes are designed to be simple, easy to use and gather as much light as possible. Because of this robust simplicity, they are very economical and popular with astronomers of all levels of ability. My own and most favourite telescope is my Skywatcher 10-inch Dobsonian and I will probably be using it for many more years to come, as it is difficult to beat!

The name of the Dobsonian telescope comes from its creator John Dobson, who combined the simple design of the Newtonian telescope with the Alt-Azimuth mount. He originally made simple homemade scopes from household materials and ground mirrors out of the glass of old ship portholes.

John Dobson is the grandfather of Sidewalk Astronomy and co-founder of the San Francisco Sidewalk Astronomers.

Credit cruxis.com