Sunday, 1 June 2014

How to Enjoy Your New Telescope: Advice for Beginner Skywatchers

Over the years when I’ve spoken with many other amateur astronomers about their interest in the sky, most have said that it could be traced back to receiving their first telescope at Christmas.
With the winter holidays now behind us, perhaps you fall into this category. If this is the case, then please read this article carefully, for you are now at a very important crossroad. 
While it is true that many have been hooked on skywatching for life by viewing the wonders of the night sky through their first scope, it is also true that many others have had their initial enthusiasm for astronomy severely dampened by their first telescope — particularly if they didn't know how to properly use it, and any initial pleasure soon turns to frustration.
So, now is the appropriate time to talk about how to best take advantage of your new instrument.
Learn your way around
Before anything else, if you have not already done so, I would invest in a couple of good books on the stars and constellations. As the late George Lovi (1939-1993), a longtime columnist of Sky & Telescope magazine, once wrote: "First spend some time learning the sky with your own personal optics — the set nature mounted in your head." [Skywatching Events for February 2012]

Thierry Legault is an amateur astronomer.
Thierry Legault is an amateur astronomer.
Credit: Thierry Legault

If you haven't yet opened the box that contains your telescope, good!  From 45 years of both personal observing and teaching many others, it’s my belief that you should not hastily rush outside with a telescope before even knowing what's in the sky or what to look at. It's not unlike buying a catamaran if you've never sailed before.

When you finally start setting up your telescope, take whatever time is needed to learn its use and operation. Be sure that you have assembled everything with great care. In the beginning, practice how to aim and focus your new instrument, not on the night sky, but on daytime terrestrial objects. Not only are these daytime targets bright and easy to see, but unlike night sky objects, they will not drift out of your field of view because of the rotation of the Earth.

Was your new instrument advertised by the manufacturer as promising "spectacular views" of the moon or the rings of Saturn at magnifications of, say, 500-power or more? Unfortunately, too many uninitiated amateurs are "power happy" (can we call this malady "poweritis?"). High power dilutes the brightness of an image, as well as aggravates any unsteadiness of detail. [Video: Types of Telescopes - Which is Right for You?]

So, always remember as a general rule of thumb: the maximum amount of magnification for any telescope is 50-power per inch of aperture. If you have, for example, a 6-inch reflector, 300-power is as high as you should ever attempt to go; the maximum for a 3-inch refractor should be 150-power. 
"But wait a minute," you may protest, "my telescope comes with a special Barlow lens, that the manufacturer promises will double or even triple the magnification of my eyepiece."
True enough. In fact, the aforementioned 500-power is likely achieved by pushing the scope's highest power eyepiece with that very same Barlow lens (a diverging lens named for its creator, the English engineer Peter Barlow), which ultimately will result in a dim, impossibly fuzzy image.

A little lesson about power
If you’re a beginner, you need to understand that using a Barlow lens is similar to enlarging a photograph.  The negative — like a telescope's image — contains only so much detail, which can be blown up only so far before all you can see is fuzz!
So, if you have purchased a 3-inch telescope — even if it is blessed with perfect optics — the claim of 500-power is more than three times the limit of the most practical magnification that it can provide.
Truth be told, you'll probably be surprised to discover that your most pleasing views with your new instrument will come at much lower powers. Low power, in fact, makes a telescope much more convenient to handle, and if your telescope mount or tripod is a bit shaky, as least lower powers will not magnify "the shakes" as much.

Personally, I’ve always felt that the most pleasing views with your scope will come at one-half of its maximum possible magnification. So, for that 6-inch telescope, use 150-power, and for a 3-inch telescope, try 75-power.

One other thing that should be mentioned is in regard to solar viewing. Some department store telescopes — especially imported varieties — may include a dark glass that is designed to screw into the eyepiece of the scope.
Supposedly, this filter is to be used to view the sun. If your telescope came with such a device, discard it immediately!

Unfortunately, by directing your telescope toward the sun its light and heat are intensified tremendously when it reaches your eyepiece. As such, there is an ongoing threat that the dark glass will be heated to a point where it will suddenly crack. Should your eye be looking through the eyepiece at the time, you likely will not have enough time to turn away. The end result can be partialor total blindness. Never, ever, look directly at the sun at any time with your telescope. [10 Most Popular Skywatching Misconceptions Explained]
If you do wish to observe the sun, the only way to go is to project its enlarged image onto a white card or screen.  
What’s up there?
Jupiter, Venus & Moon Sky Map February 26, 2012
On February 26, 2012, the Moon will be close to the planets Venus and Jupiter.
Credit: Starry Night Software
So what is there to see? Probably the most rewarding object is the moon. It is bright, easy to locate and filled with fascinating detail.
Despite its tremendous brilliance, Venus is a bit of a disappointment right now as it will appear as merely a brilliant blob of light. That will change in the coming weeks as it grows in size and will mimic the changing phases of the moon, appearing half illuminated late in March and then as a thinning crescent during April and May.

Jupiter is high and dazzling in the southern sky at nightfall and is unmistakable; its four bright moons are a constantly changing target even in binoculars.
Another target is Mars, appearing as a brilliant fiery-colored star in the eastern sky during the mid-to-late evening hours and is now approaching Earth and getting increasingly brighter with each passing night.

Rising in the east-southeast sky soon after midnight is the planet Saturn (whose famous rings can be recognized with a magnification as low as 30-power).
The brilliant starry scene in the southern sky during the early evening hours contains innumerable treats, including the Pleiades and Hyades Star Clusters and the Great Nebula of Orion. Indeed, there’s an entire universe of stars — double, multiple and all highly beautiful — as well as other nebulas and galaxies for you to explore. The choices are virtually inexhaustible.
Welcome to the club!
And as a final piece of advice, make an effort to contact a local astronomy club. You can probably locate the one nearest to you by visiting the website of the Astronomical League (AL) and clicking on "Member Societies." The AL, which is by far the largest national organization of amateur astronomers, is composed of scores of local amateur astronomical clubs and groups, totaling thousands of individuals.

By attending local club meetings, you'll get to meet a number of fellow sky gazers who can offer you valuable advice. If you own a telescope, but are experiencing problems with it, there is no better place to go than an astronomy club, whose members can offer assistance and helpful suggestions. Besides, you'll also find camaraderie and the opportunity to spend time with other people from different walks of life who all share the same love for the nighttime sky.
So, good luck and enjoy your new telescope!
Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for The New York Times and other publications, and he is also an on-camera meteorologist for News 12 Westchester, N.Y.

Friday, 9 May 2014

May is prime time for observing Saturn and rings

There is no finer sight in the night sky than the beautiful ringed
planet Saturn in the eyepiece. The gas giant comes to opposition -- the
planet directly opposite the Sun -- among the stars of Libra on 10 May,
when it's 1,331 million kilometres from Earth and observable for much of
the night.






Where to find Saturn, over the southern horizon in Libra, on opposition on 10 May. Astronomy Now graphic by Greg Smye-Rumsby.



Saturn shines like a bright star with a noticeably yellow-hue at
magnitude +0.1, brighter than nearby, white Spica in neighbouring Virgo
and a small telescope will easily show Saturn's crowning glory, its
unique major ring system and the giant moon Titan.



Saturn is the second largest planet with an equatorial diameter
of 120,536 kilometres (if we count the rings, from one tip of the A-ring
to the other, this extends to 274,000 kilometres) with an average
distance from the Sun of 1.4 billion kilometres (9.58 astronomical
units). Saturn is the most oblate of the planets with its polar diameter
(107,566 kilometres) 90 percent that of its equatorial diameter, giving
it an even more flattened appearance than Jupiter.



The ringed planet takes 29.4 years to complete one orbit around
our star, moving 12.2 degrees eastwards along the ecliptic each year.
This year observers in the Southern Hemisphere are favoured with Saturn
lying among the stars of Libra at a southerly declination of 15 degrees.




This has not been an easy apparition for Saturn observers as it
lies well south of the celestial equator. This means Saturn is never
more than 25 degrees above the southern horizon at best from the UK and
the period when it's pulled sufficiently clear of local horizons to
limit the turbulence is limited to around three and a half hours around
opposition.



However the rewards for seeing Saturn float into your telescope's
field of view or securing those decent frames far outstrip the
inconveniences I've mentioned; if you've never seen Saturn through a
telescope this is your chance and it's a never to be forgotten sight!
You will need a decent south-eastern through to south-western horizon to
make the most of observing the ringed planet.



Saturn rises at 8.15pm BST due east-south-east and takes three
hours to haul itself twenty degrees up, by then lying in the
south-south-east. The sky is just about astronomically dark from London
and the south of England (Sun more than 18 degrees below the horizon) by
this time too. Saturn is at its highest above the southern horizon (24
degrees) at 1am and remains above 20 degrees altitude until 3am, setting
at 5.45am. Saturn remains well placed through the rest of May and it's
not until late September that it starts to become difficult to observe.



Observing Saturn



Saturn is a gas giant like Jupiter so there is no solid surface
to speak of; the face we see is the top of its tumultuous atmosphere.
Apart from the magnificent rings the planet's most striking feature is
its flattened shape, its oblateness.






This
portrait looking down on Saturn and its rings was created from images
obtained by NASA's Cassini spacecraft on Oct. 10, 2013. It was made by
amateur image processor and Cassini fan Gordan Ugarkovic. Credit:
NASA/JPL-Caltech/Space Science Institute/G. Ugarkovic.




Saturn rotates on its axis every 10 hours and 14 minutes, and although
marginally slower than Jupiter, this rapid spin coupled to its lower
density (it would float if there were an ocean large enough!) and
gravity causes the obvious equatorial bulge. It does have belts and
zones but they are much less pronounced than on Jupiter and require
generally telescopes in the 150-200mm range to see well.



Astronomy Now's Peter Grego reports that the North Equatorial
Belt is nicely presented, appearing very broad and is more sharply
delineated on its southern margin where it meet the brighter Equatorial
Zone. Colour filters will make it easier to see more subtle features on
the globe and the rings; try a light blue filter to increase the
visibility of boundaries between belts and zones and a red or orange
filter to to make the belts darker. Saturn usually has a number of
low-contrast spots and projections and a light magenta filter can help
here. Advanced CCD imagers embracing the marvellous camera technology
and image processing techniques now available are brilliantly placed to
capture any short-lived atmospheric phenomena, despite Saturn's less
than generous placing in Northern Europe.



Wondrous rings



Saturn's rings are beautiful and unique are appearing to 'open
out' since appearing to be edge-on to us in 2009. At opposition the
northern side of the rings faces us at a tilt of 21.7 degrees. A small
telescope is needed to see the rings but through mounted binoculars
Saturn's elongated shape is apparent.






The Seeliger Effect will cause Saturn's rings to brighten on opposition night.



A good quality 60-80-mm refractor will easily show the brighter and
larger inner B-ring, the outer A-ring and the Cassini Division between
them in the 'ansae', the broadest part of the ring. The Encke Gap in the
outer part A-ring can be snared through a 100-mm (four-inch) apochromat
or a 150-mm (six-inch) Newtonian. The dusty inner C or Crepe ring is
semi-translucent and very hard to see even through large amateur
telescopes. As the rings open out the C-ring becomes easier to see; try a
200-mm 'scope under good conditions and perhaps a violet-blue filter.



There are a number of notable changes to Saturn's 'normal'
appearance either side of opposition that the experienced Saturn
observer is familiar with but can be readily viewed by a beginner. The
shadow of Saturn's globe can usually be seen through a small telescope;
before opposition appearing on the far side of the rings to the west of
the planet. Those observers who have been keeping Saturn under
observation these past few months will have noticed this shadow getting
ever-smaller. At opposition the shadow is almost completely hidden as
Saturn is being fully illuminated by the Sun and we are in line. After
opposition the shadow will fall to on the rings far side again, but this
time ever-widening to the east of Saturn's globe.



A really startling effect occurs right at opposition, when the
rings very noticeably brighten visually and in images. This is the
Seeliger Effect caused by the tiny ring particles being lit full on. The
phase angle, defined as the angle between the observer, the observed
object and the source of light (the Sun), is zero causing the shadows
normally cast to disappear and a temporary brightening occurring.

Astronomy for Beginners - Getting Started Stargazing!