Observing Archives

December 30, 2011December 24, 2015 by VirtualAstro

Night Sky Guide: January 2012

January Sky Northern Hemisphere Credit: Adrian West

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January brings us striking views of the night skies! You’ll be able to see well known constellations during the long hours of darkness in the Northern hemisphere, with crisp cold skies. This is an ideal time to get out and look at the wonders of the night sky as there is so much to see for the beginner and seasoned astronomer alike.

You will only need your eyes to see most of the things in this simple guide, but some objects are best seen through binoculars or a small telescope.

So what sights are there in the January night sky and when and where can we see them?

Meteor Showers

612993main_quadrantids2_466 — Quadrantid Meteor Credit: nasa.gov

As soon as the month starts we receive a welcome treat in the form of the Quadrantid meteor shower on the evening of the 3^rd/ morning of the 4^th of January.

The Quadrantids can be quite an impressive shower with rates (ZHR) of up to 120 meteors per hour at the showers peak (under perfect conditions) and can sometimes produce rates of up to 200 meteors per hour. The peak is quite narrow lasting only a few hours, with activity either side of the peak being quite weak.

Due to a waxing gibbous moon, the best time to look is after midnight and through the early hours when the moon sets in time for us to see the peak which is 07:20 UT.

The radiant of the Quadrantids (where the meteors radiate from) is in the constellation of Boötes, however many people are mislead in thinking they need to look at the radiant to see the meteors – this is not true. Meteors will come from the radiant, but will appear anywhere in the whole sky at random. You can trace the shooting stars path back to the radiant to confirm if it is a meteor from the meteor shower.

For more information on how to observe and enjoy the Quadrantid meteor shower, visit meteorwatch.org

Planets

Mercury is low down in the southeast before sunrise in the first week of January.

Venus will be shining brightly in the southwest until May and will pass within 1° of Neptune the furthest planet on the 12^thand 13th of January. You can see this through binoculars or a small telescope. On the 26^th Venus and the Moon can be seen together after sunset.

On the 5^th of January, Earth will be at “Perihelion” its closest point to the Sun.

Mars brightens slightly to -0.5 during January and can be found in the tail of Leo; it can be easily spotted with the naked eye. The red Planet is close to the Moon on the night of the 13^th/ 14^th January.

On January 2^nd Jupiter and the Moon will be very close to each other with a separation of only 5° with Jupiter just below the Moon. Jupiter will continue to be one of the brightest objects in the sky this month.

Saturn now lies in the constellation of Virgo and follows after just after Mars in Leo.

Uranus is just barely visible to the naked eye in the constellation of Pisces and can be easily spotted in binoculars or small telescopes throughout the month. The Moon will pass very close to Uranus on the 27^th and will be just 5.5° to the left of the planet.

Moon phases

First Quarter – 1^st and 31^st January
Full Moon – 9^th January
Last Quarter – 16^th January
New Moon – 23^rd January

Constellations

In January the most dominant and one of the best known constellations proudly sits in the south of the sky – Orion the hunter.

Easily distinguishable as a torso of a man with a belt of three stars, a sword, club and shield, Orion acts as the centre piece of the surrounding winter constellations. Orion is viewed upside down in the Northern sky as seen from the Southern hemisphere.

Orion contains some exciting objects and its most famous are the Great Nebula in Orion(M42), which makes up the sword and is easily seen in binoculars or a telescope and bright Betelgeuse, Orion’s bright alpha star (α Orionis). Betelgeuse is a red supergiant many times larger than our Sun; it would engulf everything in our solar system out to the orbit of Jupiter, if the two stars swapped places. Betelgeuse will eventually end its life in a Supernova explosion and some people believe that it may have already exploded and the light hasn’t reached us yet. It would make for a fantastic sight!

The Great Orion Nebula by Patrick Cullis — The Great Orion Nebula. Image Credit: Patrick Cullis

If you draw an imaginary line through the three belt stars of Orion and keep going up and to the right, you will come to a bright orange coloured star – Aldebaran (α Tauri) in the constellation of Taurus.

800px-Pleiades_large — Pleiades Cluster/ Seven Sisters

Taurus depicts a head of a bull with Aldebaran as its eye with a V shape that creates long horns starting from what we call the Hyades cluster, a V shaped open cluster of stars. If you continue to draw a line through the belt stars of Orion, through Aldebaran and keep going, you will eventually get to one of the gems in Taurus – The Pleiades cluster or Seven Sisters (M45) a stunning cluster of blue and extremely luminous stars and from our vantage point on Earth, the most recognisable cluster with the naked eye. A great object to scan with binoculars. A great object to hunt for with a small telescope is the Crab Nebula (M1) near the end of the lower horn of Taurus.

If you go back to our imaginary line drawn through the belt stars of Orion and draw it in the other direction, to left and below, you will come to the very bright star Sirius (α CMa) – The Dog Star in Canis Major. Sirius is the brightest star in the sky and is only 8.6 light years away, it is the closest star visible to the naked eye after the Sun.

Sirius along with Betelgeuse and Procyon (α CMi) in Canis Minor, form an asterism known as the Winter Triangle.

Directly above Orion and the Winter Triangle are the constellations of Gemini (The Twins), with the two bright stars of Castor and Pollux marking their heads and Auriga the charioteer, with its bright alpha star Capella (α Aur). Auriga is host to M36, M37 and M38 which are globular clusters and easily seen through binoculars or small telescope and Gemini plays host to M35.

Only a few of the objects available to see have been mentioned, so get yourself a good map, Planisphere or star atlas and see what other objects you can track down!

November 25, 2011December 24, 2015 by VirtualAstro

Beginner’s Guide To Binoculars

Before you consider buying expensive equipment for viewing the wonders of the night sky, binoculars are one piece of equipment every amateur astronomer should have.

Many beginners to astronomy (especially around the holiday period) are sometimes dead-set on getting a telescope, but many aren’t aware that a good pair of binoculars can outperform many entry level telescopes for a similar cost, or much less.

Binoculars are simplicity in themselves — maintenance free, instantly available for use and very versatile, as they can be used for daytime, or “terrestrial viewing” just as well. It is difficult to say the same for with most telescopes.

Go into any photographic store, or website that sells binoculars and you will be met with literally hundreds of different makes, types and sizes – confusing for the beginner, but with a few pointers it can be easy to choose.

Binoculars comparison1-3-300w — Credit: astronomybinoculars.com

So how do you choose a pair of binoculars that will give good results with astronomy?

When choosing binoculars for astronomy, the only variables you need to think about are size of the optics and weight.

Too small and they won’t be powerful enough or let enough light in; too big and heavy means they are almost impossible to use without a support or tripod. Beginners need to find a pair of binoculars which are just right.

The key is to get as much light into the binoculars as possible without making them too heavy. This will give sharp views and comfort when used.

Size and weight come hand in hand, the more light gathered, the heavier the binoculars will be.

All binoculars are measured or rated by two numbers, for example: 10 X 25 or 15 X 70. The first number is the magnification and the second number is the “objective diameter” which is the diameter of the objective lens and this determines how much light can be gathered to form an image.

593px-Binoculars_description_plate2 — Credit: Halfblue Wikipedia

The second number or objective diameter is the most important one to consider when buying binoculars for astronomy, as you need to gather as much light as possible.

As a rule of thumb, binoculars with an objective diameter of 50mm or more are more suited to astronomy than smaller “terrestrial” binoculars. In many cases a larger objective also gives better eye relief (larger exit pupil) making the binoculars much more comfortable to use.

For the beginner or general user, don’t go too big with the objective diameter as you are also making the binoculars physically larger and heavier. Large binoculars are fantastic, but — again — almost impossible to keep steady without a support or tripod.

Good sizes of binoculars for astronomy start at around or just under 10 X 50 and can go up to 20 X 80, but any larger and they will need to be supported when using them. Some very good supported binoculars have objective diameters of more than 100mm. Theses are fantastic, but not as portable as their smaller counterparts.

Binoculars are one of the most important items a new or seasoned astronomer can buy. They are inexpensive, easy to choose, use and will last a very long time.

Enjoy your new binoculars!

November 9, 2011December 24, 2015 by Nancy Atkinson

Images, Video from Around the World of Asteroid 2005 YU55’s Close Pass

Animation showing Asteroid 2005 YU55 moving across the sky. Each image was a 2-second exposure, taken with the GRAS Observatory, near Mayhill, New Mexico. Credit: Ernesto Guido, Giovanni Sostero and Nick Howes

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A 400-meter-wide asteroid created a lot of “buzz” as it buzzed by Earth, with its closest approach on November 08, 2011 at 23:28 Universal Time (UT). The Near-Earth Asteroid 2005 YU55 passed within 319,000 km (202,000 miles or 0.85 lunar distances, 0.00217 AU) from Earth’s surface. Later, it safely passed our moon at distance of 239,500 km (148,830 miles ). Astronomers from around the world trained their telescopes on this object, hoping to capture images and learn more about this dark space rock.

Above is an animation from the team of Ernesto Guido, Giovanni Sostero and Nick Howes, remotely using the the GRAS Observatory near Mayhill, New Mexico USA with a 0.25-meter telescope, f/3.4 reflector and a CCD camera. The trio said that at the moment of their observing session the asteroid was moving at about 260.07″/min and it was at magnitude ~11. You can see more images and details on their Remanzacco Observatory website. A single image they took is below, along with other observations from various points around the globe, including an infrared image taken with the Keck Observatory.

AsteroidYU55-NIR — This first infrared image of asteroid 2005 YU55 was captured by the Keck II telescope. Credit: William Merline, SWRI / W.M. Keck Observatory

The Keck Observatory hosted a live webcast of their observations of the asteroid, hoping to get infrared images and perhaps a three-dimensional view of the asteroid with one of the world’s largest optical/infrared telescopes. They also hoped to be able to look for moons around the asteroid, as about 20% of asteroids have “moons” orbiting them. Battling delays from fog at the summit of Mauna Kea, they team had to wait until conditions cleared, which unfortunately meant the asteroid was farther away when they were able to take a one-second infrared observation. Principal Investigator Bill Merline said it may take days to process this raw data, so look for a more refined image from the team soon. The webcast was a lot of fun, as they showed the events going on insides the observing rooms on both the summit and Waimea, and answered questions from viewers.

This video above is from Jason Ware from Plano, Texas USA who observed Asteroid 2005 YU55 with a 12 inch telescope to create the video.

chumack asteroid 2005 yu55 — Near Earth Asteroid 2005 YU55 on 11-08-2011 07:18pm E.S.T., a 10 second exposure. Credit: John Chumack

John Chumack of Galactic Images in Ohio took this image of the asteroid on 11-08-2011 at 07:18pm E.S.T., a 10 second exposure using a 16″ telescope and a QHY8 CCD. John also created a video, which is available on Flickr.

Peter Lake from Australia, has a telescope in New Mexico. He took a series of images at around 03:00 UTC on Nov. 9, using a 20-inch Planewave with a FLI PL11002M. The image field is 4008 X 2675 pixels and about 0.91 arc secs per pixel, so it passed at about 500 arc sec per minute, Lake said.

This video was taken by Steven Conard at the Willow Oak Observatory in Gamber, Maryland USA, with observations on November 9, 11 with the WOO C-14 telescope. This one has a special bonus–a satellite passes through the field as well.

We’ll add more images and video as they become available. Add your images to our Flickr group and we’ll post them.

Asteroid 2005 YU55’s flyby is the closest approach by an object of this size for the next 16 years. In August 2027, AN 10 is going to come within about one lunar distance from Earth. Astronomers estimate this asteroid is anywhere from 1/2 to 2 kilometers in diameter.

Just six months later, 2001 WN5, a 700-meter-wide asteroid will fly between the Earth and the Moon in June 2028, followed by Apophis on April 13, 2029.

October 18, 2011January 14, 2016 by Nancy Atkinson

All-Sky Camera Captures Mysterious Flashes

Every couple of weeks or so a strange flash appears on an all-sky camera that searches for meteors. What could it be? Take a look at the video above and maybe you can help solve the mystery.

“They are not iridium flares because they are stationary,” said James Beauchamp, an amateur astronomer who hosts the meteor camera for Sandia National Labs and New Mexico State University, and who posted this video on You Tube. “And they are not geosynchronous satellites because the azimuth/elevation are too far North. They are reflective because they always happen just prior to or after sunrise/sunset. Whatever it is, it’s slow and BIG.”
Continue reading “All-Sky Camera Captures Mysterious Flashes”

September 27, 2011December 24, 2015 by VirtualAstro

An Easy Guide To Observing the Aurora

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With the recent solar activity and the high possibility of more coming up, here is an easy guide to observing the aurora. An aurora is a natural light display high in the Earth’s atmosphere, caused by energetic particles from the Sun, colliding with the Earth’s magnetic field.

These light displays are called the Aurora Borealis in the Northern hemisphere and Aurora Australis in the Southern hemisphere, but are commonly known as the Northern and Southern lights.

Viewing aurorae is incredibly simple, but the conditions need to be right for a display to appear.

Normally you can only see aurorae near the poles, such as in Canada, Iceland, and Norway or southern Australia and Antarctica, but when the Sun is highly active, more solar material is thrown in Earth’s direction, creating powerful geomagnetic storms. These storms can bring auroral displays further south to areas such as Southern UK and North to mid latitudes of the USA.

The intensity scale is known as the Planetary KP index and basically the higher the KP number the further south Aurorae can be seen, KP 8 or higher can be good for observers further south. To find out what current levels are check spaceweather.com or the Geophysical Institute at the University of Alaska Fairbanks

If aurora activity is predicted to be high and there is a possibility of seeing it at your location, try and find an area away from light pollution or bright lights and let your eyes adjust to the dark. This may require you to travel into the countryside to escape bright city light pollution.

The best time to spot aurora is around local midnight, but this can change depending on viewing conditions and the current intensity of the magnetic storm.

Once you are comfortable and your eyes have adjusted to the dark, face north (or south in the Southern Hemisphere).

You do not need binoculars, a telescope, or any other optical aid other than glasses if you wear them.

Look low and close to the horizon and look for the faint green/ reddish glow of aurora. It may be quite difficult to see at first, but if it is a powerful display it can be very easy to spot.

I live in the South of the UK and have seen the waving bands and curtain like structures quite easily in powerful geomagnetic storms.

If you have a camera that takes long exposures, use a tripod and try to image the aurora and send us your results.

Most of all, enjoy the show! Good luck!

Aurora caught over Karlstad, Sweden on September 27, 2011. Credit: Socrates2013 on Flickr

Aurora September 26, 2011 From Acadia National Park Credit: hale_bopp37

Aurora Behind the Clouds Credit: Corinne Mills

September 20, 2011December 24, 2015 by Nancy Atkinson

Must See Video: Falling NASA UARS Satellite Observed While Still in Orbit

Several views of the UARS satellite in orbit, as seen from the ground with a 14" telescope. Credit: Thierry Legault Emmanual Rietsch

The huge Upper Atmosphere Research Satellite (UARS) will be plummeting to Earth in an uncontrolled re-entry this week, but here’s an incredible video from astrophotographer extraordinaire Thierry Legault who shot footage of UARS with his 14-inch telescope. Legault was in Northern France (Dunkerque) last week to attempt to capture views of the satellite, and had success on September 15, 2011 between 04:42:14 and 04:44:02 UTC, just 8-9 days before its atmospheric reentry, when it was at an altitude of only 250 km. The tumbling, uncontrolled nature of the satellite is obvious in this video, and various components are visible, such as the body itself and the solar arrays.

NASA has now refined its prediction for when this bus-sized satellite will fall to Earth. The 20-year-old defunct satellite now has a predicted re-entry Time of about 20:36 UTC on September 23, 2011, plus or minus 20 hours, according the the UARS Reentry Twitter feed. So, heads up!

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This is a day earlier than previously anticipated. Pieces of the 6.5-ton satellite are expected to survive the fiery plunge and hit our planet, but NASA does not know exactly where. There was word today that increased activity from the Sun has hastened the decay of the satellite’s orbit.

Legault said his images show the satellite at a 316 km distance to the observer. The angular speed at culmination: 1.36°/s. The speed of the sequence is accelerated two times with regard to real time (20 fps vs 10 fps). The satellite is tumbling, perhaps because of a collision with satellite debris a few years ago.

Here is the equipment Legault used: Celestron EdgeHD 14” Schmidt-Cassegrain telescope (at a focal length of 8500mm) on automatic tracking system, as described on this page. Camera: Lumenera Skynyx L2-2.

Thanks to Legault for sharing his video and images with Universe Today! See more info at Legault’s website.

Map of the UARS orbital path. Credit: @UARS_Reentry Twitter feed.

NASA says there are about 26 components that are big enough to survive and make it down to Earth, the largest weighing more than 150 kg (330 pounds.)

What are you chances of getting hit by debris? Nick Johnson, chief scientist with NASA’s Orbital Debris Program, said that numerically, it comes out to a chance of 1 in 3,200 that any one person anywhere in the world might be struck by a piece of debris. That might sound high, but if you factor in that there are 7 billion people on Earth and that a large part of Earth is covered by water, the liklihood is actually very small. The chance that any one person on Earth getting hit by debris has been estimated at about 1 in 21 trillion.

We’ll provide more updates on the UARS story. For those who would like to catch a last glimpse of UARS streaking across the night sky for yourself should check Heaven’s Above or SpaceWeather’s Satellite Tracker for flyby times in your area.

For more information about this satellite’s uncontrolled re-entry, see our earlier article detailing UARS.

September 2, 2011January 14, 2016 by Nancy Atkinson

How to See a Supernova From Your Backyard This Weekend

The timing couldn’t be better. A new supernova, named PTF11kly, which was discovered on August. 24, 2011 is continuing to brighten and should be visible to backyard astronomers this weekend using just a pair of binoculars. It’s not quite naked-eye material but this is an exciting opportunity for amateurs (as well as the pros!) to view a supernova first-hand. Of course, if your backyard is full of light, the best option is to go to an area with darker skies, and you’ll be able to see it much better. Astronomers say PTF11kly will likely continue to shine for some time, and be at its brightest on about Sept. 9, 2011.

In this video Peter Nugent, an astrophysicist from Lawrence Berkeley National Labs explains just how to find this star that exploded about 21 million light years away.

August 11, 2011December 24, 2015 by VirtualAstro

How To Enjoy The 2011 Perseid Meteor Shower

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It’s time for the Perseid Meteor Shower and you want to bag some meteors (shooting stars), but how? Maybe you just want to know where and what time to look, or perhaps you are having a Perseid party and you want everyone to have a great time.

If so, then please read on…

First, you don’t need a telescope or binoculars or any high tech equipment. You just need your own eyes and glasses if you wear them.

It’s a good idea to be away from bright lights and if possible have a red light torch or red flashlight, but most importantly try to get your eyes adapted to the dark.

Bright light will instantaneously ruin dark adaption so shining flashlights into faces is a big no-no and looking directly at the Moon isn’t going to help either. Position yourself so you don’t get the Moon in your view.

The Perseids don’t rain down out of the sky; they appear every few minutes and this year, you may only see the rarer bright ones and very bright fireballs due to the full Moon that will be up, and the glare it will unfortunately provide. But if you can get in a good position to avoid the glare, sit back and wait to see some meteors. This is totally worth the wait, but you need to be comfortable or you will give up, go indoors and not see any.

The best bet is to get a reclining garden chair or airbed or something similar to lay back and relax upon. Lots of people put those yard trampolines to very good use and use them as meteor observing platforms.

Dress warmly and cover yourself with blankets or a sleeping bag, August is a summer month, but it can get quite chilly at 1:00am and this will make you give up early too, so stay warm.

Have plenty of drinks and snacks ready so you can basically camp out and not have to keep on getting up, or doing things, because this is when you will, ironically, miss the best fireball of the evening.

Fireball Meteor — Perseid fireball. Image Credit: Pierre Martin of Arnprior, Ontario, Canada.

Where do I look and what direction?

This is the most common question I hear people ask about meteor showers and the answer is very simple.

Follow the above comfort guidelines, look up and away from the Moon and fill your gaze with the sky.

Perseid meteors originate from a fixed point in the sky called the radiant, which is in the constellation of Perseus, however meteors will appear in any part of the sky. You can trace their paths back to the radiant.

After midnight, look towards the East/Northeast part of the your sky to find Perseus. To find it look for the easily identifiable constellation Cassiopeia, the big “W” in sky! Perseus is just below Cassiopeia.

You can draw, take pictures and even video the Perseids, but the simplest and most enjoyable thing is to lay back, relax and be patient and you will be rewarded with a great a view.

The best times to look will be in the dark pre-dawn sky on August 11, 12 and 13, 2011.

You can also follow along with Universe Today and Meteorwatch.org with #meteorwatch on twitter. Ask questions, see what others are seeing, share your experiences and images using the hashtag #meteorwatch

Most of all, enjoy your Perseid experience and have fun!

August 11, 2011December 24, 2015 by VirtualAstro

The Perseids: Why is There a Meteor Shower?

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Every year from late July to mid-August, the Earth encounters a trail of debris left behind from the tail of a comet named Swift-Tuttle. This isn’t the only trail of debris the Earth encounters throughout the year, but it might be one of the most notorious as it is responsible for the annual Perseid meteor shower, one of the best and well-known yearly meteor showers.

Comet Swift-Tuttle is a very long way away from us right now, but when it last visited this part of the Solar system, it left behind a stream of debris made up of particles of dust and rock from the comet’s tail.

Earth encounters this debris field for a few weeks, reaching the densest part on the 11th to 13th August.

The tiny specs of dust and rock collide with the Earth’s atmosphere, entering at speeds ranging from 11 km/sec (25,000 mph), to 72 km/sec (160,000 mph). They are instantly vaporised, emitting bright streaks of light. These tiny particles are referred to as meteors or for the more romantic, shooting stars.

The reason the meteor shower is called the Perseid, is because the point of the sky or radiant where the meteors appear to originate from is in the constellation of Perseus, hence Perseid.

When the Perseid meteor shower reaches its peak, up to 100 meteors an hour can be seen under ideal dark sky conditions, but in 2011 this will be greatly reduced due to a full Moon at this time. Many of the fainter meteors (shooting stars) will be lost to the glare of the Moon, but do not despair as some Perseids are bright fireballs made from larger pieces of debris, that can be golf ball size or larger.

These amazingly bright meteors can last for a few seconds and can be the brightest thing in the sky. They are very dramatic and beautiful, and seeing one can be the highlight of your Perseid observing experience.

So while expectations may be low for the Perseids this year, keep an eye out for the bright ones and the fireballs. You will not be disappointed, even if you only see one!

Join in on twitter with a worldwide event with Universe Today and Meteorwatch.org just follow along using the hashtag #meteorwatch ask questions, post images, enjoy and share your Perseid Meteor Shower experience.

July 1, 2011December 24, 2015 by Nancy Atkinson

Stunning Noctilucent Clouds Shine Brightly in the UK

Panoramic view of Noctulucent Clouds from Kendal Castle in the UK. Credit: Stu Atkinson

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Mysterious “night shining” or Noctilucent Clouds are beautiful to behold, and here are some gorgeous examples what skywatchers in the UK have been experiencing. Stu Atkinson took this stunning panoramic view from Kendal Castle. (Click image for access to a larger version). NLCs are usually seen during the summertime, appearing at sunset. They are thin, wavy ice clouds that form at very high altitudes and reflect sunlight long after the Sun has dropped below the horizon. Scientists don’t know exactly why they form, and they seem to be appearing more and more in recent times.

See more below.

Science writer Will Gater also had a great view of NLCs this morning. Click the image to see his animation, or see more of his images and animations at his website post.

NLCs seen over the UK on July 1, 2011. Click to see animation. Credit: Will Gater. — NLCs seen over the UK on July 1, 2011. Click to see animation. Credit: Will Gater

Another view of Noctilucent Clouds from Kendal Castle in the UK on July 1, 2011. Credit: Stu Atkinson

See more from Stu Atkinson at his Cumbrian Sky website.