Tuesday 26 June 2012

Look out for Noctilucent Clouds


Night clouds or noctilucent clouds are tenuous cloud-like phenomena, visible in a deep twilight. They are made of crystals of water ice. They are most commonly observed in the summer months at latitudes between 50° and 70° north and south of the equator. They can only be observed when the Sun is below the horizon.

We are in the right place, at the right time to observe them this summer. Keep watching the skies.


They are the highest clouds in the Earth's atmosphere, located in the mesosphere at altitudes of around 76 to 85 kilometres. They are normally too faint to be seen, and are visible only when illuminated by sunlight from below the horizon while the lower layers of the atmosphere are in the Earth's shadow. Noctilucent clouds are not fully understood and are a recently-discovered meteorological phenomenon.

Their occurrence can be used as a sensitive guide to changes in the upper atmosphere - increasing frequency, brightness and extent is possibly connected to climate change.

Exoplanets


Extrasolar planets - exoplanets - orbit a star other than the Sun. They are too faint to be seen directly with existing instrumenets, so indirect methods of detection are necessary. The first exoplanet was only discovered in 1992. It orbits a pulsar.

There are three methods for discovering exoplanets:
1. The radial velocity method - looks for a cyclical Doppler shift in the light from a star.
2. The transit method - looks for dips in the brightness of a star as the planet crosses the face of the star.
3. Astrometry - accurately measures the wobble of a star as a planet orbits.

Planet finding spacecraft such as COROT and Kepler use the transit method and to date 786 planets are known.

You can download the free exoplanet app and follow the discoveries. Maybe life is out there waiting for us... THIS IS AN EXCITING TIME indeed.

Wednesday 20 June 2012

Summer solstice


Happy June solstice, everyone! If you’re in the Northern Hemisphere, the June solstice is your signal to celebrate summer. For us, this solstice marks the longest day of the year. Early dawns. Long days. Late sunsets. Short nights. The sun at its height each day, as it crosses the sky. Meanwhile, south of the equator, winter begins.


Planet Earth, as seen from the Sun, at the instant of June 2012 solstice: June 20 at 23:09 Universal Time (12:09 GMT) on the 21st .

What is a solstice? Ancient cultures knew that the Sun’s path across the sky, the length of daylight, and the location of the sunrise and sunset all shifted in a regular way throughout the year.

They built monuments, such as Stonehenge, to follow the sun’s yearly progress.

Today, we know that the solstice is an astronomical event, caused by Earth’s tilt on its axis and its motion in orbit around the sun.

Because Earth doesn’t orbit upright. Instead, our world is tilted on its axis by 23-and-a-half degrees, Earth’s Northern and Southern Hemispheres trade places in receiving the sun’s light and warmth most directly.

At the June solstice, Earth is positioned in its orbit so that our world’s North Pole is leaning most toward the Sun. As seen from Earth, the Sun is directly overhead at noon 23 1/2 degrees north of the equator, at an imaginary line encircling the globe known as the Tropic of Cancer – named after the constellation Cancer the Crab. This is as far north as the Sun ever gets.

For all of Earth’s creatures, nothing is so fundamental as the length of the day. After all, the Sun is the ultimate source of almost all light and warmth on Earth’s surface.

If you live in the Northern Hemisphere, you might notice the early dawns and late sunsets, and the high arc of the Sun across the sky each day. You might see how high the Sun appears in the sky at local noon. And be sure to look at your noontime shadow. Around the time of the solstice, it’s your shortest noontime shadow of the year.

For us in the modern world, the solstice is a time to recall the reverence and understanding that early people had for the sky. Some 5,000 years ago, people placed huge stones in a circle on a broad plain in what’s now England and aligned them with the June solstice sunrise.

We may never comprehend the full significance of Stonehenge. But we do know that knowledge of this sort wasn’t isolated to just one part of the world. Around the same time Stonehenge was being constructed in England, two great pyramids and then the Sphinx were built on Egyptian sands. If you stood at the Sphinx on the summer solstice and gazed toward the two pyramids, you’d see the sun set exactly between them.

Monday 18 June 2012

Infrared Astronomy

Y10 Astronomers in infrared
Infrared Astronomy is the detection and study of the infrared radiation (heat energy) emitted from objects in the Universe. All objects emit infrared radiation. So, Infrared Astronomy involves the study of just about everything in the Universe.

In the field of astronomy, the infrared region lies within the range of sensitivity of infrared detectors, which is between wavelengths of about 1 and 300 microns (a micron is one millionth of a meter). The human eye detects only 1% of light at 0.69 microns, and 0.01% at 0.75 microns, and so effectively cannot see wavelengths longer than about 0.75 microns unless the light source is extremely bright.

 
Using infrared the familiar can take on a spectacular guise - Y10 astronomers above or the winter sky constellation Orion in the infrared, as seen to the left, in this false-color image constructed from data collected by IRAS--the Infrared Astronomical Satellite.

Thanks to the University of Sussex, Department of Physics and Astronomy for their expertise and technical wizardry, for illustrating the use of infrared in astronomy.

Monday 11 June 2012

Scale of the Universe



How big is the Universe? Explore this website.

Quiz questions:

1. By how many factors of ten is the Local Group larger than a proton?

2. What other comparision could be made of the same scale?


Wednesday 6 June 2012

Awesome multiwavelength images

NASA | SDO's Ultra-high Definition View of 2012 Venus Transit

As I travelled down the motorway (thankfully as a passenger) I failed to glimpse the transit in my eclipse glasses. 4 minutes later the clouds parted and the Sun came out. Too late.

Thankfully NASA saved the day with this awesome video.

From Svalbard Venus transit in K-calcium

Studying the calcium content of the Sun during the transit