Meteor Shower ABC

•May 2, 2008 • 5 Comments

A meteoroid is a solid object – usually are dust particles or debris from comets – that floats around in space.

When meteoroid enters and burns in the Earth’s atmosphere, the visible streak in the sky is known as a meteor.

A meteorite is the meteoroid that survives and reaches Earth’s surface.

An increase in the number of meteors at a particular time is called a meteor shower.

If we trace back the path of the meteors during a meteor shower, we will find that all the meteors seem to originate from a point in the sky. This point is known as the radiant.

Zenith Hourly Rate (ZHR) of a meteor shower is the number of meteor an observer would see in an hour under a dark sky with limiting magnitude of 6.5 and if the radiant was in the zenith. In reality the rate which can effectively be seen is always lower as the radiant is closer to the horizon and it also depends on the local weather condition.

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Meteors appear as fast-moving streaks of light in the night sky that usually will only last about a second or two. They are commonly referred to as “falling stars” or “shooting stars”.  Sometimes meteor may even leave a trail behind.

The vast outer space is actually not empty as it seems to be; there are a lot of dust particles, tiny grains of sand and ice floating around in space. When these particles or meteoroids come too close to Earth, Earth’s gravity will pull them into the atmosphere, at a speed of 10 to 70 kilometres per second, to produce streaks of light in the night sky known as meteors.

Most meteors will completely burn up in the atmosphere at an altitude of 100 kilometres.  However, some bigger chunk of meteoroids may survive the trip through the atmosphere and reach the ground. These remnants are known as meteorites.

 

What is Meteor Shower?

On a normal night we can typically see a few meteors per hour. This type of meteors is called the sporadic meteors. However, at certain times of the year the rate of observable meteors is much higher. These periods are called meteor showers.

Most meteor showers have their origins with comets. Comets are primarily composed of ice and dust and when they approach the Earth, the Sun’s heat will evaporate the ice and they will shed an icy, dusty debris stream which is then distributed along their orbits. When our Earth passes through a comet’s orbit, these left-over comet debris will “bombards” Earth and causes the rate of meteors increases.

Due to Earth orbit around the Sun, we will roughly be at the same location in space every year. Hence meteor showers will occur almost the same time each year when Earth crosses the comet’s orbit. The different between the yearly showers is related to how close the comet’s orbit to ours and how long ago the debris was ejected.

 

Why is Meteor Shower named after Constellation?

During a meteor shower, if we observe carefully, we will find that the path of the meteors seem to radiate from a point in the sky. This point is called the radiant of the meteor shower and is just a perspective effect. Actually all the meteors enter the Earth’s atmosphere in a parallel path, but from our Earth perspective, the meteors appear to come from the radiant.  This is just the same as parallel railway tracks seem to converge to a point far far away.

Meteor shower is named based on the location of their radiant. For example, if the radiant is located in constellation Perseus, the particular meteor shower is known as the Perseids. If there is more than one meteor shower in a constellation, then the shower is named after the bright star nearest to the radiant. For example, the Eta Aquarids and Delta Aquarids meteor shower are both from the constellation Aquarius.

 

How to observe Meteor Shower?

All you need to enjoy a meteor shower is just your naked eyes. No equipment is needed!

To observed, find a group of at least 5 people, go to a SAFE, dark and unobstructed site, away from city light or any man-made light polluter. The darker the site, the more dimmer meteors is going to be visible (although in the end the number of meteor visible is strongly dependent on the weather).

Although the meteors are said to come from the radiant, meteors actually can be seen all over the night sky, not just only in the direction of the constellation. It is just that when you trace back the route of the meteors, they seem to converage to a point, i.e. the radiant. So, don’t stare right at the radiant; you surely will miss out a lot of meteors over your head.

To make yourself comfortable, bring along mat to lie down. Lying down flat on the ground is the best position so that we can cover the maximum area of the sky. This position is a bit “dangerous” though, because this is also the best position to fall asleep and the next thing you know might be the Sun rising. Try chit-chatting with friends, this will help to keep you awake, but make sure that your eyes are glue to the sky; you won’t want to miss the show.

Sometime it may be cold in the middle of the night, so a jacket may come in handy. Better still if you can prepare some food and drinks to fill up your empty stomach during the night. Mosquito repellent may also be something useful to bring along.

Summary:

  • Find a dark, safe and unobstructed observing site.
  • Bring along star chart, red-light torchlight, food & drinks, jacket, ground-mat or sleeping bag.
  • When you reach the observing site, find a place that is not easily disturbed by others.
  • Check your direction and use the star chart to find the location of the radiant in the sky.
  • Find a comfortable position to sit or lie down while waiting for the meteor to appear. The best position is to lie down flat on the ground so that you will cover the maximum area of the sky.

 

Why there are more Meteors after Midnight?

When Earth orbit around the Sun, basically meteoroids enter the Earth’s atmosphere from all direction. The velocity of Earth around the Sun is about 30 km/s and the meteoroids’ velocity is averagely 40 km/s.

Refer to the diagram, before midnight, the meteors are catching up with Earth from the back, hence the velocity of the meteor will be the different between the Earth’s orbital velocity and the meteoroids’ velocity, which is roughly 10 km/s.

Meteor before & after midnight

After midnight, the meteors are heading straight to Earth, so the velocity now is the total of both the Earth and meteoroids’ velocity, which is equal to 70 km/s.

Hence, before midnight, only those meteoroids moving faster than Earth will catch up, so the amount of meteor seen is lesser. Also, the velocity of the meteor is lower before midnight, so the meteor will be dimmer during this time.

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Click here for handout on Meteor Shower in both English and Chinese. You are welcome to use it as teaching or handout material to the public.

Carnival of Space #52

•May 2, 2008 • Leave a Comment

There is so much space stuff in the internet that sometimes we may get lost trying to look for interesting story. This is where the Carnival of Space comes in.

Carnival of Space is a great way to learn what other people are saying and is where you can find lots of astronomy- and space-related articles that can keep you busy reading for days. Every week, different people will host the carnival at their blog.

And this week, the 1st anniversary of Carnival of Space is back where it started, held at Homeschooling Blog. I have submitted my first entry to the carnival.  Go and have a good read!

If you are interested, this is the archive to all the past carnivals of space.

Ultra-dense Galaxies in the Early Universe

•May 1, 2008 • 1 Comment

In today’s universe, a galaxy about 100,000 light years across containing 200 billion stars is considered typical, something like our Milky Way Galaxy.

But that was not the case for galaxies in the early universe.

Astronomers, using the Hubble Space Telescope and Keck Observatory to study galaxies as they existed 11 billion years ago, found that galaxies are surprisingly compact. The nine compact galaxies that they found, each about the mass of our Galaxy, instead of hundred thousand light years across, are only 5,000 light years across.

MilkyWay & Compact Galaxy

This is a puzzle to astronomers. No massive galaxy at that distance has ever been observed to be so compact. Over the 11 billion years, these baby galaxies must have grown a lot, to about five times bigger than it previously were. They might comprise half of all galaxies of that mass 11 billion years ago, forming the building blocks of today’s largest galaxies.

Ultra-dense Galaxies

These baby galaxies are only a fraction of the size of today’s grown-up galaxies, but contain approximately the same numbers of stars.  Credit: Hubble Space Telescope.

So, how do these ultra-dense galaxies form?

One hypothesis is that the early universe contains pockets of dark matter (an invisible form of matter that accounts for about 23% of the universe’s mass), where hydrogen gas became trapped there. The gas then began spinning rapidly in the dark matter’s gravitational whirlpool, forming stars at a furious rate. The new-formed galaxies would have been very small because they are constrained in the dark matter pockets.

These galaxies are ideal targets for the Wide Field Camera 3, which is scheduled to be installed aboard Hubble during Servicing Mission 4 in the fall of 2008. “We hope to use the Wide Field Camera 3 to find thousands of these galaxies. The Hubble images, together with the laser adaptive optics at Keck and similar large telescopes, should lead to a better understanding of the evolution of galaxies early in the life of the universe,” said Garth Illingworth of the University of California, Santa Cruz, and Lick Observatory.

Source: HubbleSite NewsCentre

Features on Mercury Receive New Names

•April 30, 2008 • 1 Comment

On January 14, 2008, MESSENGER makes its first flyby of Mercury, skimming 200 kilometres above its surface. During that flyby, MESSENGER had imaged the hemisphere that has never been seen before, revealing a lot of unnamed features on its surface.

The International Astronomical Union (IAU), as the internationally recognised authority for assigning designations to surface features on celestial bodies, has approved new names for these new features on Mercury.

To name a feature on planets, moons and asteroids, you have to follow the rules – the naming rules. The craters on Mercury are named after famous deceased artists, musicians, or authors. Mercury’s cliffs are named after the ships of famous explorers.

One set of cliffs discovered by MESSENGER (called by the Latin name for cliffs, rupes) is named Beagle Rupes, after the ship on which naturalist Charles Darwin sailed around the world.

The newly named craters are Apollodorus, Atget, Eminescu, Kertész, Neruda, Raditladi, Sander, Sveinsdóttir, Xiao Zhao. Click here for brief descriptions of these people.

New Names on Mercury. Click for full map

New Names for Features on Mercury.  Click on image for full map. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington.

During this flyby, MESSENGER found a new feature, termed a fossa (plural is fossae) by the IAU. These fossae are fault-bounded troughs or grabens that radiate out from a small area near the centre of the Caloris Basin. The feature was previously nicknamed “the spider” by the science team.

No previous fossae had been discovered on Mercury from the Mariner 10 images, so the IAU had to approve a new naming scheme – “significant works of architecture”. Pantheon Fossae were named after the Pantheon, a still-used second-century Roman temple and later church. The ancient building and the fossae both feature a central circular feature and radiating texture.

MESSENGER will return to Mercury for another flyby in October, then the third one in September 2009 and finally it will return on March 2011 to settle into Mercury’s orbit.

Source: MESSENGER Mission News

International Year of Astronomy 2009 Trailer

•April 29, 2008 • 2 Comments

IYA2009

The United Nations had declares 2009 as the International Year of Astronomy (IYA2009). It will be a global celebration of astronomy and its contributions to society and culture.

Next year will also mark the 400th anniversary since the first human (Galileo Galilei) point a telescope to the sky, which had triggered a scientific revolution which profoundly affected our worldview.

While waiting for the show to start next year, let take a look at the IYA2009 trailer to build up some excitement.

The vision of the International Year of Astronomy 2009 is to help the citizens of the world rediscover their place in the Universe through the day- and night time sky, and thereby engage a personal sense of wonder and discovery.

All humans should realize the impact of astronomy and basic sciences on our daily lives, and understand better how scientific knowledge can contribute to a more equitable and peaceful society. The IYA2009 will highlight global cooperation for peaceful purposes – the search for our cosmic origin and our common heritage which connect all citizens of planet Earth.

Malaysia is also a part of this grand event – Home, Objectives and Approaches.

Proposal to build Universiti Sains Angkasa Lepas in Johor!

•April 28, 2008 • Leave a Comment

A local company, Next Systems Sdn. Bhd., together with its overseas partner plans to build a RM6.1 billion university offering space science courses in Johor, reports Utusan Malaysia yesterday. They have identified a 1000-hectare land near Kota Tinggi for the university, which will be known as Universiti Sains Angkasa Lepas Malaysia (UniSam).

If this was confirm, Malaysia will be the third country with a space science university after Embry Riddle Aeronautical University in Florida and International Space University, Strasbourg, France.

“UniSam will have eight faculties, covering the critical fields in space science researches such as Space and Aeronautic Engineering, Mechanical Engineering, Computer and Robotic Engineering, Geology, Atmospheric and Planetary Engineering, Mathematics, Physics, Astronomy etc.” said Noor Faizal Abdul Samad from Next Systems Sdn. Bhd.

These faculties will have 29 laboratories equipped with cutting edge technologies such as Fusion Reactor, Thermonuclear Reactor, Linear Collider, Large Binocular Telescope-Neural Network Telescope, High Performance Computing (HPC), Supersonic Wind Tunnel and 3D Simulation Laboratory.

Noor Faizal hopes that with these high-tech laboratories and equipment, UniSam will become a resource centre for scientist inside and outside the country.

Source: Utusan Malaysia

Jules Verne Boosts ISS to Higher Orbit

•April 28, 2008 • 1 Comment

The space where the International Space Station (ISS) orbits is not pure vacuum; there is a very thin atmosphere at where it orbits. And because of this thin atmosphere, the Station feels a small amount of friction, which slows it down and making it drop to a lower altitude. The Station’s natural altitude loss can reach up to several hundreds of metres a day.

Lower altitude means thicker atmosphere; thicker atmosphere means more frictions; more frictions means drop faster to even lower altitude and lower altitude means… the process keeps on repeating in a faster and faster rate, until the station will eventually burn itself up in our atmosphere.

To avoid this from happening, once in a while, ISS needs to be pushed to higher altitudes to compensate for this atmospheric drag. Previously, the “boosting” were done by the Space Shuttle, Russian Progress and by the ISS itself. But now, for the first time, this job was done by the advanced ESA spacecraft Jules Verne that docked with ISS early this month.

Jules Verne boosts ISS

Click here for an Animation of the ISS re-boost performed by Jules Verne ATV.

On 25 April 2008, ATV Jules Verne’s main engines burned for 740 seconds and successfully boosted the 280-tonne Station up 4.5 km to a new altitude of 342 km above the Earth’s surface.

 

Source: ESA News