Showing posts with label Sun. Show all posts
Showing posts with label Sun. Show all posts

29 Aug 2016

Astronomy Before Bedtime




Photo by NASA Goddard Space Flight Center showing a C3-class solar flare that erupted from sunspot 1105 on Sept. 8, 2010. Used under CCBY-2.0 license.

by Adrienne Montgomerie

“I really like astronomy, but I can’t stay up that late,” I said to the astronomer I met the other day.

“Lucky for me,” he said. “I do my astronomy during the daytime. Only optical astronomy really requires a night sky — and that's only for ground-based telescopes!” Then Drew the astronomy PhD student at Queen’s University went on to tell me about radio telescopy and telescopes out in space.

Light is part of the EM spectrum, and so are X-rays and radio waves. Astronomers can look for the X-rays and radio waves given off by stars and planets to learn what they are made of and how they behave. That method works even when daylight obscures the objects.

A couple years earlier, I met the team from RMC (the Royal Military College) who study stars in daylight. Their specialty is the Sun!
  
Beginning Daylight Astronomy

The easiest targets are our own Sun and Moon. You can watch the Moon with your bare eyes and observe how its shape changes from crescent to fully round and back to crescent. With a pair of binoculars, you can zoom in on the craters and other features that show the Moon’s history of being hit by space rocks. A telescope lets you see even more detail.

You can observe the how the Sun’s path across the sky changes with the seasons. But you can learn more about the Sun itself.

It can damage your eyes to look straight at the Sun, but there are filters that fit over a telescope to make observing the Sun safe. One really fun time to observe the Sun is during a solar eclipse, but even with most of the light blocked by the Moon, it’s still unsafe to look directly at the Sun. One easy trick is to have a telescope project the image of the Sun onto a piece of paper. With your back to the Sun, put paper below the telescope’s eye piece. You can then look at the Sun on the paper.
  
Events in the Daytime Sky

On August 21, 2017 there will be a total solar eclipse visible from coast to coast in the USA. It is only visible where the shadow meets Earth, so not everyone will see it.

An eclipse is a great time to get a better look at the Sun’s corona. Because the Moon blocks most of the Sun during an eclipse, it makes the remaining part easier to see. The outer edge (corona) is where you can see great tongues of fire exploding from the star (like in this picture). Those are called flares and they can be as powerful as 1 billion megatons of TNT! Solar flares are what send electromagnetic waves outward from the Sun. When they reach Earth, they cause Northern Lights (and Southern Lights, too). When there’s a big solar flare, you can watch for signs of it affecting Earth a few days later. It’s not just pretty lights that solar flares cause. Sometimes that radiation interferes with radio and power transmission here on Earth.

Lunar eclipses sometimes happen during the day, too. It’s not as dramatic as a nighttime eclipse, but you can see Earth’s shadow take a bite out of the Moon. You can see that without anything but your eyes.

To learn more about astronomy, check the Royal Astronomical Society of Canada (RASC) and Sky News magazine. 

Adrienne Montgomerie is a science and education editor who helps publishers and businesses develop training resources. She believes we can make even the most complex ideas and procedures easy for learners to take in, maybe even to master.

3 Mar 2016

Eclipse Plans

NASA has plans for the total eclipse of the sun expected in Indonesia on March 9. Here's their short video discussing the photographs they plan to take during that brief time:

 

If the video doesn't load here, you can see it by clicking on this link. Click on it anyways if you're interested in eclipses! On that webpage, NASA writers have posted several short comments with interesting pictures on their studies of eclipses and the sun. Most important among these comments is the advice on eye safety when observing a solar eclipse -- that's a must read for anyone!

2 Nov 2012

What's NOT a black hole?

By M. E. Powell
(Photo - http://creativity103.com)

Scientists and science fiction writers often influence or inspire each other. I gained some insight into that process during "When Words Collide," the Calgary science fiction and genre writers festival, earlier this year.

For example,  David Wesley Hobill of the University of Calgary led a workshop in his special interest subjects: black holes, dark energy, and dark matter. I'm sure I'll over-simplify what he said, but his lecture shed some light on the "dark side of the universe" for me.

Hobill talked about finding black holes by observing gravitational effects. For example, we may observe a quasar at a far distance from Earth. If something is between us and the quasar, we know the gravity of that object will bend the light coming from the quasar. This "gravitational lensing" results in multiple images. If we observe light bending or being redirected around an object, but we can't see what is causing the light to bend, we deduce that a black hole is likely the cause.

Gravitational time delays caused by strong gravity may also cause time to slow down. Curved space requires more time to traverse. Inside it, a person's heartbeat may slow to two beats per hour, for instance, causing the person to live longer. Time would appear to stop. (You can imagine what science fiction writers might make of that train of thought!)

Hobill also debunked some popular science fiction myths about black holes. For example, he said, black holes are not:
- cosmic vacuum cleaners
- portals to another universe
- made of dense material.
In fact, black holes are completely empty space, he said, caught at the moment of a change of energy.

Instead, he pointed out, scientists would say that black holes are:
- formed from the gravitational collapse of a star 
- empty of space-time
- boundaries of causally separated regions
- cold and black
- and very very small.
If our sun collapsed into a black hole, for example, it would implode the gravitational forces, and it would become 400,000 times smaller. In other words, Hobill said, it would end up being about the size of downtown Calgary.

Here are some interesting links to follow up, if you're interested in black holes:
Hubble Site: Black Holes - Gravity's relentless pull: http://hubblesite.org/explore_astronomy/black_holes/
NASA: Black Holes - What are they? http://imagine.gsfc.nasa.gov/docs/science/know_l2/black_holes.html
NASA: What is a black hole? http://www.nasa.gov/audience/forstudents/k-4/stories/what-is-a-black-hole-k4.html 
Black Holes - Frequently asked questions: http://cosmology.berkeley.edu/Education/BHfaq.html

M. E Powell is the a Regina-based professional writer and the author of Dragonflies are Amazing (Scholastic Canada, 2007).

6 Oct 2012

Celestial Navigation


by Joan Marie Galat

Imagine you’re a sailor more than 300 years ago. A storm takes you out of sight of land and you don’t know your location. You worry you could run out of fresh water and food or pirates might attack. Clouds hide the Sun and make it difficult to tell your direction. You have a compass but maps in the 1700s are not very accurate. With night coming, all you can do is hope your ship doesn’t hit any rocks.

Now suppose your only compass falls into the sea! Good thing you know a bit about celestial navigationIf the Moon should rise before the Sun sets, you will be able to tell your direction. The rising Moon is illuminated on its west side because the Sun sets in the west. But if you look after midnight, the eastern side is lit.

If the sky clears you’ll be able to find Polaris, the North Star. You can use your sextant to measure the angle of a star or other celestial body. This tells you your latitude—how far north or south you are from the equator. Celestial navigation can save your life. But you still need to know your longitude—your direction east and west.

A carpenter named John Harrison spent many years trying to solve the problem of determining longitude at sea. He realized that if you knew the time at a specific location on land, as well as your exact time at sea, you could figure out your longitude. Unfortunately, time pieces were not very accurate at this time. Clocks with pendulums could not keep accurate time on a boat.

Harrison devoted his life to solving the problem but it took the King of England to make sure he got the recognition he deserved. Thanks to Harrison’s work, everyone on Earth recognizes the same time zones. 

You can read his story in my newest title, The Discovery of Longitude. This historical picture book for ages five and up
is published by Pelican
Publishing Company. Visit www.joangalat.com for details.

30 Jan 2012

When is a planet a dwarf planet?

by Joan Marie Galat

When visiting schools or delivering presentations via Skype, one of the most common questions I’m asked is “Do you think Pluto should still be called a planet?” If only my opinion mattered! My reply brings approving nods from my audience. “Deep in my heart, Pluto will always be a planet to me.” But the nodding stops when I go on to say "I understand why the International Astronomical Union (IAU) felt it was necessary to redefine what constitutes a planet."

It is no longer enough for a celestial object to orbit a star and be larger than an asteroid. A planet must be round or nearly-round, with gravity strong enough to disperse celestial objects from its orbit. The IAU defines Pluto as a dwarf planet.While it is the right shape and does orbit the Sun, it also travels through an area where asteroids exist. Pluto moves through the Kuiper Belt, a zone of icy objects beyond Neptune’s orbit. Other dwarf planets include Eris and the former asteroid Ceres. 

Here’s some fun space trivia about Pluto and the planets in our Solar System.

    Photo courtesy of NASA
  • Pluto was classified as a planet for 75 years.

  • Venus, Uranus, and Pluto rotate in a direction opposite to that of the other planets.

  • Mercury travels around the Sun at an average speed of 172,300 km an hour (107,000 miles an hour).

  • Mercury’s core is made up of iron.

  • The surface of Venus is a desert. About 64 km (40 miles) above the desert surface, winds blow at 426 km/hour (265 miles/hour). The upper atmosphere swirls 50 times faster than the planet rotates!

  • Gently rolling hills, as well as thousands of volcanoes cover most of the surface of Venus. Some craters are produced by volcanic eruptions, while others are produced by impacts.

  • When closest to Earth, Mars is only 56 million km (35 million miles) away, but its farthest point is 400 million km (250 million miles).

  • The clouds surrounding Jupiter travel at different speeds, rotating faster at the equator than near the poles.

  • Another moon of Jupiter, called J3, is only 40 km (25 miles) across. It is the fastest moon in the solar system, traveling 113,300 km/hour (70,400 miles/hour). J3 would only take a few minutes to travel over North America, from the Atlantic to the Pacific coast.

  • There are always storms on Jupiter. It is not unusual for a Jovian storm to be 9600 km (6000 miles) across. Wind on Jupiter has been measured at 650 km/hour (404 miles/hour).

  • Electricity flows back and forth between Jupiter and Io, which has active volcanoes that erupt with hot gas and molten sulphur.

  • Wind speeds on Saturn can reach 1770 km/hour (1100 miles/hour).

  • Uranus is tipped on its side, causing each pole to alternate facing the Sun. At times, this makes Uranus’s polar regions warmer than its equator.

  • Neptune’s largest moon is called Triton. It is one of the coldest places in the solar system, with temperatures of –391° F (–235° C). Triton revolves in the opposite direction from the planet’s rotation and is the largest moon in the solar system to do so.
 
Explore more cool space facts in Dot to Dot in the Sky, Stories of the Planets, published by Whitecap Books. Look for it at your local bookstore, online, or order an autographed copy from my website. Discover the Greek myths associated with each planet's namesake, along with astronomy facts and tips for observing the planets.

8” x 9”
64 pp. ISBN 1-55285-392-6
Color illustrations
Ages 8-12


“This is an excellent book. It’s very interesting to read about the mythological stories behind the names of the planets of our solar system, as well as the planetary facts. I appreciate that Joan Marie Galat is very careful in making the important distinction between the myths and the facts of what we know today. I believe that star gazers of all ages will be fascinated by these stories.”
Julie Payette, astronaut