The Earth’s Wobble – Precession

•October 14, 2008 • 1 Comment

In space, our Earth not only feels the gravitational pull of the mighty Sun, it too can feel the gravitational effect of the Moon acting on it. Our Moon may be much much smaller than our Sun, but remember, it is much much closer.

Since our Earth is not completely rigid, as it rotates on its axis, centrifugal force causes the equator to bulge. This is the same force that causes you to fling to the side of a giant spinning wheel in a theme park. The non-uniform gravitational force of the Sun and the Moon will pull on this bulge and causes the Earth to wobble as it spin around it axis, just like a spinning top that is almost falling off.

Technically, this wobble is called precession. Precession of Earth’s rotational axis takes approximately 26,000 years to make one complete revolution. Through each 26,000-year cycle, the direction in the sky to which the Earth’s axis points goes around a big circle. In other words, precession changes the “North Star” as seen from Earth.

Earth Precession

Precession – the slow and gradual shift of Earth’s axis through a 26,000-year cycle.
When viewed from outside and looking down onto the Earth from the north, the direction of precession is clockwise. When standing on Earth looking outward, the axis appears to move counter-clockwise across the sky.

Currently, the Earth’s axis is pointing somewhere near Polaris in Ursa Minor, hence north star today is Polaris. However, almost 5,000 years ago, Thuban in the constellation of Draco was the north star, and was used by the ancient Egyptians. In 13,000 years from now, precession will bring Earth’s rotational axis near Vega in Lyra. That time, Vega will become our north star.

Precession was discovered by Greek astronomer Hipparchus, who had access to several centuries of Babylonian and Greek records. He compared these ancient records to his own and concluded that the axis which the heavens seemed to rotate shifted gradually, though very slowly.

Carnival of Space #74

•October 10, 2008 • Leave a Comment

It’s time for carnival again… this week’s host is Kentucky Space.  Check it out!

Images from Mercury 2nd Flyby

•October 8, 2008 • Leave a Comment

Mercury by MESSENGER. Click to enlarge

The spectacular image shown here was taken at an altitude of 27,000 km and shows a Wide Angle Camera image of Mercury taken about 90 minutes after the spacecraft’s closest approach to the planet. The surface we are seeing here is almost opposite to the side we see during the first flyby, so most of surfaces were previously unseen by spacecraft. Credit: NASA/JHUAPL/CIW

My first impression is “uh, watermelon??”… but wrong colour…

No, this is Mercury, taken by MESSENGER during its second flyby on Monday. The bright stripes that make it look like a watermelon is known as rays. When something slammed onto a surface it formed an impact crater, at the same time materials were thrown out in all direction from the crater forming radial streaks called rays. Look at any full moon pictures and you will see similar rays radiating out from some of the craters on our own Moon.

The crater responsible for these rays is located near the north pole of the planet and we can clearly see that the rays are stretching almost all the way around the globe to the south pole. These rays actually are not new to astronomers – we know they were there before MESSENGER by bouncing radar signals off Mercury from Earth.

The bright crater slightly below the middle of the image is called Kuiper, identified in the 1970s during the Mariner 10 mission. The rest of the terrain to the right of Kuiper is new.

Kuiper, and other bright craters with rays, are relatively young craters. Reason is we seldom see rays system on old craters because over time space weathering such as meteorite impacts will erase the rays. If we see rays system, then it must be a recent impact since there has been little time to erode it. Also, younger craters tend to be brighter for the same reason.

Mercury by MESSENGER. Click to enlarge.

This close-up image of a portion of Mercury’s surface is imaged by spacecraft for the first time. Credit: NASA/JHUAPL/CIW

Mercury by MESSENGER. Click to enlarge.

The largest impact feature at the top of the image is about 133 km in diameter and is named Polygnotus, after a Greek painter from the 5th century B.C. Another comparably large crater at the top left of the image is named Boethius, after the 6th century Roman philosopher. These two features appear to be filled with smooth plains, which is very different in texture form their surrounding terrain. Credit: NASA/JHUAPL/CIW

Source: MESSENGER Gallery

10th Anniversary of Hubble Heritage Project

•October 7, 2008 • Leave a Comment

The Hubble Space Telescope or HST or sometime just called Hubble, was taking tons of incredibly fantastic images faster than the Hubble team could release to the press, and hence some of these incredible images were not seen by the public. But the astronomers working with Hubble wanted to share them with everyone.

So in October 1998, the astronomers came up with the Hubble Heritage Project. The idea is that each month they will release a previously unseen Hubble image, showcase some of the most attractive images ever taken by the telescope and share them with the public. The images they released is not just science, but it’s an art as well, for the Heritage team has presented aesthetic images that present the universe from an artistic perspective.

And this month marks the 10th anniversary of this project. To celebrate this birthday, the Heritage team releases the image below – a close-up detail at the edge of nebula NCG3324.

Close-up detail at the edge of NGC3324. Click to enlarge. 

NGC3324 is a star-forming region located in the northwest corner of the Carina Nebula in the southern hemisphere. The intense ultraviolet radiation from nearby young and hot stars (don’t forget this is a star-forming region!) ionised the surrounding material causing the nebula to glow.

NGC3324 is a “hole” or a “bubble” in space (see image below, the Hubble image above is located at about 2 o’clock position); strong stellar winds from young, massive and hot stars nearby blow away their surrounding material and leaves behind a “hole” (blue colour in the image above) full of wispy tendrils of gas.

However, in some part of the nebula, the gasses and dusts are thicker, so they are harder to erode. The result is the “fingers” you see in the image above – denser blobs of material light-years in height, rising above the glowing gas. Enlarge the image above and follow the edge of the “hole”, you will sure to find more of them, big and small.

NGC3324

Ground-Based Image of NGC 3324 in the Carina Nebula Complex.
Credit: Copyright 2006 Brad Moore and Southern Astro

Hubble may be having problem now, but no matter what happens to it eventually (nothing last forever, anyway), the tons of science and images of the universe that it has brought for us will be treasured forever.

Prepared for Mercury 2nd Flyby by MESSENGER

•October 3, 2008 • 1 Comment

MESSENGER at Mercury10 months ago, MESSENGER, a spacecraft designed to study Mercury, made its first flyby of the innermost planet. On this coming Monday, October 6, MESSENGER is going to make its second flyby, passing a mere 200 km above its surface.

The primary purpose of flyby is to use Mercury for a gravity assist to tighten the spacecraft’s orbit and to keep it on track so that it can enter into orbit around Mercury in 2011, becoming the first spacecraft ever to orbit Mercury.

Gravity assist is important because it can greatly reduce the fuel load requirement of MESSENGER by using the gravitational attraction of planets to change and shrink its orbit about the Sun. The more massive the planet and the closer the spacecraft passes above the planet, the greater the change in the spacecraft’s orbit.

Since the launch of MESSENGER from Earth on August 2004, it has already flown past Earth once, Venus twice and Mercury once. This upcoming flyby and another last pass of Mercury in September 2009 will use Mercury’s gravity to brake and guide the probe progressively closer to the planet, so that at the 4th Mercury encounter in March 2011, Mercury can “capture” MESSENGER into orbit around the planet.

MESSENGER Trajectory Adjustments. Click to enlarge.
MESSENGER mission timeline featuring major trajectory adjustments.

Although gravity assist is the main priority, we, of course, will not miss the chance to snap some beautiful pictures and make some measurements.

During the first flyby in January, MESSENGER captured images of about 20% of Mercury’s surface not previously seen by any spacecraft, revealing new and unexpected features. During this second flyby, MESSENGER plans to reveal another 30% of the surface that has never been seen before. It will show us a completely new surface, opposite from the side of the planet we saw during the first flyby.

Additional to revealing new surface features, other instruments onboard the spacecraft will also be busy taking measurements, such as the Mercury Laser Altimeter (MLA), the Visible-Infrared Spectrograph (VIRS) on the Mercury Atmospheric and Surface Composition Spectrometer (MASCS), the X-Ray Spectrometer, and the Gamma-Ray and Neutron Spectrometer.

The second flyby is expected to yield more surprises. Stay tuned for more updates and more images of our smallest planet!

Source: MESSENGER Mission News

Carnival of Space #73

•October 3, 2008 • Leave a Comment

“HAPPY BIRTHDAY TO YOU, DEAR NASA” – this is an acronym for the posts at Carnival of Space this week in celebration of NASA’s 50th Anniversary. The Carnival is now live at Alice’s Astro Info.  Check it out!

Hubble Space Telescope is Terribly Sick…

•September 30, 2008 • 2 Comments

Hubble Space TelescopeHubble Space Telescope, the scope that had brought us tons and tons of beautiful pictures of the universe, has encountered a major failure and was unable to send any data back to Earth…

The failure of the “Side A” control system forced to shut down Hubble’s science operations and currently Hubble is in safe mode. The spacecraft is basically still operational but just that it is unable to operate the instruments.

We are still not totally out of hope though, because there is a backup system known as “Side B”. But the problem is all this while we have been using only Side A; and Side B has never been operated since the launch of Hubble 18+ years ago.

So the plan as of now is to transfer science operations to Side B by later this week. This is going to be a significant operation because it requires that five other modules used in managing data also be switched to their B-side systems. Hopefully everything will be fine.

Actually, there is going to be a servicing mission to Hubble middle of next month to extend its operational life, to install new instruments and to replace some old one. Now, NASA is thinking whether a replacement control system – to act as spare – will be required to launch with the current servicing mission. If that is the case, then the mission will be delayed until the replacement part has been tested and sent to Kennedy Space Center (KSC) and also the time required to trained the astronauts to install them.

So now what we can do is just wait. If Side B managed to come online, then Hubble can continue its work. If it fails, then we’ll have a non-working observatory up there until the next servicing mission, which may be at least three months before it can be launched.

However, to look at the bright side, at least this happens before the servicing mission…