When the Seeing is Bad

Last week I shot a little video of Mars and Saturn in an attempt to get some nice imagery of these planets. Mars is approaching opposition and Saturn is well placed in the sky for observation. It appeared at first as if the seeing was pretty good, but reviewing the video shows that there were issues.

The results? No so good actually. The Mars shot shows no detail beyond the polar cap, the Saturn shot is marginally better, but still nothing I am happy with. The imagery was taken with the Canon 60D in crop movie mode, and the C11 telescope operating at f/10. I spent some time tweaking the collimation, that looked looked fairly good. The video? The resulting material is not so good, I suspect the main cause of the poor results was seeing, some variant of high frequency distortion blurring the fine details.

There may also be some issues with the new version of Registax. Version 6 has some major differences in how it operates, not sure if I am doing everything right. The program may have some bugs as well, I crashed it several times while attempting to process the imagery.

Saturn
Saturn, C11 and Canon 60D, best 800 of 1200 frames processes in registax

Mars Opposition

Mars during the 2005 opposition
Mars during the 2005 opposition
Today the planet Mars will pass through opposition.

Closest approach of the two planets is not necessarily on the same day as opposition, but can vary up to two weeks. This year closest approach will occur March 5th with the two planets approaching to 99,331,411 km (61,721,554 miles) at 07:01HST. At this distance the red planet will show a disk 13.89″ arc-seconds across in the eyepiece.

All month Mars will be visible throughout the night, high in the sky at midnight. This is the time to enjoy observing our closest neighboring planet while it is nearby and high in the night sky.

Mars Opposition Reminder

One week from today, on March 3rd, the planet Mars will pass through opposition.

Mars orbits the Sun every 1.88 years, with Earth only taking one year for each orbit. Like two runners on a track the two planets race each other around the Sun. But we have the inside lane, lapping the red planet every two years. These events are called opposition, when Mars is closest to us and best positioned for viewing by earthbound telescopes.

Closest approach of the two planets is not necessarily on the same day as opposition, but can vary up to two weeks. This year closest approach will occur March 5th with the two planets approaching to 99,331,411 km (61,721,554 miles) at 07:01HST.1 At this distance the red planet will show a disk 13.89″ arc-seconds across in the eyepiece.2

Mars during the 2005 oppositionMars during the 2005 opposition

Do not worry about viewing on the 3rd or 5th, any time in the month leading up to and after opposition the viewing will be very good. With even a modest telescope it should be possible to see the bright polar caps and light and dark markings on the planet.

All month Mars will be visible throughout the night, high in the sky at midnight. This is the time to enjoy observing our closest neighboring planet while it is nearby and high in the night sky.

1) 2012 Mars Opposition at SEDS
2) The 2012 Aphelic Apparition of Mars

The Moon and Mars

Tonight a nearly full Moon will rise together with the planet Mars. The pair will rise about 20:28 and will be about 9° apart.

Mars is approaching opposition, as the Earth draws closer to the red planet it is getting larger and brighter in our sky. It is now over 12 arc-seconds in diameter and shining at -0.8 magnitude. Opposition will occur March 3rd.

Mars Opposition 2012

About a month from today, on March 3rd, the planet Mars will pass through opposition.

Mars orbits the Sun every 1.88 years, with Earth only taking one year for each orbit. Like two runners on a track the two planets race each other around the Sun. But we have the inside lane, lapping the red planet every two years. These events are called opposition, when Mars is closest to us and best positioned for viewing by earthbound telescopes.

Closest approach of the two planets is not necessarily on the same day as opposition, but can vary up to two weeks. This year closest approach will occur March 5th with the two planets approaching to 99,331,411 km (61,721,554 miles) at 07:01HST.1 At this distance the red planet will show a disk 13.89″ arc-seconds across in the eyepiece.2

Mars during the 2005 oppositionMars during the 2005 opposition

Do not worry about viewing on the 3rd or 5th, any time in the month leading up to and after opposition the viewing will be very good. With even a modest telescope it should be possible to see the bright polar caps and light and dark markings on the planet.

All month Mars will be visible throughout the night, high in the sky at midnight. This is the time to enjoy observing our closest neighboring planet while it is nearby and high in the night sky.

1) 2012 Mars Opposition at SEDS
2) The 2012 Aphelic Apparition of Mars

Pits in the Ice

You know it is cold when the very air starts to freeze.

This is what happens in a Martian winter when no sunlight reaches the polar region. It grows so cold that the atmosphere, mostly carbon dioxide, begins to freeze and fall to the ground as snow. Frozen carbon dioxide, dry ice, accumulates into a permanent polar cap. While the extent of this polar cap waxes and wanes with the Martian seasons, there is always some ice.

The image below, taken by the HiRISE camera aboard the Mars Reconnaissance Orbiter shows of a section of the southern permanent polar cap. Late summer has caused much of the polar cap to sublimate (convert back to gas), exposing some of the rock under the ice.

Here much of the terrain is shaped by the annual freeze and thaw cycles. These pits are probably the result of these cycles and are about 60m (200ft) across. Soon the region will return to the darkness of winter and the pits will be re-buried in the ice.

Pits in the Polar Cap
Pits in the southern Martian polar cap exposed by late summer sunlight, image taken July 29th 2011, credit: NASA/JPL/University of Arizona