Saturday, 12 October 2013

Ison GIF from NASA's STEREO-A spacecraft

Is animated GIF is of comet Ison comes from the NASA Comet Ison Observing Campaign and was taken by NASA's STEREO-A spacecraft using the SECCHI HI-2 camera. STEREO-A is is now the 7th spacecraft to view Ison and will continue to observe her right through to January.

The image is made up from photo's taken on the 10th and 11th of October and was put together by Karl at the CIOC. Karl is very critical of his work but we're sure you'll agree he did an excellent job!

Ison can be seen between the red lines. Ison GIF by Karl of the CIOC taken by the STEREO-A 

Explaining the GIF Karl said:
"Obviously comet ISON appears very small right now, as it is a long distance from the spacecraft, and the pixels in that image are very big. By that, I mean that each pixel of the image actually contains a fairly significant chunk of sky. By my very rough estimates based on previous experience with comets in that camera, I'd say ISON is somewhere around mag 10 -- which is more-or-less what ground observers are beginning to see, too. Also visible in the image are lots of bright blobs -- those are stars. Finally, that funny wedge-shaped thing is something we placed in the instrument field of view for early during the STEREO mission (back in 2007-ish) when the Earth was in the field of view and would have blinded the camera if not for that little wedge. "


NASA's STEREO spacecraft


The CIOC are still processing the data from the STEREO-A mission and are hoping to release more pictures in the next few days. In addition to the STEREO-A spacecraft there is also a STEREO-B craft and ISON should becoming in to it's view in a few weeks! 
NASA's STEREO Mission was launched in 2006 to study coronal mass ejections from the Sun. The mission consists of 2 craft A and B, one craft travels ahead of Earths orbit while the other follows. STEREO stands for Solar TErrestrial RElations Observatory and both craft are fitted with an extreme ultraviolet imager, two white-light coronagraphs and a heliospheric imager.




New image of Ison with Mars and Regulus by Norbert Mrozek

This great image of Ison was captured by astronomer Norbert Mrozek and cleaned up by the good people at comet Ison news. You can see Ison to the left of the photo, Mars in the centre while Regulus is to the right. We love the clarity of this shot as well as the glare from Mars!

Ison, Mars and Regulus by Norbert Mrozek

Wednesday, 9 October 2013

New reseach shows Ison Will survive the Sun and will put on a show!

Great news for astronomers await Ison.... it looks like Ison will survive her encounter with the Sun, and will put on quite a show doing it! Today we have heard the conclusions from two separate research teams who have been studying Ison, and both have good news!

Planetary Science Institute scientist Dr Jian Yang Li, has been tasked with studying Ison.
Dr Jian Yang Li who is a world leading comet expert and has worked with NASA on the Deep Impact and Dawn missions, presented his research findings which were funded by NASA and the Space Telescope Science Institute to the American Astronomical Society's division for planetary sciences 45th Annual Meeting in Denver.

Dr Jian Yang Li said:
“We measured the rotational pole of the nucleus. The pole indicates that only one side of the comet is being heated by the sun on its way in until approximately one week before it reaches it closest point to the sun,
Since the surface on the dark side of the comet should still retain a large fraction of very volatile materials, the sudden exposure to the strong sunlight when it gets closer to the sun than Mercury could trigger huge outbursts of material. We measured the color of the coma, and found that the outer part of the coma is slightly redder than the inner part, This color change is unusual in comets, and seems to imply that the inner part contains some water ice grains, which sublimate as they move away from the nucleus.”
“As a first-time visitor to the inner solar system, Comet C/ISON provides astronomers a rare opportunity to study a fresh comet preserved since the formation of the Solar System, The expected high brightness of the comet as it nears the sun allows for many important measurements that are impossible for most other fresh comets.”


This image shows the color change of Comet C/ISON’s dust coma. The white dot at the center of the coma marks the location of the nucleus. ISON’s dust coma appears to be less red near the nucleus than it is further away from the nucleus. Although the color change is actually very small, it could be an indication of relatively more water ice particles near the nucleus. Those icy particles evaporate, as they move outward, makes the coma appear redder.


In a separate study by scientists at the Lowell Observatory and Southwest Research Institute (SwRI).
funded by NASA's Lunar Science Institute, carried out new numerical simulations and interpreted them using data from the historical records of  Sun-grazing comet behavior.

Dr Kevin Walsh, a research scientist in SwRI's Planetary Science Directorate at Boulder, Colorado said:
"A major part of our work was to test if the encounter with the Sun would provide enough of a spin increase to pull material off the surface of the comet, When the comet passes near the Sun, it feels the tidal forces pulling on it, and it also gets a slight spin increase due to this rapid flyby. This spin increase is in the prograde direction, so if the comet is already spinning prograde, then it's just that much closer to spinning fast enough to lose mass.A non-spinning or retrograde (back-spinning) comet is more likely to survive because the "backspin" cancels out some of the tidal forces nearest the Sun. The opposite effect would be seen if the comet were spinning prograde, similar to a tennis ball with topspin. In that case, the spin direction would increase the tidal forces at the surface nearest the Sun and aggravate the disruptive potential, even for a comet of far greater density. The faster the prograde rotation and the lower its density, the greater the chances of a comet's disruption."


There has been a lot of speculation of late that Ison will not be as bright as previously thought. This research by the Planetary Science Institute shows that as Ison is not spinning as fast as we would normally expect a comet too. This means that some where in the region of half the ice and gasses that make up the tail are still locked up and waiting to be set free. It is these gases that make up the comets tail and coma.  The study by the Lowell Observatory and Southwest Research Institute has given us new hope that Ison WILL survive its encounter with the sun and backs up the finds by the PSI. All in all today has been full of great news of astronomers across the world!



Tuesday, 8 October 2013

ESA's SOHO Spacecraft image of Ison


With the US shutdown there has been a lack of images coming from NASA, which is particularly disappointing as last week Ison made her closest pass to Mars. Luckily the European Space Agency (ESA) is still up and running and releasing images! The ESA's Solar and Heliospheric Observatory or SOHO for short is a satellite that was launched in 1995 to study the Sun with a variety of on board instruments.Originally the SOHO mission was only going to last a couple of years but due to the amazing results it was producing it is still running today.



The SOHO craft is fitted with a special instrument called SWAN (Solar Wind ANisotrpies) which is the only instrument on board not to be pointed at the Sun, instead it looks at everything else! Swan watches the rest of the sky, measuring hydrogen that is ‘blowing’ into the Solar System from interstellar space. 
By studying the interaction between the solar wind and this hydrogen gas, SWAN determines how the solar wind is distributed. The ESA have used SWAN to detect the hydrogen in Ison's coma, which should be able to tell us how much water is being produced and at what rate. The data from SWAN should give us great new insights in to the emissions given off by sun grazing comets like Ison.

Ison captured by European Space Agency's SOHO craft using the SWAN instrument

The image above is the first image of Ison taken by SWAN to be released by the ESA, over the next few weeks as Ison brightens we should get ever more impressive pictures. Swan takes 360 degree images of space the only thing it doesn't picture is the Sun and the Earth, which are the dark spots on the image. What SWAN is photographing is the effect that solar wind has on the element hydrogen. Sounds complicated but its quite simple really, imagine you wanted to take a picture of the wind, but you cant see it. So you photograph the effect the wind has blowing dust on the ground or on the leaves of a tree, this is basically what SWAN does! Instead of dust and leaves it photographs the effect on hydrogen by the solar wind. What makes this camera particularly important for studying Ison is that because it basically photographs hydrogen, we can tell how much hydrogen is being given off by Ison, which is the main make up of a comets coma and tail. Now even we will admit that this image is not the most spectacular of Ison we've seen, but as Ison gets closer to the sun and more hydrogen is given off  her coma and tail will expand and the images by SWAN will get bigger and better and the data will be invaluable! 

Sunday, 6 October 2013

Ison Location Update 06/10/2013


These are the current co-ordinates for Ison at 18:50 GMT  06/10/2013

Click here for Ison's position on a sky map

Co-ordinates: 09h  47m  30.8s    16*  20'  18.4"
Distance from Sun: 230,379,972 km
Distance from Earth: 296,098,153 km
Magnitude: 10.69

For those who don't know you can track Ison in real time from the comfort of your computer by visiting the fantastic The Sky live website

With thanks to The Sky Live

New photo's of Ison from the Liverpool telescope by Nick Howes

Nick Howes, Ernesto Guido and Martinao Nicolini of theRamanzacco Obsersatory in Itay have been capturing some amazing images of late using the 2m Liverpool telescope. The pictures below are their latest works and show Ison in all her glory! The top image is an enlargement which has been colour corrected. The bottom picture is a stack of twenty, 11 second exposures.

Ison by Nick Howes, Ernesto Guido and Martinao Nicolini

Ison by Nick Howes, Ernesto Guido and Martinao Nicolini


Saturday, 5 October 2013

New photo of Ison by Martin Mobberley

Famous British astronomer Martin Mobberley caputured these fantastic images of Ison.
Martin was using the iTelescope for these pictures. Martin Mobberley is a former president of the British Astronomical Association and currently operates International Astronomical Union Observatory 480. He was honnored by the IAU for his services to astronomy by the renamingof asteroid 7239 to "Mobberley"
He has also written a number of very good books including a biography of Sir Patrick Moore which you can find here.

Ison  05/10/2013   by Martin Mobberley


Ison  04/10/2013   by Martin Mobberley