Question on Comet 67P tail in Rosetta image

In summary: The absence of a magnetic field at Philae's location could mean that the exposed surface does not contain any magnetic material, or that the material is too weak to be detected."The magnetic field detected by the Rosetta mission was not due to the nucleus of the comet.
  • #1
ehilge
163
0
I cam across this picture from the Rosetta mission the other day. You'll notice the sun is illuminating the right hand side of the comet. Additional the tail is coming off the right hand side. This goes against what I've been taught about comets in that the solar wind pushes the tail the opposite direction from the sun. So what's going on here?

My personal thought: The FOV is small enough that we don't see the larger tail getting pushed away. Just some local effects from the sunlight. Does that seem reasonable?
 
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  • #2
Read the description below the picture. It says that heat from the Sun causes the comet's nucleus to expel gas and dust, which is what we see in the picture. You may well be right about the field of view, and also perhaps the larger tail is too dark to see in the comet's shadow, especially next to the bright cloud and comet.
 
  • #3
sk1105 said:
Read the description below the picture. It says that heat from the Sun causes the comet's nucleus to expel gas and dust, which is what we see in the picture.

that doesn't answer the question ... we all know that that is what happens

I agree with the OP ... it seems incorrect and I am not sure why

Dave
 
  • #4
I think that's just material expelled from the sunny side where the surface gets heated. Only subsequently the dispersed material floating around the nucleus gets blown away by solar wind to form the tail (which is a huge, diffuse structure only visible from afar).
It would be odd if it had these jets erupting preferentially on the dark, colder side.
 
  • #5
Bandersnatch said:
It would be odd if it had these jets erupting preferentially on the dark, colder side.
Oddly enough, a dark side jet was captured in the act of erupting the other day.

http://blogs.esa.int/rosetta/2015/04/20/osiris-catches-activity-in-the-act/
ESA_Rosetta_OSIRIS_WAC_20150312T071518-350x343.jpg

The scene at 07:15 CET on 12 March. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

It happens elsewhere, too.
http://rpmedia.ask.com/ts?u=/wikipedia/commons/thumb/c/c1/Hartley2jets2_epoxi_big.jpg/220px-Hartley2jets2_epoxi_big.jpg
Gas and snow jets on http://www.ask.com/wiki/Comet_Hartley_2?qsrc=3044
 
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  • #6
Dotini said:
Oddly enough, a dark side jet was captured in the act of erupting the other day.
That's to be expected - the comet is rotating, and the incoming heat gets conducted throughout its bulk. But the energy input comes from the illuminated side only, so the temperature will always be the greatest there (disregarding variations due to reflectivity, material composition, etc) and most of the jets should come off that side.
 
  • #8
Could this all be the result of some sort of electrically driven erosion? Comet 67P itself was found not to be magnetic yet a magnetic field was detected by both spacecraft . So what could be driving that field?
 
  • #9
Plasmaverse said:
Comet 67P itself was found not to be magnetic yet a magnetic field was detected by both spacecraft
That's a contradiction. The comet was found not to have a global magnetic field, because the sensors did not detect any.
 
  • #10
Plasmaverse said:
Could this all be the result of some sort of electrically driven erosion? Comet 67P itself was found not to be magnetic yet a magnetic field was detected by both spacecraft . So what could be driving that field?
A magnetic field will be associated with the coma.

"The ion tail is formed as a result of the ionisation by solar ultra-violet radiation of particles in the coma. Once the particles have been ionized, they attain a net positive electrical charge, which in turn gives rise to an "induced magnetosphere" around the comet."
http://en.wikipedia.org/wiki/Comet

Speculation about electrically driven cometary erosion is not well justified at the present time and place; we should allow the Rosetta team time to do their studies and papers. Even so, there are a small clutch of papers published on the interaction between solar wind and various bodies such as the Moon producing interesting effects.

"Protons in the solar wind can make small amounts of water continuously on the lunar surface by interacting with metal oxides in the rocks. But some of the water is probably deposited on the Moon from other places in the solar system."
http://science.nasa.gov/science-news/science-at-nasa/2010/18mar_moonwater/

 
  • #11
Bandersnatch said:
That's a contradiction. The comet was found not to have a global magnetic field, because the sensors did not detect any.

From the Rosetta mission site: http://www.esa.int/Our_Activities/Space_Science/Rosetta/Rosetta_and_Philae_find_comet_not_magnetised

"ROMAP measured a magnetic field during these sequences, but found that its strength did not depend on the height or location of Philae above the surface. This is not consistent with the nucleus itself being responsible for that field."
 
  • #12
Alright, you mean the background readings from the solar wind? Sorry, I completely missed your point earlier.

From the same page you linked to:
'Instead, the magnetic field that was measured was consistent with an external one, namely the influence of the solar wind interplanetary magnetic field near the comet nucleus. This conclusion is confirmed by the fact that variations in the field that were measured by Philae closely agree with those seen at the same time by Rosetta.'
 
  • #13
Dotini said:
A magnetic field will be associated with the coma.

"The ion tail is formed as a result of the ionisation by solar ultra-violet radiation of particles in the coma. Once the particles have been ionized, they attain a net positive electrical charge, which in turn gives rise to an "induced magnetosphere" around the comet."
http://en.wikipedia.org/wiki/Comet

Speculation about electrically driven cometary erosion is not well justified at the present time and place; we should allow the Rosetta team time to do their studies and papers. Even so, there are a small clutch of papers published on the interaction between solar wind and various bodies such as the Moon producing interesting effects.

"Protons in the solar wind can make small amounts of water continuously on the lunar surface by interacting with metal oxides in the rocks. But some of the water is probably deposited on the Moon from other places in the solar system."
http://science.nasa.gov/science-news/science-at-nasa/2010/18mar_moonwater/
This "induced magnetosphere" is supposed to deflect the solar wind around the nucleus of the comet so I'm not sure how it could really interact with it to form water. Though I do believe the water is electrically generated.
 

1. What is Comet 67P and what is its tail?

Comet 67P, also known as 67P/Churyumov-Gerasimenko, is a comet that was studied by the European Space Agency's Rosetta mission. Its tail is a long stream of gas and dust particles that is formed as the comet gets closer to the Sun.

2. How was the tail of Comet 67P captured in the Rosetta image?

The Rosetta spacecraft had a high-resolution camera that was able to capture detailed images of the comet's surface and its tail. These images were taken from a close distance as the spacecraft orbited the comet.

3. Why does the tail of Comet 67P appear curved in the image?

The tail of a comet is affected by the solar wind, a stream of charged particles from the Sun. As the comet moves closer to the Sun, the solar wind pushes the tail in the opposite direction, causing it to curve.

4. What can we learn from studying the tail of Comet 67P?

By studying the composition and behavior of the tail, scientists can learn more about the composition and activity of the comet itself. The tail also provides valuable information about the interactions between the comet and its environment, such as the effects of solar radiation and the solar wind.

5. How long is the tail of Comet 67P?

The tail of Comet 67P can vary in length depending on its distance from the Sun, but it can reach up to millions of kilometers in length. In the image captured by Rosetta, the tail appears to be several thousand kilometers long.

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