STEREO Maps Far Reaches of Solar System

Article written: 2 Jul , 2008
Updated: 24 Dec , 2015
by

NASA’s twin STEREO spacecraft have been studying the sun since their launch in 2006. But the mission made a surprising and unexpected discovery by detecting particles from the edge of the solar system, and for the first time, scientists have now been able to map the region where the hot solar wind meets up with the cold interstellar medium. However, this wasn’t done with optical instruments imaging in visible light, but by mapping the region by means of neutral, or uncharged, atoms. This breakthrough is a “new kind of astronomy using neutral atoms,” said Robert Lin, from the University of California Berkeley, and lead for the suprathermal electron sensor aboard STEREO. “You can’t get a global picture of this region, one of the last unexplored regions of the heliosphere, any other way because it is too tenuous to be seen by normal optical telescopes.” The findings also help clear up a discrepancy in the amount of energy in the region found by the Voyager 2 spacecraft as it passed through the edge of the solar system last year.

The heliosphere stretches from the sun to more than twice the distance of Pluto. Beyond its edge, called the heliopause, lies the relative quiet of interstellar space, at about 100 astronomical units (AU) – 100 times the Earth-sun distance. The termination shock is the region of the heliosphere where the supersonic solar wind slows to subsonic speed as it merges with the interstellar medium. The heliosheath is the region of churning plasma between the shock front and the interstellar medium.

The twin STEREO spacecraft, in Earth’s orbit about the sun, take stereo pictures of the sun’s surface and measure magnetic fields and ion fluxes associated with solar explosions.

Between June and October 2007, however, the suprathermal electron sensor in the IMPACT (In-situ Measurements of Particles and CME Transients) suite of instruments on board each STEREO spacecraft detected neutral atoms originating from both the shock front and the heliosheath beyond.

“The suprathermal electron sensors were designed to detect charged electrons, which fluctuate in intensity depending on the magnetic field,” said lead author Linghua Wang, a graduate student in UC Berkeley’s Department of Physics. “We were surprised that these particle intensities didn’t depend on the magnetic field, which meant they must be neutral atoms.”

UC Berkeley physicists concluded that these energetic neutral atoms were originally ions heated up in the termination that lost their charge to cold atoms in the interstellar medium and, no longer hindered by magnetic fields, flowed back toward the sun and into the suprathermal electron sensors on STEREO.

“This is the first mapping of energetic neutral particles from beyond the heliosphere,” Lin said. “These neutral atoms tell us about the hot ions in the heliosheath. The ions heated in the termination shock exchange charge with the cold, neutral atoms in the interstellar medium to become neutral, and then flow back in.”

According to Lin, the neutral atoms are probably hydrogen, since most of the particles in the local interstellar medium are hydrogen.

The findings from STEREO, reported in the July 3 issue of the journal Nature, clear up a discrepancy in the amount of energy dumped into space by the decelerating solar wind that was discovered last year when Voyager 2 crossed the solar system’s termination shock and entered the surrounding heliosheath.

The newly discovered population of ions in the heliosheath contains about 70 percent of the energy dissipated in the termination shock, exactly the amount unaccounted for by Voyager 2’s instruments, the UC Berkeley physicists concluded. The Voyager 2 results are reported in the same issue of Nature.

A new NASA mission, the Interstellar Boundary Explorer (IBEX), is planned for launch later this year to map more thoroughly the lower-energy energetic ions in the heliosheath by means of energetic neutral atoms to discover the structure of the termination shock and how hydrogen ions are accelerated there.

Original News Source: EurekAlert


10 Responses

  1. Sps says

    Good point IT-SYSTEMS. Although I strongly disagree on your concluding argument.

  2. Al Hall says

    Me too! It would a little more like:

    ê  ñ¥°¢å°­?å° ?í»µ ñ¨±²å¬®Ì®í² æ¬ í ±ò°®©ê ¬ ﮤ䥰檠 ñ¥°¢å°­î£® 𳤮⠭迮
    😉

  3. Sili says

    Høbs bøbberjøbs, du gamle.

    I take it this doesn’t have any bearing on the Pioneer-anomaly?

  4. Sps says

    Although IT-SYSTEMS points were rather controvertial, I did not find them inappropriate enough so as to remove them.

  5. Al Hall says

    Sps –
    I know.. I have been trying to post the IBEX link here but I am guessing her filter is squeezed too tight.. Anyway, here is the link for those interested..:
    ibex.swri.edu/mission/index.shtml
    Just copy and paste..
    🙂

  6. alphonso richardson says

    Not sure it a full or proper conclusion, this ‘ energy dumping’. BUT, if it has an effect on the velocity/trajectory anomalies experienced by these probes (voyager/Pioneer (?)), maybe, just maybe, we can just think about possibly stop babbling on about dark matter, at least in this instance.

  7. Ayti says

    Given this new understanding do we still think that solar sails will power interstellar travel? If these particles are inbound won’t they have a cancelling effect on the leading face of the sail reducing overall momentum? A the termination shock the solar wind slows down why would the sail manitain it’s momentum? It seems that there is still some fiction in the science of interstellar propulsion at least as far as sails are concerned. I’m not a physicist so I look forward to reading some responses on the question.

  8. Ayti says

    alphonso richardson how does this obviate the need for a theory of dark matter to explain part of the “missing ” matter in the universe?

  9. zifferman says

    I never knew the outer solar system had so
    many colors.

    Wow, man – the sixties were right after all.

  10. Nexus says

    Ayti-
    Once the solar wind gives out at the termination shock, the ship will continue to move at the velocity it had when it hit the termination shock because there’s nothing out there to slow it down. It just won’t get any faster

    And if incoming particles are significant enough to slow the ship, then probably the solar sails could be folded up or broken off.

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