A Surprise at the Termination Shock

by | Oct 15, 2009 | Interstellar Medium | 5 comments

Findings that are outside our expectations seem par for the course as we explore the Solar System. From the volcanoes of Io to the geysers of Enceladus, unusual things show up with each new mission. Why should IBEX be any different? The Interstellar Boundary Explorer is the first spacecraft expressly designed to study what happens at the edge of the Solar System, where nearby space meets the interstellar medium.

The ‘bubble’ around the Sun called the heliosphere comes about as charged particles in the solar wind move continuously away from the Sun. Although IBEX is far from the heliopause (it’s orbiting the Earth with an apogee of 322,000 kilometers and a perigee of 16,000 kilometers), its instruments are tuned to study energetic neutral particles (ENAs) swept up by the solar wind in the boundary between the edge of the heliosphere and interstellar space beyond. IBEX has been mapping this area since last October.

And here comes the surprise, as explained by IBEX principal investigator David J. McComas (SwRI):

“The IBEX results are truly remarkable, with emissions not resembling any of the current theories or models of this never-before-seen region. We expected to see small, gradual spatial variations at the interstellar boundary, some ten billion miles away. However, IBEX is showing us a very narrow ribbon that is two to three times brighter than anything else in the sky.”

IBEXribbondetail

Image: Accurate timing of the incoming ENAs allows the IBEX team to obtain a higher resolution in the latitudinal direction. The inset at right shows some of the fine detail of the ribbon. Credit: SwRI.

Yes, we’ve got two Voyager spacecraft out there, but IBEX is giving us the big picture, imaging the region not with photons but ENAs from its distant vantage in a highly elliptical Earth orbit. It’s focusing on the so-called ‘termination shock,’ where the solar wind collides with interstellar gas. As they pass through the region, neutral hydrogen and oxygen atoms are dragged by the plasma at the interstellar boundary, while neutral helium passes straight through. Tracing their different arrival directions tells the tale.

McComas adds:

“The most astounding feature in the IBEX sky maps — the bright narrow ribbon — snakes through the sky between the Voyager spacecraft, where it remained completely undetected until now.”

IBEXmagneticfieldinfluence

Image: This image illustrates one possible explanation for the bright ribbon of emission seen in the IBEX map. The galactic magnetic field shapes the heliosphere as it drapes over it. The ribbon appears to trace the area where the magnetic field is most parallel to the surface of the heliosphere (the heliopause). Credit: SwRI.

We’re learning that our Solar System’s interactions with the interstellar medium are more intense than previously believed. As helpful as Voyager’s point measurements are, we now see the region far more clearly. And because the ribbon these data reveal seems to be governed by the direction of the local interstellar magnetic field, it appears that the interstellar medium has a much greater influence on the heliosphere than we originally thought.

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5 Comments

  1. This shows not onlyhow big space really is, but that we better conduct a
    thorough investigation of our immediate celstial neighborhood outside
    the Sol system before we start sending probes all the way to any stars,
    because we clearly do not have the full picture on what is happening right
    near us let alone Alpha Centauri.

    The fact that the two Voyager probes missed this huge ribbon reminds me
    of how the first three successful Mariner probes to flyby Mars missed all the
    goodies on the Red Planet. I realize that the Voyagers were not meant to be
    interstellar explorers directly, but just making a point about how we need
    to really start focusing and examining the near interstellar regions.

  2. Professor Gruntman has an informative site that explains the science and associated challenges of accurate detection of the ENAs: http://astronauticsnow.com/ENA/index.html

  3. Is it just me or does the “ribbon” seem suspiciously near the ecliptic?

  4. Another question: Did the data from the Pioneer 10 and 11 probes
    help in this finding? Was it consulted?

    And can New Horizon contribute to this study of the outer Sol system and
    beyond when it gets past Pluto in 2015?

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  1. Orbiting Frog - [...] Centauri Dreams describes the surprising early results from the IBEX mission, which is mapping the area where the heliosphere meets…
  2. OrbitalHub » Carnival of Space #125 - [...] can read about superconducting magnets used to enable hyperdrive propulsion, the LCROSS mission, surprising early results from the IBEX…
  3. IBEX: From System’s Edge to Nearby Space - [...] IBEX surprise, announced last October, was the discovery that the expected variations in emissions from the [...]

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In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

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