Yearly Archives: 2011

Mercury, MESSENGER, NASA

Standard Mercury Orbit, Mr. Sulu

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Mercury Has a Long-Term Visitor

MESSENGER at Mercury (artist's conception). Courtesy MESSENGER Mission.

Last night I went down to the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado for a briefing and “wait-it-out” event for the MESSENGER spacecraft’s orbital insertion. The lab built one of the instruments onboard the spacecraft — the Mercury Atmospheric and Surface Composition Spectrometer (MASCS). As I was sitting there watching the folks in the control room at the Johns Hopkins Applied Physics Laboratory (by remote link), I thought about all the times we’ve seen “standard parking” orbit commands applied in shows like Star Trek. They make it sound so easy. The captain just says “Standard orbit” to the helm, the officer punches a few buttons or slides a fader or waves a hand over the console, and the ship slides into the correct spot.  What we don’t see are the ship’s thrusters firing to nudge the ship — a massive behemoth compared to a small planetary probe like MESSENGER —  from its previous course into the parking orbit around the world it’s visiting.

We didn’t actually see MESSENGER’s thruster fire either last night. What we heard was a stream of announcements that told us what the Doppler readings were from the spacecraft as its fuel tanks fed the thruster that nudged it into a parking orbit (highly elliptical at that!) around Mercury.  You can see an animation of how it might have looked here.

To see the kind of orbital trip MESSENGER has taken since its launch on August 3, 2004 , go here for an animation showing its long journey. As of today, the spacecraft has traveled 4,902,668,000 miles. That’s 7,890,000,000 kilometers, or 52.7 astronomical units. If Messenger had traveled in a straight line for that distance, it would be well beyond the most distant point of Pluto’s orbit!

MESSENGER's orbit around Mercury is very elliptical, meaning its lowest point is only about 124 miles (200 km) above the surface and gets as far asway as 9,300 miles (15,000 km) at its most distant. The closest approach of the orbit will take it high over the north pole, where there is some radar evidence of something -- possibly water ice -- hidden on crater walls. Courtesy NASA/JHUAPL.

MESSENGER is small, only about the size of a minivan, so it wouldn’t take nearly as much power to put it into “standard orbit” as a giant starship would need.  But, the principles are the same no matter what size of object you’re trying to put in orbit around another one.  The incoming object has a certain path it’s following, and it’s going at a certain speed. If you want the spacecraft to merely fly by, you wouldn’t need to deviate the probe from its path.  But, if you want it to go into orbit, you have to slow it down at the right place, the right time, and at the right rate. Once you do that, you’ve got your spacecraft (regardless of its size) at a point where the gravitational pull of the planet it’s orbiting is EXACTLY matched by the spacecraft’s speed around the planet. It’s a constant tug of war that must be balanced correctly.

Now that MESSENGER is safely orbiting Mercury, scientists are testing its systems to make sure they’re doing okay in the hot, harsh environment around the planet.  The spacecraft is subject to solar heating eleven times hotter than we experience here on Earth, and it is protected with a sunshade to protect the delicate instruments inside. As soon as they’re satisfied that all systems are working on the nominal, they’ll turn the instruments on and commence the next phase of mission science.  The first images should start streaming to Earth in the first part of April, so stay tuned!

black hole, black holes, chandra x-ray telescope, x-ray astronomy

Blobs in Space

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Often Turn Out to be Pretty Interesting

his composite image shows the central region of the spiral galaxy NGC 4151, dubbed the "Eye of Sauron" by astronomers for its similarity to the eye of the malevolent character in "The Lord of the Rings". Courtesy Chandra X-ray Telescope.

You just have to know what you’re looking at when you see something like this appear in the astronomy news of the day. Sometimes I laughingly refer to pictures like this as “blobs in space”. But, as I know — and you’re about to read– a further look at them gives you a peek at something you didn’t expect.And, you get to learn something new about things like galaxy cores and black holes, in the bargain.

This set of “blobs” is dubbed the “Eye of Sauron” because astronomers studying it decided this central region of the spiral galaxy NGC 4151 kind of looked like the object of the same name in the “Lord of the Rings” movie. The pupil of this “eye” shows x-rays (colored blue) streaming from a central object embedded in the core of the galaxy.

The yellow spots out in the corners of the eye are actually visible-light data (called “optical”) showing the location of positively charged hydrogen gas (also known as H II, which means it is energized in some way).  These are regions where star formation has occurred in the recent past.

The red blobs are clouds of neutral hydrogen gas, which show up in radio wavelengths.  They are part of a larger structure that is being distorted by gravitational interactions with other parts of the galaxy. And, some of it is material falling INTO the center of the galaxy, toward the pupil.

So, now that we know what the pieces and parts are, what does they mean?  Recent work shows that the blue-labeled x-ray emission is probably coming from an outburst powered by a supermassive black hole at the heart of the galaxy.  That black hole region is colored white in the image.

Evidence for the idea that some kind of action is tossing out x-rays from the center comes from the elongation of the x-ray emissions running from the top left to the bottom right and details of the x-ray spectrum. There are also signs of interactions between a central source and the surrounding gas, particularly the yellow arc of H II emission located above and to the left of the black hole.

Astronomers have posed a couple of  different scenarios to explain the x-ray emission. One possibility is that the central black hole was growing much more quickly about 25,000 years ago (in Earth’s time frame) and the radiation from the material falling onto the black hole was so bright that it stripped electrons away from the atoms in the gas in its path. X-rays were then emitted when electrons recombined with these ionized atoms.

The second possibility also involved a hefty flow of material into the black hole in relatively recent times. The energy released by material flowing into the black hole in an accretion disk created a vigorous outflow of gas from the surface of the disk. That outflox directly heated gas in its path to  temperatures hot enough to permit the emission of x-rays.  Unless the gas is confined somehow, it would expand away from the region in less than 100,000 years. In both of these scenarios, the relatively short amount of time since the last episode of high activity by the black hole may imply such outbursts occupy at least about 1% of the black hole’s lifetime.

It’s amazing what you can learn when you look at blobs in space through the viewpoint of astronomers. They use not just astronomy and physics, but also chemistry and astrophysics to explore and understand the processes and events that occur in the hearts of galaxies like this one, which lies some 43 million light-years away from us. Thanks to tools like the Chandra X-ray Telescope, the Isaac Newton Group of  Telescopes on La Palma, and the National Radio Astronomy Observatories, images like this can be obtained, explained, and shared with everybody.  We all win when that happens. For more information on this image and to see other wavelength views of the “Eye of Sauron” visit the Chandra X-ray Telescope’s story about these observations.