Archive for the ‘Astronomy’ Category

Astronaut Training Day 2 - Centrifuge Flights

Saturday, January 16th, 2010

Day 2 was all about the Phoenix centrifuge at NASTAR. After some instruction on techniques to increase blood pressure to avoid loss of vision and black out, we did a series of four flights in the morning. Because the centrifuge only accommodates one person at a time, and because there were a dozen of us, it took a while for everyone to get a ride. I was fifth to go. The four flights consisted of brief profiles of sustained acceleration along either the body’s plus X axis (into the chest) or the plus Z axis (down the spine). The latter pose problems for consciousness because +Gz makes it harder for the heart to pump blood to the brain. The Gx flights make it difficult to breathe, but are not generally likely to make one pass out, at least for the durations we were doing (about 20 seconds at a time).

I have previously had experience with two G’s on parabolic airplane flights. The first time I flew one of those flights, I oriented my body so that the two G’s were in the +z direction, and I got very sick after about a half dozen parabolas. On subsequent flights I lay flat on the floor of the plane, making those G’s in the +x direction and therefore much easier to bear. So I was concerned about our 2 Gz and 3.5 Gz flights, though they wouldn’t have the repetition of the “vomit comet” nor would they be interspersed with 0 G parabolas. On the 3.5 Gz flight I had to apply all of the body-tensing countermeasures we used because I started to get a bit of tunnel vision. The countermeasures worked. The Gx flights, at 3 and 6 G’s, were impressive. The sensation of going up very very fast was completely convincing. At 6 Gx it was a real effort to breathe, and speech was very difficult. All in all, the flights were smooth and didn’t make me sick.

In the afternoon we did two flights simulating the acceleration profile of Virgin Galactic’s SpaceShipTwo. One was at 50% of the total acceleration, and the other was full acceleration. These profiles involved both Gx and Gz at the same time, along with a visual simulation of what we would see through the window of the spaceship. These flights really gave the impression of going somewhere FAST. On the final run, I had to apply countermeasures to keep my vision as things started to go gray during the 3.8 Gz portion of the rocket burn. The peak accelerations are actually on re-entry, but they are Gx and so are easier to deal with.

Astronaut Training Day 1 - Altitude Chamber

Wednesday, January 13th, 2010

Today we got a tour of the NASTAR center which has some impressive aircraft simulators and a gigantic centrifuge (11 ton, 25-foot arm, with bolts going 45 feet down into the bedrock and a huge mass of concrete underneath to keep it stable as it swings around). Then we had a course on the physiology of hypoxia (oxygen deprivation) and some basics on atmospheric physics before getting fitted with oxygen masks and heading for the altitude chamber. I’m not actually sure that’s the write term, but it’s a room with a dozen seats and ports for oxygen masks and can have its pressure adjusted to simulate various altitudes.

After 30 minutes of denitrogenation (breathing pure oxygen to remove nitrogen bubbles from the blood to reduce the likelihood of those bubbles expanding to painful size on ascent to high altitudes), we took our masks off and they took the chamber up to 18,000 feet. That is to say, they lowered the pressure in the room to what it is at an altitude of 18,000 feet. At that altitude, the pressure is about half what it is at sea level. So each breath delivers half the oxygen of a breath at sea level. We had some simple exercises to perform - simple math operations, some writing - to identify any degradation in mental function as we entered a hypoxic state. I noticed an increased heart rate, but no other symptoms. I have done two altitude “flights” in the past, about 10 years ago, with no noticeable effects. I could not tell if the increased heart rate was due to lack of oxygen or simple anxiety about possibly worse effects. After about 15 minutes, one member of our group passed out. By that time I was feeling a bit tired, but otherwise no overt effects of hypoxia. My simple math problems were done without error, as were the two mazes.

Suborbital Astronaut Training at NASTAR - Day 0

Tuesday, January 12th, 2010

Today I flew to Philadelphia with my graduate student, Akbar Whizin, in preparation for a two-day course on suborbital spaceflight at the NASTAR center. With at least two companies readying commercial suborbital rockets to carry paying passengers to the lower limits of outer space, there is increased interest in the uses of these vehicles for science and education and not just high-priced sightseeing. NASA has long had a vigorous program of experimentation in suborbital sounding rockets. These new vehicles may soon find a place as laboratories for scientists and students who need quick and easy access to either the upper reaches of the atmosphere or a few precious minutes of high quality microgravity.

My own scientific interest in these vehicles lies in the study of the collisional behavior of small objects and aggregates of objects at low impact speeds. I’ve had one such experiment fly twice on the space shuttle and a similar experiment has flown several times on parabolic airplane flights. These experiments simulate in various ways the collisions that were common in the early stages of the formation of the solar system and are currently taking place in Saturn’s rings (and the rings of the other planets). It is not possible to perform experiments on these kinds of collisions without a microgravity environment. A few seconds of microgravity can be achieved in a drop tower, and 10-15 seconds of a relatively uneven low-gravity environment can be obtained on parabolic airplane flights. For many experiments a longer, more stable microgravity environment is needed.

Virgin Galactic has unveiled the first of its passenger-carrying suborbital crafts, the VSS Enterprise. Blue Origin has selected my experiment and two others to fly on a test flight of their New Shepard suborbital rocket. Other companies are developing rockets for passengers and some just for payloads. Someday soon, scientists may be flying alongside their experiments on these rockets, reacting to the performance and making real time adjustments to the operation of the experiment. And so I find myself getting ready to undergo two days of “astronaut boot camp” at the NASTAR center. Tomorrow features some hypoxia training and time in a chamber simulating high altitudes (low atmospheric pressure). Wednesday will be a full simulation of a flight on the VSS Enterprise. The final frontier awaits.

The Geysers of Enceladus

Sunday, December 6th, 2009

As Saturn’s south pole slips into its long winter, so does the active southern region of Enceladus, nicknamed the Tiger Stripes, bid farewell to the Sun for the next 15 years. The latest flyby of Enceladus by Cassini - the E-8 flyby - provided the most dramatic and perhaps final views of such clarity of the water vapor geysers emanating from the Tiger Stripes.

The geysers at Enceladus's south polar region.

The geysers at Enceladus's south polar region. Image: NASA/JPL/Space Science Institute.

The vapor is visible in geometries when we look back toward the Sun. In the image below, the Tiger Stripes are seen in relief making use of detailed images and a topographic map created by Paul Schenk at the Lunar and Planetary Institute.

Crevasses in the south polar region of Enceladus.

Crevasses in the south polar region of Enceladus. Image: NASA/JPL/Space Science Institute.

Researchers are still working on models to explain how such a small moon, just a few hundred miles across and therefore an object that would cool off and freeze solid shortly after formation, manages to have a reservoir of liquid water - or at least very warm ice - near its surface. If it is like the active moons of Jupiter, then flexing of the moon by tidal forces from Saturn explain the melting in Enceladus. To maintain tidal heating, Enceladus must be pushed around by gravitational interactions with nearby moons. The problem is that the tidal heating scenario for Enceladus is far less clear than it was for Io, the volcanically hyperactive moon of Jupiter. Stan Peale, a professor at UC Santa Barbara and lead author of the paper that predicted Io’s volcanoes, presented an alternative hypothesis for Enceladus at this year’s DPS meeting. Some of Saturn’s moons have co-orbital satellites: small satellite shards that share an orbit with their larger lunar siblings. Peale and co-author Rick Greenberg suggested that a collision between Enceladus and a co-orbital moon within the relatively recent past (less than 200,000 years ago) could have supplied the necessary heating to drive the geysers to the present epoch.

The LCROSS Crash

Monday, October 12th, 2009

Like many, I was up bright and early last Friday morning to watch the live coverage of the LCROSS impact into the shadows of the Moon’s south polar region. While the complete fizzle of the impact probably should not have been a surprise to me, it was certainly a disappointment to countless people whose expectations had been unreasonably heightened. The purpose of the impact, of course, was not to make a cosmic fireworks display, but to determine the abundance of water ice near the surface in the permanently shadowed craters near the Moon’s south pole. Whether it met that goal will become clear in the days and weeks ahead. Science usually moves forward gradually. Eureka moments usually take some time for to confirm and validate. There are the occasional moments in space exploration, however, when something definitive happens, when there is an EVENT. Given the realities of the 24-hour news cycle, NASA usually seizes on the opportunities provided by these events (the launch of a rocket, the arrival of a spacecraft at another planet) to get some air time with the public. But they risk losing the attention of that public if they don’t learn to be more careful about managing expectations.

Saturn’s Wound-Up C Ring

Thursday, October 8th, 2009

Here’s an article I wrote about one of the coolest discoveries from Cassini to date. Thanks to Emily Lakdawalla at the Planetary Society for posting this.

Annual Planetary Science Conference Kicks Off This Week

Monday, October 5th, 2009

The 41st annual meeting of the Division of Planetary Sciences takes place October 4-9 in Fajardo Puerto Rico. The DPS is a division of the American Astronomical Society. About 700 scientists and students have congregated here in Fajardo to present the latest results from their research on the solar system, ranging from Mercury to the outer solar system and extrasolar planets. Tomorrow we have sessions on the icy satellites of the giant planets, exoplanets, and first results from the Moon Mineralogy Mapper on the Indian Chandrayaan-1 spacecraft. Also on Monday we have an open forum meeting (town hall style, without the Hitler references, though) on the decadal surveys. These surveys, conducted by the National Research Council at the request of NASA, identify the leading scientific questions in the various fields of interest to NASA and become useful roadmaps in the following decade for prioritizing missions and exploration programs.

It looks like it will be a very full week: in addition to being an author on 5 papers here, I’ll be chairing a session, serving on two committees that are meeting here, including DPS’s governing committee, as well as meetings to discuss various scientific collaborations.

Daphnis Wake Shadows

Saturday, June 13th, 2009

As we get closer and closer to Saturn’s equinox in August, the shadows in the rings are revealing dramatic three-dimensional structure at ring edges. Check out this cool picture.

Moon Shadow on the Rings

Monday, May 25th, 2009

Another cool sequence of images of shadows as Saturn approaches its northern spring equinox in just a few months. This time, we see the shadow of the moon Epimetheus moving across the outer A ring. The wide gap is the Encke Gap, about 330 km across, while the narrow gap near the outer edge of the ring is the Keeler Gap (about 30 km across). Epimetheus shares an orbit with the moon Janus. They each orbit Saturn roughly 6 times for every 7 orbits of a particle at the outer edge of the A ring. This orbital resonance between the moons and the ring edge controls the structure and evolution of the edge.

As equinox approaches, the shadows will get longer, and we will start to see shadows cast by warps and distortions within the rings themselves. NASA’s full press release is here.

Click here for the movie

NASA/JPL/SSI

NASA/JPL/SSI

Ring Image: You Can’t Make This Stuff Up

Saturday, May 16th, 2009

Just another stunning example of the beautiful compositions that arise from the combination of Saturn and its rings when you have a spacecraft that can view it from a variety of angles. With Saturn’s equinox approaching, the rings are getting dark, but it still makes a difference whether we are seeing the lit side (currently south) or the unlit side, as in the image below. The opaque B ring is completely dark, while the inner translucent C ring allows light through. Though we are seeing the night side of the planet (as can be seen from the shadow line of the planet on the rings, the Sun is to the left), the southern hemisphere is fairly well illuminated by light reflecting off the southern face of the rings. The northern hemisphere of the planet is much darker because it is only illuminated by light that makes it through the rings. The darkest line on the planet is the equator which gets virtually no light from the rings.

Saturn and its rings
Image Credit: NASA/JPL/SSI