Posted on by Nancy Atkinson

Famous People Wandering the Halls of AAS

Walking the halls of the AAS meetings we found Galileo Galilei, who actually looks pretty good for being 440 years old. He had a briefing with officials from the inquisition (the media) and said that he has just returned from Rome on his book tour, promoting Sidereus Nuncius (Starry Messenger). But here, he met up with another author, Dava Sobel, who wrote “Galileo’s Daughter,” and is in St. Louis to speak at a public lecture in conjunction with the AAS meeting.

The International Year of Astronomy (IYA) which celebrates 400 years since Galileo looked through his telescope, is being promoted heavily here at the AAS meeting, which includes educational workshops and symposiums sponsored by the Astronomical Society of the Pacific, highlighting special educational programs specifically created for IYA.

Speaking of education, Galileo says that being a professor is difficult. “The work is hard and the pay is terrible,” he said. “I’m looking to invent something here during the next year which might give me some fame.”

Galileo was played by Mark Thompson, an impersonator who actually is an amateur astronomer. Although he kind of transited back and forth to the present and the past, he said he’s currently living in IYA time, which means he hasn’t yet built his telescope. That will happen coming up next year.

More information about Mark Thompson as Galileo.

Posted on by Nancy Atkinson

How To Weigh a Black Hole: Just Look At Its Galaxy

Traveling to distant locations, like Andromeda, could have interesting consequences. Credit: NASA

My father was a rancher, who had the uncanny ability to accurately estimate the weight of each animal in his herd of cattle simply by looking at them. Today, at the American Astronomical Society meeting in St. Louis, astronomers announced a new, simple way of determining masses of super-massive black holes by just looking at images of galaxies. Dr. Marc Seigar from the University of Arkansas at Little Rock has been studying images available at the Hubble Space Telescope archive site, and looking at the how tightly the galaxy’s arms wrap around itself in relation to the size of the galaxy’s super-massive black hole. “This provides a much simpler method of determining black hole mass,” said Seigar. “You just need an image of a galaxy and you can measure the tightness of the spiral structure. This can easily be applied to distant galaxies, up to 8 billion light-years away.”

Usually astronomers determine masses of super-massive black holes by looking at how fast the stars are moving in the central regions of the galaxies. But that method only works for nearby galaxies. Astronomers have been looking for a new method for galaxies that are father away. This new inexpensive method can use already-existing images, as Seigar has used from the Hubble Site.

Seigar and his team looked at photographs of 27 spiral galaxies including the Milky Way and the Andromeda Galaxy. They observed galaxies with the smallest black holes had spiral arms with angles up to 43 degrees between the arms and the central bulge. Those with the biggest black holes had spiral arms at angles of only 7 degrees between the arms and the bulge.

Seigar said its also possible that the main factor in determining the mass of a super massive black hole is the amount of central concentration of dark matter in a galaxy. “We think dark matter is driving most of the relationships between black holes and their galaxies,” he said. “The masses of these black holes can be determined indirectly from the characteristics of the light emitted from in falling material.”

Seigar will continue to use this method to verify his findings, as well as looking at other aspects. “We have to determine if the relationship between spiral arms and black hole mass evolves over time.”

Source: AAS press conference

Posted on by Nancy Atkinson

Phoenix Digs on Mars

Phoenix’s first dig in the Martian soil. Image credit: NASA/JPL-Caltech/ University of Arizona

The Phoenix lander used its robotic arm scoop to dig up soil on Mars surface for the first time during its activities during its seventh day on the Red Planet. The image above shows the hole dug by Phoenix, and below is a picture of the scoop itself, with the Martian soil inside.

The plan was to do a test dig and then dump the soil. If that works correctly, then Phoenix will dig another scoop and bring it to the TEGA device on board the lander, the Thermal and Evolved Gas Analyzer, a “furnace” and mass spectrometer instrument that scientists will use to analyze Martian ice and soil samples.

During its previous day’s activities on Sol 6, Phoenix reached out and touched Mars with its robotic arm scoop to make an impression on the Martian surface. And please, no conspiracy theories here, but the impression looks like a footprint, and the Phoenix scientists have dubbed the mark “Yeti.” Touching the surface was a preliminary test for the robotic arm and scoop, to make sure everything was working correctly before making the first scoop.

However, the TEGA device has experienced an intermittent short circuit, and the TEGA scientists are developing a procedure to work around the problem. But Phoenix can still deliver the soil sample to TEGA, and the sample can be held there until the device is working.

Original News Source: Phoenix

Posted on by Nancy Atkinson

Launchpad Damaged During Saturday’s Shuttle Launch

Debris falls into the water following Discovery’s launch on Saturday. Images from CBS Space Place.

The launchpad at Kennedy Space Center was damaged during Saturday’s space shuttle launch. Pictures taken during Discovery’s launch show debris raining down into the waterway just behind launchpad 39A. Additional images show debris that appears to be broken concrete littering a nearby road as well as damaged and buckled concrete on one side of the launchpad. CBS News’ Bill Harwood reported that the damage to the pad occured on the north side of the “flame trench” wall. The trench is used to divert exhaust from the shuttle’s solid rocket boosters.


The damage is “unusual,” Harwood quoted NASA spokesman Bill Johnson, who verified the damage was serious and tomorrow (Monday) a full report on the incident will be issued. Harwood also reported that a NASA manager said part of the pad’s base was repaired following a previous launch, but possibly something was either missed or not repaired correctly.

The debris appears to come from the lauchpad itself, and not the shuttle. And whether any of the debris hit the shuttle is currently unknown. The astronauts on board Discovery have not yet been able to conduct the usual inspection of the shuttle nose cap and wing leading edge panels because the 50-foot-long boom equipped with laser scanners and high-resolution cameras was unable to fit into the shuttle’s payload bay due to the large size of the Japanese Kibo laboratory that Discovery is bringing to the International Space Station. The last shuttle crew left the orbiter boom sensor system at the ISS, and the crew of Discovery will retrieve it while docked to the station. ISS crew members will take high resolution pictures of the shuttle as it approaches the station on Monday. Docking is scheduled about 2 pm EDT.

Both launchpads at KSC, 39A and 39B were originally built for the Apollo spacecraft/Saturn rockets and were modified for the space shuttles. During launches the pads must withstand both high heat and extreme pressure.

Original News Source: CBS Space Place

Posted on by Nancy Atkinson

Get Ready for High-Energy GLAST

It’s not hard to grab someone’s attention when you mention the words “super massive black holes,” “gamma ray bursts,” “cosmic rays,” and ” dark matter.” NASA’s next space telescope will attempt to grab data about some of these high-energy objects in our universe to help us understand their mysteries. GLAST, the Gamma-ray Large Area Space Telescope will use its instruments to study those objects that generate gamma-ray radiation, the most energetic form of radiation we know of, billions of times more energetic than the type of light visible to our eyes. Liftoff for GLAST is set for Thursday, June 5, and the launch window extends from 11:45 a.m. to 1:40 p.m. EDT.

GLAST will reside in a circular, low Earth orbit of about 560 km ( 350 miles ). This orbit was chosen to minimize the effects of charged particles that surround Earth, and which would create additional unwanted background signals in the detectors. At that altitude, the observatory will circle Earth every 90 minutes. In sky-survey mode, GLAST will be able to view the entire sky in just two orbits, or about 3 hours.

The instruments on the GLAST mission are the Large Area Telescope (LAT) and the GLAST Burst Monitor. Lat has a tracker for gamma-ray detection and direction measurement, and can also measure the energies of the rays. The GBM will have two types of scintillators mounted on the sides of the spacecraft to detect electromagnetic waves.

Phil over at Bad Astronomy has a couple of very nice (and fun) videos with info about GLAST (one starring Phil himself), but these are the major goals of GLAST:

• Explore the most extreme environments in the Universe, where nature harnesses energies far beyond anything possible on Earth.
• Search for signs of new laws of physics and what composes the mysterious Dark Matter.
• Explain how black holes accelerate immense jets of material to nearly light speed.
• Help crack the mysteries of the stupendously powerful explosions known as gamma-ray bursts.
• Answer long-standing questions across a broad range of topics, including solar flares, pulsars and the origin of cosmic rays.

GLAST should provide some very interesting data about these spectacular and remarkable objects in our universe, and will create a full-sky map of gamma radiation.

Kapla GLAST!

Source: GLAST site

Posted on by Nancy Atkinson

It Really Looks Like Ice on Mars

Take a look at this image sent back from the Phoenix lander. On Friday, Phoenix scientist Ray Arvidson said there may be ice directly under the Phoenix lander, exposed in the blast zone by the retrorockets used for Phoenix’s soft landing. Friday’s image showed a small portion of the exposed area that looks brighter and smoother than the surrounding soil. On Saturday, Sol 5 for Phoenix on Mars, a new image shows a greater portion of the area under the lander. Scientists say the abundance of excavated smooth and level surfaces adds evidence to a hypothesis that the underlying material is an ice table covered by a thin blanket of soil. This is just what the Phoenix mission was hoping to find, and how incredible to land directly over your goal.

The bright-looking surface material in the center, where the image is partly overexposed, may not be inherently brighter than the foreground material in shadow. But the scientists are calling this area “Holy Cow.” Reportedly (via Emily at the Planetary Society) that’s exactly the phrase exclaimed when this image was returned. More pictures of this feature will be imaged using different exposures in an effort to determine if this really is ice.

The other interesting aspect of this image is that the retrorocket nozzles are visible right at the top of the image.

We’ll keep you posted when there’s more information and data available on the area under the lander.

Sources: Phoenix, Planetary Blog

Posted on by Nancy Atkinson

Phoenix Spies Possible Ice; TEGA Short Circuit Likely

Scientists from the Phoenix mission say the lander may have exposed ice just beneath Mars surface when soil was blown away as the spacecraft landed last Sunday, May 25. The possible ice appears in an image the robotic arm camera took underneath the lander, near a footpad. The robotic arm was moved so the camera could peer beneath the lander to make sure Phoenix’s footing is secure before any digging operations start. In the top center of the image above is the area in question.


“We could very well be seeing rock, or we could be seeing exposed ice in the retrorocket blast zone,” said Ray Arvidson of Washington University, St. Louis, Mo., co-investigator for the robotic arm. “We’ll test the two ideas by getting more data, including color data, from the robotic arm camera. We think that if the hard features are ice, they will become brighter because atmospheric water vapor will collect as new frost on the ice.”

Arvidson said in today’s Phoenix press conference that Phoenix will provide full confirmation of what lies below the lander when it excavates and analyzes layers in the nearby landscape.

One bad piece of news for the nearly flawless mission, however. The Thermal and Evolved Gas Analyzer (TEGA) instrument that “bakes and sniffs” samples to identify the chemical make-up of the soil might have a short circuit. In a test conducted on Thursday, the instrument exhibited electrical behavior consistent with an intermittent short circuit in the spectrometer portion. The team is currently developing diagnostic steps that will be sent to the lander in the next few days. TEGA includes a calorimeter that tracks how much heat is needed to melt or vaporize substances in a sample, plus a mass spectrometer to examine vapors driven off by the heat.

“We have developed a strategy to gain a better understanding of this behavior, and we have identified workarounds for some of the possibilities,” said William Boynton of the University of Arizona, Tucson, lead scientist for the instrument.

The latest data from the Canadian Space Agency’s weather station shows another sunny day at the Phoenix landing site with temperatures holding at minus 30 degrees Celsius (minus 22 degrees Fahrenheit) as the sol’s high, and a low of minus 80 degrees Celsius (minus 112 degrees Fahrenheit). The LIDAR instrument was activated for a 15-minute period just before noon local Mars time, and showed increasing dust in the atmosphere.

If you’d like to download this Phoenix weather widget for your desktop, check HERE.

“This is the first time LIDAR technology has been used on the surface of another planet,” said the meteorological station’s chief engineer, Mike Daly, from MDA in Brampton, Canada. “The team is elated that we are getting such interesting data about the dust dynamics in the atmosphere.” HERE is an animation of the LIDAR

The mission passed a “safe to proceed” review on Thursday evening, meeting criteria to proceed with evaluating and using the science instruments.

“We’re still in the process of checking out our instruments,” Phoenix project scientist Leslie Tamppari of JPL said. “The process is designed to be very flexible, to respond to discoveries and issues that come up every day. We’re in the process of taking images and getting color information that will help us understand soil properties. This will help us understand where best to first touch the soil and then where and how best to dig.”

And finally, here’s the latest version of Phoenix’s panorama, compiled of images from Phoenix’s Stereo Surface Imager (SSI) camera that were taken on sols 1 and 3. The top portion has been stretched eight fold to show details of features in the background. Phoenix’s parachute, backshell, heatshield, and impact site can also be seen.

Posted on by Nancy Atkinson

Lunar Art

NASA recently invited college and high school students to submit artwork for a contest on the theme “Life and Work on the Moon.” NASA encouraged students to form inter-disciplinary teams, so that art and humanities students could collaborate with science and engineering students, “to produce the most well-informed art work possible.” NASA just announced the winners of the contest. The first place submission is above, and is called Traffic Jam, by Justin Burns, a sophomore at the University of Memphis.

Why would an institution like NASA sponsor an art contest? “Once humans establish a presence on the Moon, the arts will be a desired facet of life there, as they are here on Earth,” says NASA’s art contest web page. “It is our intention to provoke non-science and engineering students to think about the science and engineering required to achieve the conditions suitable for humans to live and work on the moon. It is also our intention to help the science and engineering communities appreciate valuable contributions from other communities, particularly the arts.”

See more of the winners below:


2nd Place: “A Busy Day on the Moon” by Johnathan Culpepper, Senior, Medgar Evers College

3rd Place: “Enabling Exploration” by Lann Brumlilk and Corey DiRutigliano, Graduate Students, University of Cincinnati

4th Place: “Perseid Meteor Shower on a Newly Terra-formed Moon” by Ellen Ladwig, Senior, University of Missouri, St. Louis

High School Division: Tie for 1st Place:

“Pole Colony” by Asa Shultz, High School Senior, Home-schooled, Covenant Academy

“To the Moon and Beyond” by William Zhang, High School Sophomore, Skoldberg Art Academy

Source: NASA Art Contest page

Posted on by Nancy Atkinson

Meet Us in St. Louis

I’ll be attending the American Astronomical Society/Astronomy Society of the Pacific Meeting in St. Louis for the next few days, starting Saturday, May 31 with some educational workshops and symposiums, and then Monday-Thursday is the AAS conference. This will be my first conference as a journalist, and I’m looking forward to being overwhelmed and star-struck.

If you’ll be there, or if you happen to be in the St. Louis area, we are planning a “Astroblogger Meet-Up” on Tuesday, June 3 at 7:00 pm at KitchenK bar & restaurant. The big names who will be there: Pamela Gay from Astronomy Cast and Star Stryder, Phil Plait from Bad Astronomy, Chris Lintott from Chris Lintott’s Universe and Galaxy Zoo, and Tammy Plotner and me (Nancy) from Universe Today, and more. Please join us if you can!

If you can’t be in St. Louis, we’ll try to bring the conference to you via reports and articles here on UT and liveblogging on Astronomy Cast Live.

Posted on by Nancy Atkinson

Phoenix News & Weather; Full Panorama Complete, Arm “Raring To Go”

Phoenix’s Surface Stereo Imager (SSI) has finished its initial survey of the area surrounding the Phoenix lander, and returned the images to Earth for completion of the first panorama, seen above. “The panorama takes your around the entire scene,” said Phoenix Principal Investigator Peter Smith. “We see this “hummocky” terrain, with troughs in between the hummocks. In the background we can see the backshell and parachute.” Also visible are disturbances in the soil caused by the landing. And one of the most important aspects of the image shows the robotic arm now up and off the lander, with its scoop in the ready position. Flight Software Lead Matt Robinson reported, “The arm is busted loose now and is raring to go!”

Robinson said the arm is now unstowed out of all its launch restraints, and it required movement from all four of the joints to break loose of the bio-barrier that covered the arm during its journey from Earth. However, it will probably be next week before any digging is done with the arm. The team will first need to determine the stability of the lander. The camera on the end of the arm will look up under the lander to make sure everything is stable, and that each footpad is secure.


Smith said the rocks in the area are fist size, and there are ample places between the rocks to dig down to look for the ice layer thought to lie beneath the Martian surface. Data from the Odyssey spacecraft has indicated water in the form of ice lies beneath the Mars arctic region. Smith added that smaller rocks can be moved by robotic arm, if necessary, to get a good place to dig.

As customary, the science team has begun naming the rocks in the area to help distinguish them, and are using themes from fairy tale characters from Humpty Dumpty, The Legend of sleepy hollow, and Alice in Wonderland.


The “scoop” on the end of Phoenix’s robotic arm is now up and off the lander.

Science team is looking at the patterns in the rocks, and patterns in how they are distributed around the hummocks and troughs. “We do not have a full spectral analysis of any of the rocks, so its early to say anything about their composition,” Smith said. “That’s high on our list of things to do.” He added that the 12 spectroscopic filters on the SSI should be able to tell us if they are the same as the five other locations we’ve studied on Mars. He also offered a couple of clues about the rocks: Many are flat like paving stones, which may be a clue to their origin, and the rocks seem to be brighter than the surface rather than darker.

The SSI can also be used to create stereoscopic images that allow them to get elevation information. Additionally, the camera on the end of the arm, while not stereoscopic, can take one image and then be moved slightly to create stereoscopic images. The suite of science instruments on the arm also includes a microscopic imager with resolution 6 times better than the MER instruments.

Asked how he thought the mission has been going so far, Phoenix project manager Barry Goldstein said, “We’ve exceeded even our optimistic goals.”

And now, here’s the latest weather report from the Phoenix landing site:

Quicktime hi-res movie of the terrain to the northwest of the Phoenix lander.

Link for Mars Weather Widget — Get Mars Weather on your desktop!
Image sources: Phoenix Gallery