9 X-Class Solar Flares Between September 7 – 19, 2005.

"Why is such a wimpy Solar Minimum cycle, with only a few sunspots, so strong when it comes to making flares?"

- David Hathaway, Ph.D., NASA Solar Physicist

September 23, 2005  Huntsville, Alabama - The sun in our solar system is a big ball of hydrogen and helium gas that's 107 times larger than the Earth. The sun is like a big nuclear fusion reactor that gives light and heat to the planets. Even at 93 million miles from the sun, the temperatures can support life from the icy poles to the hot equator. Scientists who have studied ice cores report that long before the current Industrial Age's emissions of greenhouse gases linked to global warming, there have been many cycles of heating and cooling on the planet. Could it be that the so-called Solar Constant is not so constant? Could cycles in the sun ranging from lots of sunspots and big solar flares to few sunspots and small solar flares have more to do with Earth temperatures than originally thought?

 

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“Planet X” and the Kuiper Belt’s Oddballs, “Santa” and “Easterbunny”

 "Instead of Pluto being a unique object that's difficult to understand (has frozen methane crust), we now see it as part of a family of objects (Xena, Sedna and Easterbunny that also have frozen methane crusts). We can try to understand the entire family, with Pluto being the middle sized member of the three. That's very exciting to us."

- Michael E. Brown, Astronomer  

Planet X, or Xena, or 2003 UB313, illustrated as red in color because it has a surface  of frozen methane similar to Pluto, "Easterbunny," and Sedna. Nine billion miles from the sun,  Xena is 20 to 30 percent larger than Pluto. Illustration by Cal Tech.
Planet X, or Xena, or 2003 UB313, illustrated as red in color because it has a surface of frozen methane similar to Pluto, "Easterbunny," and Sedna. Nine billion miles from the sun, Xena is 20 to 30 percent larger than Pluto. Illustration by Cal Tech.

September 15, 2005  Pasadena, California - A couple of months ago in late July, astronomer Michael Brown and his colleagues at the California Institute of Technology, announced their discovery of "Planet X." It's a big chunk of rock and ice nine billion miles from the sun. It's actually bigger than Pluto - and far beyond Pluto in what is known as the Kuiper Belt that circles our solar system. Now, almost two months later, the International Astronomical Union still has not decided if the exciting discovery should be classified a planet or what it's official name should be.

 

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Dust Devils and “Lemon Rinds” on Mars

Above: Several dust devils caught by NASA's Mars Exploration Rover, Spirit, on July 13, 2005, during its exploration of the Gusev Crater. Below: Mars map, yellow arrow points in far right at the Ma'Adim Vallis dry river channel that empties into the Gusev Crater nera the Elysium Planitia region at the Martian equator. Image credit: NASA/JPL/Cornell.
Above: Several dust devils caught by NASA's Mars Exploration Rover, Spirit, on July 13, 2005, during its exploration of the Gusev Crater. Below: Mars map, yellow arrow points in far right at the Ma'Adim Vallis dry river channel that empties into the Gusev Crater nera the Elysium Planitia region at the Martian equator. Image credit: NASA/JPL/Cornell.


August 24, 2005  Pasadena, California - For twenty months now, the robotic explorer, Spirit, has been exploring the Gusev Crater on Mars, while its twin rover, Opportunity, has been exploring the Meridiana Planum. The two sites are 6,600 miles from each other in the equatorial region.

 

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Deep Impact Spectra: Carbonate, PAHs and Some Amino Precursors in Comet Tempel I

Left: NASA illustration of Deep Impact's impactor just before hitting Comet Tempel I on July 4, 2005. Right: Actual cratered surface of Comet Tempel I ninety seconds before the impactor smashed into the fluffy ice at 23,000 mph. Photograph courtesy NASA.
Above: NASA illustration of Deep Impact's impactor just before hitting Comet Tempel I on July 4, 2005. Below: Actual cratered surface of Comet Tempel I ninety seconds before the impactor smashed into the fluffy ice at 23,000 mph. Photograph courtesy NASA.

Moment of impact on potato-shaped Comet Tempel I at 10:52 p.m. PDT, July 3, 2005 / 1:52 a.m. EDT, July 4, 2005. Image by NASA, ESA, Johns Hopkins University Applied Physics Lab.
Moment of impact on potato-shaped Comet Tempel I at 10:52 p.m. PDT, July 3, 2005 / 1:52 a.m. EDT, July 4, 2005. Image by NASA, ESA, Johns Hopkins University Applied Physics Lab.

August 12, 2005  College Park, Maryland - This week geologists, chemists, physicists and planetary scientists from around the world gathered at the 9th International Asteroids, Comets and Meteors Conference in Brazil. One of the presentations was by Carey Michael Lisse, Ph.D., Prof. of Physics at the University of Maryland, and member of the Deep Impact Science Team. Dr. Lisse is Principal Investigator of Deep Impact spectral results from the Chandra X-Ray and Spitzer telescopes.

 

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Astronomers Report 10th Planet Far Beyond Pluto

"It is bigger than Pluto!!!"

Astronomer Michael Brown of Cal Tech wrote at his website.

"And it's not planetoid 2003EL61 announced yesterday,"

also by Brown's group.

Tenth planet, 2003UB313, photographed above in the white circle by Palomar Observatory astronomers lead by Michael Brown, Ph.D., from CalTech, was discovered for the first time on January 8, 2005, at Palomar Observatory's Samuel Oschin telescope which took this image.
Tenth planet, 2003UB313, photographed above in the white circle by Palomar Observatory astronomers lead by Michael Brown, Ph.D., from CalTech, was discovered for the first time on January 8, 2005, at Palomar Observatory's Samuel Oschin telescope which took this image.

July 30, 2005 Pasadena, California - Brown had hoped to confirm the object's size before public disclosure. But late last night at NASA's Jet Propulsion Laboratory in California, he made a rushed announcement after his astronomy team, including Chad Trujillo (Gemini Observatory), and David Rabinowitz (Yale University), learned that a hacker had broken into their data with the idea of making "the tenth planet" discovery public first. Beyond 2003UB313, it has no other name yet, but a "more melodious name" was submitted to the International Astronomical Union in Paris for approval. It might have "Lila" in it, since Michael Brown has a 3-week-old daughter named Lila.

 

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First Data from Deep Impact Crash Into Comet Tempel I

This image shows the view from Deep Impact's flyby spacecraft as it turned back to look at comet Tempel 1. Fifty minutes earlier, the spacecraft's probe had been run over by the comet. That collision kicked up plumes of ejected material, seen here streaming away from the back side of the comet. This image was taken by the flyby craft's high-resolution camera. Image credit: NASA/JPL-Caltech/UMD.
This image shows the view from Deep Impact's flyby spacecraft as it turned back to look at comet Tempel 1. Fifty minutes earlier, the spacecraft's probe had been run over by the comet. That collision kicked up plumes of ejected material, seen here streaming away from the back side of the comet. This image was taken by the flyby craft's high-resolution camera. Image credit: NASA/JPL-Caltech/UMD.

July 10, 2005  Austin, Texas - Astronomer Anita Cochran has been working at the University of Texas since 1982. Now she is a senior research scientist and Assistant Director of the McDonald Observatory in Austin. She and several hundred scientists around the world are helping to analyze the spectral data from the Deep Impact crash with Comet Tempel I on July 3 to 4, 2005. That night, Dr. Cochran was in Hawaii at the Kech I telescope, the largest in the world, watching to see if a light flare at the moment the impactor hit the very dim magnitude 11 comet could be seen.

 

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July 3-4, 2005: NASA “Deep Impact” Spacecraft to Blast Hole in Comet Temple I

Top: Deep Impact lifted off January 12, 2005, at 1:47:08.574 PM ET from pad 17-B at Cape Canaveral Air Force Station, Florida, bound for Comet Tempel 1. Image courtesy NASA. Bottom: Arrow points to Comet Tempel 1 photographed on December 11, 2004, by Observatoriode Begues, Spain. The plan is to create a crater by impacting the icy snowball on July 3-4, 2005, to see what it's made of. Image from Observatorio de Begues.
Top: Deep Impact lifted off January 12, 2005, at 1:47:08.574 PM ET from pad 17-B at Cape Canaveral Air Force Station, Florida, bound for Comet Tempel 1. Image courtesy NASA. Bottom: Arrow points to Comet Tempel 1 photographed on December 11, 2004, by Observatoriode Begues, Spain. The plan is to create a crater by impacting the icy snowball on July 3-4, 2005, to see what it's made of. Image from Observatorio de Begues.



 Schedule of Impact Events

- NASA TV coverage: Begins July 3, 8:30 p.m., Pacific Daylight Time, PDTFor NASA TV, click on: http://www.nasa.gov/multimedia/nasatv/index.html

- Expected time of impact with comet:
July 3, 10:52 p.m. PDT
11:52 p.m. MDT
July 4,  12:52 a.m. CDT
1:52 a.m. EDT

- NASA Post-impact briefing: July 4, 1 a.m. PDT
- NASA Post-impact press conference: July 4, 11 a.m. PDT

 

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A Harmless Virus Kills Cancer Cells

June 24, 2005   Hershey, Pennsylvania - A scientist at Penn State College of Medicine in Pennsylvania announced at a recent meeting of the American Society for Virology that his lab has killed cancer cells with a virus called "adeno-associated virus type 2," or AAV-2.

The AAV-2 virus has killed a variety of cancer cells in Petrie dishes investigated by Dr. Craig Meyers, Prof. of Microbiology and Immunology at Penn State College of Medicine in Hershey, Pennsylvania. This cancer-killing virus infects 80% of the human population. If the AAV-2 virus is so prevalent, why isn't it killing cancers all the time in people? I asked Dr. Meyers what activates the virus to kill cancer cells in his laboratory?

 

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Mars Express Orbiter Finally Turns On Deep Ground-Penetrating Radar

Mars Express Orbiter with MARSIS radar antennae unfurled in orbit around Mars. Illustration by ESA.
Mars Express Orbiter with MARSIS radar antennae unfurled in orbit around Mars. Illustration by ESA.


June 23, 2005   Darmstadt, Germany - I learned something amazing today from the Mars Express Orbiter Spacecraft Operations Manager. He is Michel Denis based at the European Space Agency's office in Darmstadt, Germany. I was getting an update about the plans for the deep ground-penetrating radar on ESA's Mars Express Orbiter which was turned on for the first time at 3 p.m. Pacific. The amazing fact I learned was that a month ago on May 7th, the Mars Express Orbiter and NASA's two spacecraft, the Odyssey and the Mars Global Surveyor ­ could have collided!

 

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EARTHFILES