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<<back forward>> -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
Current conditions
Solar wind
speed: 392.0 km/sec
density: 1.2 protons/cm3
explanation | more data
Updated: Today at 2245 UT
X-ray Solar Flares
6-hr max: A2
1820 UT May29
24-hr: A2
1820 UT May29
explanation | more data
Updated: Today at: 2245 UT
Daily Sun: 29 May 07
A new, small sunspot is emerging at the sun's eastern limb. Credit: SOHO/MDI
Sunspot number: 0
What is the sunspot number?
Updated 28 May 2007
Far side of the Sun:
This holographic image reveals no large spots on the farside of the sun. Image credit: SOHO/MDI
Planetary K-index
Now: Kp= 1 Quiet
24-hr max: Kp= 2
explanation | more data
Current Auroral Oval:
Europe, Antarctica, USA
Interplanetary Mag. Field
Btotal: 2.6 nT
Bz: 2.3 nT south
explanation | more data
Updated:Today at 2246 UT
Coronal Holes:
A solar wind stream flowing from the indicated coronal hole should reach Earth on or about June 2nd. Credit: SOHO Extreme Ultraviolet Telescope
NOAA Forecasts
Updated at: 2007 May 29 2203 UTC
0-24 hr
24-48 hr
01 %
01 %
01 %
01 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2007 May 29 2203 UTC
0-24 hr
24-48 hr
15 %
15 %
01 %
01 %
01 %
01 %
High latitudes
0-24 hr
24-48 hr
15 %
15 %
05 %
05 %
01 %
01 %
What's up in Space
May 29, 2007
He already has a neck tie. This year give Dad something truly heavenly for Father's Day: SpaceWeather PHONE.

STORM WARNINGS: Astronauts can breathe a little easier. A scientist using the Solar and Heliospheric Observatory (SOHO) has found a way to predict dangerous solar radiation storms. The new alert system offers as much as one hour advance warning, giving astronauts on EVA extra time to seek shelter and avoid radiation sickness. Get the full story from Science@NASA.

DARK FILAMENT: Today, astronomers with solar telescopes are monitoring a dark filament on the sun. This picture comes from the observing team J. Raschack, A. Royer and John Stetson of South Portland, Maine:

Filaments are ribbon-shaped clouds of hydrogen held above the sun's surface by magnetic fields. The appear dark because they are slightly cooler than the surface of the sun below. In reality, however, they are hot and bright. If you snipped off a solar filament and placed it in the night sky far from the sun, it would shine like a full moon. Imagine that!

FIND THE MOON: On May 23rd, when photographer Guillaume Bertrand looked at the sky over Saint Laurent sur Sèvre, France, he was transported thousands of light years away. "The scene reminded me of a star-forming region in the Small Magnellanic Cloud," he says. (continued below)

Photo details: Canon 300D

But when he took the picture and examined it closely, he found no stars--only the Moon! "Can you find it?" he asks. Click here to search.

When you locate the Moon, note how its surface brightness compares favorably to that of bright white clouds. That's why, contrary to popular belief, the Moon is so easy to see during the day.

more images: from Pete Lawrence of Selsey, West Sussex, UK; from Günther Strauch of Borken, NRW, Germay; from Anthony Ayiomamitis of Athens, Greece; from Ralph Nevins of Ottawa, Ontario

Near-Earth Asteroids
Potentially Hazardous Asteroids (PHAs) are space rocks larger than approximately 100m that can come closer to Earth than 0.05 AU. None of the known PHAs is on a collision course with our planet, although astronomers are finding new ones all the time.
On May 29, 2007 there were 863 potentially hazardous asteroids.
May 2007 Earth-asteroid encounters:
Miss Distance
1862 Apollo
May 8
72 LD
2.4 km
2007 JD
May 11
12 LD
100 m
2007 JZ2
May 14
7.0 LD
30 m
Notes: LD means "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU. MAG is the visual magnitude of the asteroid on the date of closest approach.
Essential Links
NOAA Space Environment Center
  The official U.S. government bureau for real-time monitoring of solar and geophysical events, research in solar-terrestrial physics, and forecasting solar and geophysical disturbances.
Atmospheric Optics
  The first place to look for information about sundogs, pillars, rainbows and related phenomena.
Solar and Heliospheric Observatory
  Realtime and archival images of the Sun from SOHO.
Daily Sunspot Summaries
  From the NOAA Space Environment Center
Current Solar Images
  from the National Solar Data Analysis Center
  more links...
©2007, -- This site is penned daily by Dr. Tony Phillips.
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