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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
SPACE WEATHER
Current conditions
Solar wind
speed: 550.1 km/sec
density: 1.4 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A8
1830 UT May06
24-hr: B2
0620 UT May06
explanation | more data
Updated: Today at: 2340 UT
Daily Sun: 06 May 10
Sunspot 1069 has a beta-gamma magnetic field that harbors energy for M-class solar flares. Credit: SOHO/MDI
Sunspot number: 77
What is the sunspot number?
Updated 05 May 2010

Spotless Days
Current Stretch: 0 days
2010 total: 21 days (16%)
2009 total: 260 days (71%)
Since 2004: 791 days
Typical Solar Min: 485 days
explanation | more info
Updated 05 May 2010


The Radio Sun
10.7 cm flux: 83 sfu
explanation | more data
Updated 05 May 2010

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 3
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 4.9 nT
Bz: 3.2 nT south
explanation | more data
Updated: Today at 2345 UT
Coronal Holes:
Earth is inside a solar wind stream flowing from the indicated coronal hole. Credit: SOHO Extreme UV Telescope
SPACE WEATHER
NOAA Forecasts
Updated at: 2010 May 06 2201 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
20 %
20 %
CLASS X
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: 2010 May 06 2201 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
05 %
15 %
MINOR
01 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
20 %
MINOR
01 %
05 %
SEVERE
01 %
01 %
What's up in Space
May 6, 2010

NEW AND IMPROVED: Turn your iPhone or iPod Touch into a field-tested global satellite tracker. The Satellite Flybys app now works in all countries.

 

METEORS FROM HALLEY'S COMET: The eta Aquarid meteor shower, caused by dust from Halley's Comet, peaks this year on May 6th and 7th. The shower is strongest over the southern hemisphere, where observers could see more than 30 meteors per hour despite the bright light of a waning half Moon. No matter where you live, the best time to look is during the hours before local sunrise on Friday. [full story]

meteor photos: from John Chumack of Dayton, Ohio; from Thomas Ashcraft near Santa Fe, New Mexico

CINCO DE MAYO BLAST: With May 5th winding down, magnetic fields on the sun wound up and erupted, producing a bright coronal mass ejection (CME). Click on the image to set the cloud in motion:

The eruption came from a spotless region near the sun's southwestern limb. Extreme ultraviolet images from SOHO pinpoint the blast site: movie. The billion-ton cloud is not heading directly for Earth, although it could deliver a glancing blow to our planet's magnetic field on or about May 8th. High-latitude sky watchers should be alert for auroras this weekend.

May 2010 Aurora Gallery
[previous Mays: 2008, 2005, 2004, 2003, 2002] [aurora alerts]

RED RAINBOW: Yesterday in Muncie, Indiana, the sun was just about to set when--"Wow! This red rainbow popped up out of nowhere," reports Mike Hutchinson. "It hung there for about 15 minutes--just enough time to grab my camera and snap a rain-splattered picture."

What made the rainbow red? Simple. The sun itself was red. "The sun was low in the west and strongly reddened by atmospheric scattering and ominous-looking clouds," says Hutchinson.

The real question. according to Hutchinson, is why the inside of the rainbow was so much brighter red than the outside. Atmospheric optics expert Les Cowley has the answer: "A rainbow is not just a set of colored rings, but rather a set of colored disks. The sky inside is bright because raindrops direct light there, too." All rainbows have this property, but it is particularly evident when the sky above the 'bow is dark and cloudy--as it was on May 3rd in Muncie, Indiana.

Got sunset, clouds and rain? Be alert for red rainbows!

more images: from Lauri Kangas of Caledon, Ontario, Canada

 
       
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 6, 2010 there were 1116 potentially hazardous asteroids.
April 2010 Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Mag.
Size
2010 GV23
April 5
2.1 LD
19
12 m
2010 GF7
April 8
2.8 LD
18
30 m
2010 GA6
April 9
1.1 LD
16
27 m
2010 GM23
April 13
3.4 LD
17
47 m
2005 YU55
April 19
5.9 LD
15
185 m
2009 UY19
April 23
8.8 LD
18
87 m
2002 JR100
April 29
8.0 LD
19
65 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 Weather Prediction Center
  The official U.S. government space weather bureau
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.
STEREO
  3D views of the sun from NASA's Solar and Terrestrial Relations Observatory
Daily Sunspot Summaries
  from the NOAA Space Environment Center
Current Solar Images
  from the National Solar Data Analysis Center
Science Central
   
  more links...
   
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