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<<back forward>> -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
Solar wind
speed: 370.1 km/sec
density: 5.4 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: B7
2201 UT Dec03
24-hr: C1
0628 UT Dec03
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 03 Dec 15
Both of these sunspots are in decay, and the face of the sun is almost blank. . Credit: SDO/HMI

Sunspot number: 26
What is the sunspot number?
Updated 03 Dec 2015

Spotless Days
Current Stretch: 0 days
2015 total: 0 days (0%)

2014 total: 1 day (<1%)
2013 total: 0 days (0%)
2012 total: 0 days (0%)
2011 total: 2 days (<1%)
2010 total: 51 days (14%)
2009 total: 260 days (71%)

Updated 03 Dec 2015

The Radio Sun
10.7 cm flux: 95 sfu
explanation | more data
Updated 03 Dec 2015

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 2
explanation | more data
Interplanetary Mag. Field
Btotal: 5.6 nT
Bz: 1.2 nT south
explanation | more data
Updated: Today at 2348 UT
Coronal Holes: 03 Dec 15

Solar wind flowing from this broad coronal hole could reach Earth as early as Dec. 7th. Credit: SDO/AIA.
Noctilucent Clouds The southern season for noctilucent clouds is about to begin. Monitor the daily daisies, below, from NASA's AIM spacecraft for the first wisps of electric blue above Antarctica.
Switch view: Ross Ice Shelf, Antarctic Peninsula, East Antarctica, Polar
Updated at: 12-03-2015 17:55:03
NOAA Forecasts
Updated at: 2015 Dec 03 2200 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: 2015 Dec 03 2200 UTC
0-24 hr
24-48 hr
15 %
15 %
05 %
05 %
01 %
01 %
High latitudes
0-24 hr
24-48 hr
20 %
20 %
30 %
25 %
20 %
20 %
Thursday, Dec. 3, 2015
What's up in space

Marianne's Heaven On Earth Aurora Chaser Tours invites you to join them in their quest to find and photograph the Aurora Borealis. Experience the winter wonderland in the Tromsø Area.

Chase the Light Tours

VAST HOLE OPENS IN SUN'S ATMOSPHERE: A vast hole in the sun's atmosphere--a "coronal hole"--has opened up in the sun's northern hemisphere, and it is spewing a broad stream of solar wind into space. NASA's Solar Dynamics Observatory photographed the coronal hole during the early hours of Dec. 3rd:

Coronal holes are places where the sun's magnetic field opens up and allows solar wind to escape. Hot plasma flows outward at speeds exceeding a million mph. In the extreme-ultraviolet image, above, the boundaries of the coronal hole are traced by dashed lines; arrows indicate the escape of hot plasma.

Solar wind flowing from this coronal hole will reach Earth beginning ~Dec. 6th, and our solar wind environment will be dominated the stream for days after first contact. High-latitude sky watchers should be alert for auroras. Aurora alerts: text or voice

Realtime Aurora Photo Gallery

INTERPLANETARY SPACECRAFT TO BUZZ EARTH ON DEC. 3RD: Japan's Hayabusa 2 spacecraft, on a six year mission to catch and sample an asteroid, will fly past Earth on Dec. 3rd. Earth's gravity will slingshot the spacecraft toward its target, 162173 Ryugu, which Hayabusa 2 is expected to reach in July 2018. This animation from JAXA (the Japanese space agency) previews the flyby:

Many readers have never heard of Hayabusa 2. It is an amazing mission. After the spacecraft reaches Ryugu in 2018, it will orbit the asteroid for a year and a half. During that time, Hayabusa 2 will deploy four landers and drop a copper impactor to blow a hole in the asteroid's side. Hayabusa 2 itself will touch down on the asteroid, briefly, at least once to collect samples excavated by the impactor. In Dec. 2019, the spacecraft will leave the asteroid and use its ion engines to return to Earth, carrying precious samples of Ryugu. Ambitious? Yes. But if Hayabusa 2 completes even a fraction if its mission, it will be a success.

The spacecraft is small (mass: 590 kg, dimensions: 2 x 1.6 x 1.25 meters), so when it flies by Earth it will not be very bright--definitely invisible to the naked eye. "I expect it will be about 13th magnitude at best when it appears low in the west-northwest sky after evening twilight ends across the USA," says Richard Alan Keen of the University of Colorado, who observed a similar flyby of the Rosetta spacecraft in 2005, and bases his brightness estimate on that. Another experienced observer, Bill Gray of Project Pluto, estimates that the magnitude could reach +11. Either way, it is still very dim.

Observers with telescopes in Alaska, Hawaii and Japan are favored with the best views of the tiny spacecraft as it passes over the Pacific during closest approach. Ephemerides for specific locations may be obtained on the JPL HORIZONS website. Additional charts and a ground track are available in Japanese at this URL.

This just in: On Nov. 26th, at a distance of 3 million km, Hayabusa 2 took this picture of the Earth-Moon system:

According to JAXA analysts, you can see the Australian continent on the right, the Eurasian continent covered by clouds on the left, and the white vertical areas between them are clouds over the equator. Better views are expected as Hayabasa approaches Earth in the hours ahead.

Realtime Space Weather Photo Gallery

Realtime Comet Photo Gallery

Realtime Noctilucent Cloud Photo Gallery

Realtime Meteor Photo Gallery

  All Sky Fireball Network
Every night, a network of NASA all-sky cameras scans the skies above the United States for meteoritic fireballs. Automated software maintained by NASA's Meteoroid Environment Office calculates their orbits, velocity, penetration depth in Earth's atmosphere and many other characteristics. Daily results are presented here on

On Dec. 3, 2015, the network reported 45 fireballs.
(38 sporadics, 3 Geminids, 2 November omega Orionids, 1 Quadrantid, 1 Puppids-Velid)

In this diagram of the inner solar system, all of the fireball orbits intersect at a single point--Earth. The orbits are color-coded by velocity, from slow (red) to fast (blue). [Larger image] [movies]

  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 December 3, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Miss Distance
2003 EB50
Nov 29
48.8 LD
2.2 km
2007 BG29
Dec 1
54.1 LD
1.1 km
2015 WZ12
Dec 1
8.8 LD
22 m
2015 WA13
Dec 6
7.5 LD
26 m
2015 WF13
Dec 7
10.8 LD
86 m
2015 VZ145
Dec 8
9.2 LD
80 m
2015 XC
Dec 8
3.3 LD
39 m
1998 WT24
Dec 11
10.9 LD
1.1 km
2011 YD29
Dec 24
9.7 LD
24 m
2003 SD220
Dec 24
28.4 LD
1.8 km
2008 CM
Dec 29
22.8 LD
1.5 km
2004 MQ1
Jan 2
55.4 LD
1.1 km
1999 JV6
Jan 6
12.6 LD
410 m
1685 Toro
Jan 22
60.9 LD
1.7 km
2001 XR1
Jan 23
74.4 LD
1.5 km
2015 VC2
Jan 28
5.8 LD
15 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.
  Cosmic Rays in the Atmosphere
Situation Report -- Oct. 30, 2015 Stratospheric Radiation (+37o N)
Cosmic ray levels are elevated (+6.1% above the Space Age median). The trend is flat. Cosmic ray levels have increased +0% in the past month.
Sept. 06: 4.14 uSv/hr (414 uRad/hr)
Sept. 12: 4.09 uSv/hr (409 uRad/hr)
Sept. 23: 4.12 uSv/hr (412 uRad/hr)
Sept. 25: 4.16 uSv/hr (416 uRad/hr)
Sept. 27: 4.13 uSv/hr (413 uRad/hr)
Oct. 11: 4.02 uSv/hr (402 uRad/hr)
Oct. 22: 4.11 uSv/hr (411 uRad/hr)
These measurements are based on regular space weather balloon flights: learn more.

Approximately once a week, and the students of Earth to Sky Calculus fly "space weather balloons" to the stratosphere over California. These balloons are equipped with radiation sensors that detect cosmic rays, a surprisingly "down to Earth" form of space weather. Cosmic rays can seed clouds, trigger lightning, and penetrate commercial airplanes. Our measurements show that someone flying back and forth across the continental USA, just once, can absorb as much ionizing radiation as 2 to 5 dental X-rays. Here is the data from our latest flight, Oct. 22nd:

Radiation levels peak at the entrance to the stratosphere in a broad region called the "Pfotzer Maximum." This peak is named after physicist George Pfotzer who discovered it using balloons and Geiger tubes in the 1930s. Radiation levels there are more than 80x sea level.

Note that the bottom of the Pfotzer Maximim is near 55,000 ft. This means that some high-flying aircraft are not far from the zone of maximum radiation. Indeed, according to the Oct 22th measurements, a plane flying at 45,000 feet is exposed to 2.79 uSv/hr. At that rate, a passenger would absorb about one dental X-ray's worth of radiation in about 5 hours.

The radiation sensors onboard our helium balloons detect X-rays and gamma-rays in the energy range 10 keV to 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.

  Essential web 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 Dynamics Observatory
  Researchers call it a "Hubble for the sun." SDO is the most advanced solar observatory ever.
  3D views of the sun from NASA's Solar and Terrestrial Relations Observatory
Solar and Heliospheric Observatory
  Realtime and archival images of the Sun from SOHO.
Daily Sunspot Summaries
  from the NOAA Space Environment Center
  the underlying science of space weather
Synergy Spray Foam Insulation of Houston TX
  Protection from the Sun!
Kotton Grammer, Search Engine Marketing
  a sponsor of
Columbia Northern High School
  Web-based high school science course with free enrollment
  the underlying science of space weather
  more links...
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