SOLAR WEATHER
and some interesting space stuff

2010

compiled by Dee Finney

OCTOBER - 2010

PAGE 10

updated  -  10-31 -10

 

THIS COMPILATION IS BEING DONE IN HONOR OF KENT STEADMAN
OF  www.cyberspaceorbit.com  who left his earthly abode in 2008

 

2008 SOLAR WEATHER

 

2009 SOLAR WEATHER
JANUARY - FEBRUARY - MARCH - APRIL - MAY  - JUNE - JULY -
AUGUST - SEPTEMBER - OCTOBER - NOVEMBER - DECEMBER

 

2010 SOLAR WEATHER

JANUARY - FEBRUARY - MARCH - APRIL - MAY - JUNE - JULY
AUGUST - SEPTEMBER - OCTOBER - NOVEMBER - DECEMBER

 

On January 17, there were 1092 potentially hazardous asteroids.
On February 17, there were 1100 potentially hazardous asteroids.
NOTE:  These are not 'new' asteroids'  merely newly discovered by people and their new telescopes.
On March 24, there were 1110 potentially hazardous asteroids.
On April 5, there are 1110 potentially hazardous asteroids.
On April 14, there are 1117 potentially hazardous asteroids.

On May 15, there are 1127 potentionally hazardous asteroids.
On June 19, there are 1133 potentially hazardous asteroids.
On June 23, there are 1138 potentially hazardous asteroids.
On July 23, there are 1140 potentially hazardous asteroids.
On August 12, there are 1142 potentially hazardous asteroids.
On September 3, there are 1144 potentially hazardous asteroids.

On October 8, there are 1149 potentially hazardous asteroids.

 

ONE YEAR UNTIL THE METEOR OUTBURST: Every year around Oct. 8th, Earth passes through a minefield of dusty debris from Comet Giacobini-Zinner, source of the annual Draconid meteor shower. This year, forecasters expect Earth to narrowly miss several of the debris streams, resulting in no appreciable display for 2010. Next year, however, could be different. On Oct. 8, 2011, Earth will have a near head-on collision with a tendril of dust, setting off a strong outburst of as many as 750 meteors per hour. People in Europe, Africa and the Middle East will have a front-row seat for what could be the strongest shower since the Leonid storms a decade ago. Mark your calendar and, meanwhile, follow these links for more information: Draconid forecasts; sky map; history;

 

 

10-31-10  sunspot 1117

Solar wind
speed: 335.6 km/sec
density: 0.1 protons/cm3
explanation | more data
Updated: Today at 1016 UT
X-ray Solar Flares
6-hr max: C4 0430 UT Oct31
24-hr: C4 0430 UT Oct31
explanation | more data


HALLOWEEN FLARES: After two days of quiet, big sunspot 1117 is once again crackling with solar flares. Magnetic fields around the active region became unstable on Oct. 31st, unleashing a C2-class flare at 0318 UT and a C6-class flare at 0431 UT. Stay tuned for movies.



Updated: Today at: 1010 UT
10-30-10  sunspoy 1117 
Solar wind
speed: 393.2 km/sec
density: 0.3 protons/cm3
explanation | more data
Updated: Today at 1125 UT
X-ray Solar Flares
6-hr max: B3 0540 UT Oct30
24-hr: B3 0540 UT Oct30
explanation | more data
Updated: Today at: 1125 UT
 

SHADOWS ON JUPITER: On Saturday night, Oct. 30th, two of Jupiter's moons (Europa and Ganymede) will simultaneously cast their shadows on the giant planet's cloudtops. The closely-spaced shadows will be visible in mid-sized backyard telescopes and live on the web. The time to look is between 9:16 p.m. and 11:59 p.m. Pacific Daylight Time. [sky map]

ASTEROID FLYBY: Asteroid 2003 UV11 flew past past Earth last night only 1.2 million miles away. Many amateur astronomers were able to photograph the 600 meter-wide space rock racing like Speedy Gonzales among the stars of Andromeda and Pegasus. Browse the images: #1, #2, #3, #4, #5, #6, #7, #8, #9  [images: #1, #2, #3] [ephemeris] [3D orbit]

 


10-29-10   sunspot 1117

GIANT SUN TWISTER: On Oct. 27th and 28th, a twisted filament of magnetism on the sun decided to untwist. The result was a spectacular eruption recorded in full-disk detail by NASA's Solar Dynamics Observatory:


Movie formats: 8 MB gif, 3 MB gif, 1.7 MB iPad, 0.7 MB iPhone

At its peak, the twister--or rather, untwister--towered more than 350,000 km above the stellar surface. It appears to have hurled a fragment of itself into space, but not toward Earth; the blast was not geoeffective.

Now that the filament has relaxed, it is unlikely to erupt again. The next blast is more likely to come from big sunspot 1117, which NOAA forecasters say could produce an M-class solar flare. Readers with solar telescopes are encouraged to monitor developments.



Solar wind
speed: 339.6 km/sec
density: 0.1 protons/cm3
explanation | more data
Updated: Today at 2344 UT
X-ray Solar Flares
6-hr max: B1
2340 UT Oct29
24-hr: B3
0535 UT Oct29
explanation | more data
Updated: Today at: 2340 UT


DURING THE PAST 24 hours, the EARTH has been hit by about a million small meteoroids – most of which burned up in the atmosphere as shooting stars. This happens every day. And occasionally – once every 10,000 years or so —
a really big asteroid (500 meters in diameter or larger) comes along and smacks EARTH with an EXTINCTION-LEVEL IMPACT. But in between are other asteroid hits that occur every 200-300 years where a medium-sized chunk of space rock intersects with Earth’s orbit, producing a Tunguska-like event, or worse.

THERE ARE LIKELY about one million NEAR EARTH OBJECTS out there that could do substantial damage if one hit the EARTH. We DO possess the technology to move asteroids or change their orbits, and that this technology does need to be tested, and tested SOON. An impact event could affect the entire world, and the decisions on policies and international agreements about asteroid mitigation could pose a bigger challenge to dealing with an asteroid threat. The Mission Planning and Operations Group (MPOG) workshop included astronauts and space scientists and was the latest in a series of workshop designed to offer suggestions to the UN Committee on the Peaceful Uses of Outer Space.
-- Nancy Atkinson


10-28-10-  sunspot `1117
Solar wind
speed: 439.5 km/sec
density: 1.8 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: B1 2255 UT Oct28
24-hr: B2 1455 UT Oct28
explanation | more data
Updated: Today at: 2340 UT

DEAD SPACECRAFT WALKING: Two NASA spacecraft that were supposed to be dead a year ago are instead flying to the Moon for a breakthrough mission in lunar orbit. The research they conduct could lead to important advances in space weather forecasting. For more information, read "Dead Spacecraft Walking" from Science@NASA.

 


Oct. 27, 2010:  A pair of NASA spacecraft that were supposed to be dead a year ago are instead flying to the Moon for a breakthrough mission in lunar orbit.

"Their real names are THEMIS P1 and P2, but I call them 'dead spacecraft walking,'" says Vassilis Angelopoulos of UCLA, principal investigator of the THEMIS mission. "Not so long ago, we thought they were goners. Now they are beginning a whole new adventure."

Artemis (artemis, 550px)
An artist's concept of THEMIS-P1 and P2 (since renamed ARTEMIS-P1 and P2) in lunar orbit. [larger image]

The story begins in 2007 when NASA launched a fleet of five spacecraft into Earth's magnetosphere to study the physics of geomagnetic storms. Collectively, they were called THEMIS, short for "Time History of Events and Macroscale Interactions during Substorms." P1 and P2 were the outermost members of the quintet.

Working together, the probes quickly discovered a cornucopia of previously unknown phenomena such as colliding auroras, magnetic spacequakes, and plasma bullets shooting up and down Earth’s magnetic tail. These findings allowed researchers to solve several longstanding mysteries of the Northern Lights.

Artemis (Northern Lights, 200px)
In their previous life, THEMIS-P1 and P2 were on a mission to study Northern Lights. [more]

The mission was going splendidly, except for one thing: Occasionally, P1 and P2 would pass through the shadow of Earth. The solar powered spacecraft were designed to go without sunlight for as much as three hours at a time, so a small amount of shadowing was no problem. But as the mission wore on, their orbits evolved and by 2009 the pair was spending as much as 8 hours a day in the dark.

"The two spacecraft were running out of power and freezing to death," says Angelopoulos. "We had to do something to save them."

The team brainstormed a solution. Because the mission had gone so well, the spacecraft still had an ample supply of fuel--enough to go to the Moon. "We could do some great science from lunar orbit," he says. NASA approved the trip and in late 2009, P1 and P2 headed away from the shadows of Earth.

With a new destination, the mission needed a new name. The team selected ARTEMIS, the Greek goddess of the Moon. It also stands for "Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon’s Interaction with the Sun."

The first big events of the ARTEMIS mission are underway now. On August 25, 2010, ARTEMIS-P1 reached the L2 Lagrange point on the far side of the Moon. Following close behind, ARTEMIS-P2 entered the opposite L1 Lagrange point on Oct. 22nd. Lagrange points are places where the gravity of Earth and Moon balance, creating a sort of gravitational parking spot for spacecraft.

 

10-27-10  subspot 1117

POSSIBLE METEORS FROM COMET HARTLEY 2: A pair of unusual fireballs over Canada and the southeastern USA have experts wondering if Comet Hartley 2 might produce a meteor shower in early November. Get the full story from Science@NASA.

BIG BRIGHT OBJECT NEAR THE SUN: Don't panic, it's just Venus. The brilliant evil twin of Earth is passing between our planet and the sun this week, making a bright UFO-like light in SOHO coronagraph images:

venus 10-27-10

The bright rays and luminous bloom centered on the planet are digital artifacts. Venus is so bright, it saturates SOHO's CCD detectors, causing electrons to "bleed" across pixel boundaries. The same thing happens to a lesser degree with Mercury, which is bisected by a horizontal bar--another artifact. Note how the star Spica, dimmer than the planets, appears as a normal pinprick. It does not saturate the CCD.

Venus will continue its flamboyant passage for the next few days. Join SOHO for a ringside seat.

A BIG SUNSPOT GETS BIGGER: Behemoth sunspot 1117 is not merely growing, it is transmogrifying. Click on the image to launch a two-day movie from NASA's Solar Dynamics Observatory (8 MB):

sunspot 1117

Since yesterday, the shape-shifting sunspot has developed a "beta-gamma" magnetic field that harbors energy for M-class solar flares. Any such eruptions will likely be geoeffective because the sunspot is almost-squarely facing Earth. Readers with solar telescopes are encouraged to monitor developments.

more images: from Rogerio Marcon of CASLEO Observatory, San Juan, Argentina; from Patrick Bornet of Saint Martin sur Nohain, Nièvre, France; from David Arditti of Edgware, UK; from John Stetson of Portland, Maine


October 2010 Aurora Gallery
[previous Octobers: 2009, 2008, 2007, 2006, 2004, 2003, 2002, 2001]

10-27-10  Solar wind

speed: 495.7 km/sec
density: 1.1 protons/cm3
explanation | more data
Updated: Today at 2006 UT
X-ray Solar Flares
6-hr max: B7 1705 UT Oct27
24-hr: B7 1705 UT Oct27
explanation | more data
Updated: Today at: 2005 UT
10-26-10  sunspot 1117

Solar wind
speed: 552.2 km/sec
density: 1.1 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: B1 2310 UT Oct26
24-hr: C1 0110 UT Oct26
explanation | more data
Updated: Today at: 2340 UT

ARCTIC AURORA OUTBURST: On Oct. 24th, an outburst of color bright enough to rival the Moon spread across the skies of Scandinavia. Thilo Bubek sends this picture from the outskirts of Tromsø, Norway:



aurora 10-26-10

"The auroras were beautiful," says Bubek. Bright moonlight often overwhelms auroras, but in this case the nearly-full Moon was an asset. "It illuminated the landscape, setting the stage for a nice photo-op."

The source of the display was a high-speed solar wind stream, which hit Earth's magnetic field over the weekend, sparking two days of intermittent polar geomagnetic activity. It could turn into three days: High-latitude sky watchers should be alert for more auroras tonight as the solar wind continues to blow.


10-25-10  sunspot 1117

FAST-GROWING SUNSPOT: Sunspot group 1117 more than tripled in size over the weekend: SDO movie. The active region has not yet produced a major eruption, but it is crackling with picturesque B-class solar flares. Stay tuned for updates.



Solar wind
speed: 607.8 km/sec
density: 0.7 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: C2 2210 UT Oct25
24-hr: C2 2210 UT Oct25
explanation | more data
Updated: Today at: 2340 UT

10-24-10  subspot group 1017
Sunspot group 1117 continues to increase in spot count and magnetic complexity. No big flares yet, however.
Credit: SOHO/MDI. 2-day movie: 8 MB mpg

GEOMAGNETIC STORM WARNING: NOAA forecasters estimate a 40% chance of severe geomagnetic storms around the poles on Oct. 25th. The forecast is prompted by a possible double whammy: both a solar wind stream and a CME could hit Earth's magnetic field on that date. High-latitude sky watchers should be alert for auroras.



Solar wind
speed: 633.8 km/sec
density: 1.3 protons/cm3
explanation | more data
Updated: Today at 1146 UT
X-ray Solar Flares
6-hr max: B2 1050 UT Oct24
24-hr: B2 1050 UT Oct24
explanation | more data
Updated: Today at: 1145 UT
10-23-10- sunspot 1047
Solar wind
speed: 643.6 km/sec
density: 0.8 protons/cm3
explanation | more data
Updated: Today at 2228 UT
X-ray Solar Flares
6-hr max: B4 2010 UT Oct23
24-hr: B4 2010 UT Oct23
explanation | more data
Updated: Today at: 2340 UT

AURORA ALERT: High-latitude sky watchers should be alert for auroras. A high-speed solar wind stream is buffeting Earth's magnetic field and causing polar geomagnetic storms.

THE SURPRISING CONTENTS OF LUNAR CRATERS: Nearly a year after announcing the discovery of water molecules on the moon, scientists say there's more than just water hiding in cold lunar craters. Get the full story from Science@NASA.

10-22-10 - sunspots 1015, 1017

Solar wind
speed: 649.8 km/sec
density: 1.5 protons/cm3
explanation | more data
Updated: Today at 2157 UT
X-ray Solar Flares
6-hr max: B4 2010 UT Oct23
24-hr: B4 2010 UT Oct23
explanation | more data
Updated: Today at: 2145 UT
 


COMET HARLEY

Photography is difficult due to the Moon, but with narrowband filters the comet stands out quite nicely," he says. "The tail is now very well defined, and stands in beautiful contrast to the diffuse green coma. This was a 15 minute exposure."

Astronomers who wish to monitor this small but active comet should point their optics at the constellation Auriga high in the northern sky before dawn. Moonlight will make finding the comet a little tricky. On the bright side, reading the finder chart will be a breeze!

more images: from Rolando Ligustri using a robotic telescope in New Mexico; from Efrain Morales Rivera of Aguadilla, Puerto Rico; from Tamás Ábrahám of Zsámbék, Hungary;

 

10-21-10 - sunspot 1017

SUNDIVING COMET: The solar system now has one less comet. Earlier today, a sundiving comet discovered on Oct. 19th by Chinese amateur astronomer Bo Zhou passed too close to the sun and apparently evaporated. A coronagraph onboard the Solar and Heliospheric Observatory (SOHO) recorded the death plunge:



comet-10-21-10

The comet was likely a member of the Kreutz sungrazer family. Named after a 19th century German astronomer who studied them in detail, Kreutz sungrazers are fragments from the breakup of a giant comet at least 2000 years ago. Several of these fragments are thought to pass by the sun and disintegrate every day. Most are too small to see but occasionally a big fragment like this one attracts attention

ASTEROID FLYBY: Asteroid 2010 TG19 is flying past the Earth-Moon system today, Oct. 22nd, only 24,000 miles beyond the orbit of the Moon. The 70-meter space rock is about twice the size of the asteroid or comet that flattened a forest in Siberia in 1908. In this case, however, there is no danger of a collision.
Astronomers at the Sormano Astronomical Observatory in Italy photographed the asteroid's approach on Oct. 21st using a 20-inch telescope: image.


Solar wind
speed: 372.5 km/sec
density: 2.4 protons/cm3
explanation | more data
Updated: Today at 0315 UT
X-ray Solar Flares
6-hr max: B3
1910 UT Oct21
24-hr: B3
1910 UT Oct21
explanation | more data
Updated: Today at: 2355 UT

ORIONID METEOR UPDATE: Earth is exiting a stream of debris from Halley's Comet, the source of the annual Orionid meteor shower. According to preliminary counts from the International Meteor Organization, the shower peaked on Oct. 21st with 35 meteors per hour. Here are some of them: #0, #1, #2, #3. Activity should continue at reduced levels for another day or two with continued interference from the bright Moon. Listen for stragglers at Spaceweather Radio.


10-20-10- sunspot 1113

Solar wind
speed: 402.5 km/sec
density: 2.4 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: B1 1745 UT Oct20
24-hr: C1 1150 UT Oct20
explanation | more data
Updated: Today at: 2340 UT

SUNDIVING COMET: A newly-discovered comet is diving toward the sun. Chinese comet hunter Bo Zhou found it on Oct. 19th in SOHO coronagraph images. The comet is faint now, but it should brighten in the hours ahead as it heats up. To see it, first check the finder chart, then play the latest movie. That tadpole is a doomed comet. Updates will be posted as the view improves.

ORIONID METEOR SHOWER: Earth is entering a broad stream of debris from Halley's Comet, and this is causing the annual Orionid meteor shower. "The best time to look is during the hours before dawn on Thursday, Oct. 21st, and again on Friday, Oct 22nd," advises Bill Cooke of NASA's Meteoroid Environment Office. "Unfortunately, we have a bright Moon this year. Even so, I'd expect some bright Orionids to shine through the moonlight." An all-sky camera at the University of Western Ontario recorded this early Orionid fireball on Oct. 18th:


Orionid meteors stream from the elbow of Orion the Hunter: sky map. Because the shower's radiant point is close to the celestial equator, sky watchers in both hemispheres can enjoy the show. Moonlit meteor rates will probably be around a dozen per hour.

Radar rates could be much higher. The US Air Force Space Surveillance Radar in Texas is scanning the skies for satellites, space junk, and meteoroids. When an Orionid passes overhead--ping!--there is an echo. Moonlight does not interfere with this method of meteor observing, so it's perfect for this year's Orionids. Tune into Spaceweather Radio for live echoes.

Orionid images: from John Chumack of Dayton, Ohio; from Calvin Hall of Knik Valley, near Palmer Alaska; from Martin Popek of Nýdek, Czech republic

 

Apart from the blue-green color, this view matches what the comet looked like visually through large binoculars — a round fuzzball," says Dyer.

Many readers have asked, why is the comet green? Answer: Hartley 2's green color comes from the gases that make up its Jupiter-sized atmosphere. Jets spewing from the comet's nucleus contain cyanogen (CN: a poisonous gas found in many comets) and diatomic carbon (C2). Both substances glow green when illuminated by sunlight in the near-vacuum of space.

NASA scientists say 103P/Hartley 2 is one of the most active comets they've seen, with copious outgassing from jets in the nucleus. Amateur astronomers are encouraged to monitor the action and submit their images here.

more images: from Doug Zubenel near Onaga, Kansas.; from Paul Klauninger of Marathon, Ontario, Canada; from Jimmy Westlake of Stagecoach, Colorado; from Nick Howes of Cherhill, Wiltshire, UK; from Abe Schwartz of San Juan, Puerto Rico; from Dr Paolo Candy of Ci.A.O. Cimini Astronomical Observatory - Italy; from John Chumack of Dayton, Ohio; from Keith Johnson of Durham, England,UK; from Joao Porto of Ponta Delgada, Azores islands, Portugal

 

10-19-10  a rash of new sunspots is erupting - no numbers as yet

Solar wind
speed: 431.2 km/sec
density: 2.4 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: B2 2305 UT Oct19
24-hr: C1 0650 UT Oct19
explanation | more data
Updated: Today at: 2340 UT

JUPITER-MOON CONJUNCTION: Look east after sunset. Jupiter and the Moon are having a close encounter (< 6o) in the constellation Pisces. The bright conjunction is visible even from light-polluted urban areas, no sky map required.

Jupiter-Moon images: from Stefano De Rosa of Turin, Italy;

FILAMENT ERUPTION: For days, astronomers have been monitoring a "mega-filament" of magnetism splayed across the sun's southern hemisphere. Measuring more than 500,000 km from end to end, it spans a distance greater than the separation of Earth and the Moon. Oct. 18th the massive structure erupted:

 

Movie formats: 1.6 MB mpeg, 1 MB m4v. Credit: Solar Dynamics Observatory

Instabilities in the filament sparked a C2-class flare and hurled a portion of the filament's own magnetic backbone into space. The blast was not Earth-directed. Remarkably, the structure survived mostly intact and is still visible in backyard optics. Readers with solar telescopes are encouraged to monitor developments.

more images: from Paul Maxson of Surprise, Arizona; from Didier Favre of Brétigny sur Orge, France; from Jan Timmermans of Valkenswaard, The Netherlands; from Stephen W. Ramsden of Atlanta, GA; from Francesc Pruneda of Palamos, Girona, Spain;

 


10-18-10   sunspot 1112, 1113, 1115

MEGA SOLAR FILAMENT: An awesome, monstrous, jaw-dropping, 400,000 km long filament of magnetism is stretched across the sun's southern hemisphere. If it collapses or erupts, as filaments often do, the result could be an Earth-directed coronal mass ejection. Meanwhile it is a fine target for backyard solar telescopes.

FILAMENT UPDATE: Magnetic instabilities in the filament caused an eruption today around 1600 UT. The filament was not destroyed, nor was material hurled toward Earth. SDO movies: mpeg, m4v.



Solar wind
speed: 379.5 km/sec
density: 3.2 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: C1 2135 UT Oct18
24-hr: C2 1640 UT Oct18
explanation | more data
Updated: Today at: 2340 UT

TIME TO SEE COMET HARTLEY: For backyard stargazers, the next few nights are the best time to see green Comet 103P/Hartley 2 as it approaches Earth for an 11-million-mile close encounter on Oct. 20th. Set your alarm for the dark hours before dawn, go outside, and look straight up. You will find Hartley 2 not far from the bright star Capella: sky map. Although the comet is barely visible to the unaided eye, it is easy to find in binoculars and looks great through a backyard telescope.

Last night, Filipe Alves of Portalegre, Portugal, obtained the following long-exposure image using an 8-inch telescope and a KAF-8300 refrigerated CCD camera. It shows the comet's vast green atmosphere and an auburn tail of dust:

comet harley 10-19-10

Many readers have asked, why is the comet green? Answer: Hartley 2's green color comes from the gases that make up its Jupiter-sized atmosphere. Jets spewing from the comet's nucleus contain cyanogen (CN: a poisonous gas found in many comets) and diatomic carbon (C2). Both substances glow green when illuminated by sunlight in the near-vacuum of space.

NASA scientists say 103P/Hartley 2 is one of the most active comets they've seen, with copious outgassing from jets in the nucleus. Amateur astronomers are encouraged to monitor the action and submit their images here.

more images: from Tom Jorgenson of Neenah, Wisconsin; from Yandong Hu of Mt. Wawushan, Jiangsu, China; from Rolando Ligustri using a robotic telescope in New Mexico; from Marian Urbaník of Staškov, Slovak republic; from John Chumack of Dayton, Ohio; from Jan Koeman of Kloetinge, the Netherlands; from Jodi and Roy McCullough of Salem Ohio; from Mike Broussard of Maurice, Louisiana; from Mike Holloway of Van Buren, Arkansas; from Norm Klekoda and Al Bell near Grand Rapids, MI; from Doug Zubenel of Monument Rocks, Gove County, Kansas; from Gregg Ruppel of Ellisville, Missouri


10-17-10  sunspot 1112, 1113, 1115

SOLAR FLARES: Fast-growing sunspot 1112 is crackling with solar flares. SDO movies show the three strongest of the past 24 hours: an M3-flare @ 1910 UT on Oct. 16th, a C1-flare @ 0900 UT and another C1-flare @ 1740 UT on Oct. 17th. So far, none of the blasts has hurled a substantial CME toward Earth.


Solar wind
speed: 410.2 km/sec
density: 0.5 protons/cm3
explanation | more data
Updated: Today at 2342 UT
X-ray Solar Flares
6-hr max: B5 1745 UT Oct17
24-hr: C1 0900 UT Oct17
explanation | more data
Updated: Today at: 2340 UT
10-16-10  sunspot 1112, 1113

Solar wind
speed: 346.6 km/sec
density: 0.2 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: M1 1910 UT Oct16
24-hr: M1 1910 UT Oct16
explanation | more data
Updated: Today at: 2340 UT
10-15-10  sunspot 1013 and 1014

Solar wind
speed: 333.3 km/sec
density: 0.5 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: B1
2335 UT Oct15
24-hr: B1
0035 UT Oct15
explanation | more data
Updated: Today at: 2340 UT
GREAT FILAMENT: The biggest thing on the sun today is not a sunspot--and it's not even close. A dark magnetic filament 20 times wider than a typical sunspot is meandering across the sun's southern hemisphere. It's so big, astrophotographer Pete Lawrence of Selsey, UK, had to stitch together several pictures to display the entire structure
sun filament-10-15-10'

The filament is filled with relatively dense plasma held above the stellar surface by magnetic forces. Because this plasma is cooler than the sun below, it appears dark. In fact, it is not. If you could hold the filament out against the black of space, it would glow more brightly than a full Moon.

The 400,000-km scale of the filament--long enough to stretch from Earth to the Moon!--makes it an easy target for safely-filtered backyard optics. If you have a solar telescope, take a look.

more images: from Stephen Ramsden of Immaculate Heart of Mary Catholic School, Atlanta, GA; from Jean-Pierre Brahic of Uzès ( France); from Michael Boschat of Halifax,Nova Scotia,Canada; from James Kevin Ty of Manila , Philippines; from the Solar Dynamics Observatory in Earth orbit; from Didier Favre of Brétigny-sur-Orge, France; from Ron Cottrell of Oro Valley, Arizona;

COMET HARTLEY UPDATE: "Comet 103P/Hartley 2 is growing at an amazing rate," reports Nick Howes of Cherhill, Wiltshire, UK. "The comet's atmosphere (coma) is now more than 1o wide." He took this picture on Oct. 13th using the 2-meter robotic Faulkes North Telescope in Hawaii:

comet hartley-10-16-10

Comet Hartley is approaching Earth for an 11-million-mile close encounter on Oct. 20th. Although it is barely visible to the naked eye, the comet looks great through backyard telescopes. The best time to look is during the dark hours before sunrise when the comet is almost straight overhead in the constellation Perseus. Check Sky & Telescope for a sky map and more.

Need a telescope for Comet Hartley 2? We recommend the David H. Levy Comet Hunter, specifically designed by comet-master David Levy for times like these.

more images: from Rolando Ligustri using a robotic telescope in New Mexico; from Mike Broussard of Maurice, Louisiana; from Fredrik Broms of Kvaløya, Norway; from Tamás Ábrahám of Zsámbék, Hungary; from Efrain Morales Rivera of Aguadilla, Puerto Rico; from P-M Hedén of Vallentuna, Sweden;


10-14-10  sunspt 1113

Solar wind
speed: 299.0 km/sec
density: 4.8 protons/cm3
explanation | more data
Updated: Today at 1217 UT
X-ray Solar Flares
6-hr max: B1 1125 UT Oct14
24-hr: B1 1125 UT Oct14
explanation | more data
Updated: Today at: 1210 UT

NEW SUNSPOT ERUPTS: New sunspot 1113 emerged over the sun's northeastern limb yesterday and immediately announced itself with a towering eruption. NASA's Solar Dynamics Observatory (SDO) recorded the blast on Oct. 13th around 1600 UT:



Magnetic fields reconnecting above the sunspot produced a B4-class solar flare and hurled a narrow coronal mass ejection into space: SOHO movie. Earth was not in the line of fire--but this could change in the days ahead as the sunspot turns to face our planet. Readers with solar telescopes are encouraged to monitor developments

MONTANA AURORAS: On Oct. 11th, a bright curtain of Northern Lights unfurled along the US-Canadian border. Watching from Glasgow in northern Montana, Ben Fyngyrz took this picture:

Nontana auroras
Photo details: Canon EOS 50D, 4 seconds, ISO 1600, f/1.8

"The lights didn't make it all the way down to my latitude," he says , "but the side-view was interesting because it showed the vertical structure of the auroras." More of Ben's photos show dark clouds and a 19th century prairie house backlit by the auroras--very pretty.

 

10-12-10  sunspot 1112

PHOTOGENIC SUNSPOT: An enormous magnetic filament is perched directly above sunspot 1112 near the sun's southeastern limb. If the filament collapses (as they often do) and hits the sunspot below, the resulting explosion could be impressive. Actually, it's already impressive:

sunspot 1112

Dutch amateur astronomers Jo Dahlmans and Wouter Verhesen took the picture yesterday using a Lunt solar telescope. "We inverted (made negative) the sun's surface for a stunning display of the snaking filament," says Dahlmans. "In the distance you can see prominences dancing like flames along the limb of the sun. What a vista!"

Readers with solar


Readers with solar telescopes, you know what to do.

more images: from Dave Gradwell of Birr, Ireland; from Jimmy Eubanks of Boiling Springs, SC; from Robert Arnold of Isle of Skye, Scotland; from James Kevin Ty of Manila, Philippines; from Michael Buxton of Ocean Beach, California; from Gianfranco Meregalli of Milano, Italy


Solar wind
speed: 394.2 km/sec
density: 0.7 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A9 2325 UT Oct12
24-hr: A9 2325 UT Oct12
explanation | more data
Updated: Today at: 2340 UT

ASTEROID FLYBY--DONE! Asteroid 2010 TD54 flew past Earth this morning (Oct. 12) at 6:50 am EDT only 46,000 km above the planet's surface. For comparison, geosynchronous satellites orbit at 36,000 km, so the asteroid was not far beyond Earth's satellite fleet. No damage was done--to spacecraft or to the planet below. Amateur astronomer Patrick Wiggins photographed the flyby using a 14-inch Celestron telescope: movie.

10-11-10

10-10-10  sunspot 1012  is no threat

ACTIVE REGION 1112: Emerging sunspot 1112 is connected to a vast network of dark magnetic filaments looping around the sun's southeastern limb. NASA's Solar Dynamics Observatory took this picture of the region just hours ago:

sunspot 1112

Filaments such as these have a habit of erupting. Will the fact that they are rooted in a sunspot make them more--or less--stable? No one knows. The magnetohydrodynamics of sunspots is so complex, not even the most powerful supercomputers on Earth can predict when they will erupt. Readers with solar telescopes are encouraged to monitor this region for unexpected developments.

more images: from Ingmar Glass of Bavaria, Germany; from Cai-Uso Wohler of Bispingen, Germany; from Larry Alvarez of Flower Mound, Texas


Solar wind
speed: 327.4 km/sec
density: 6.0 protons/cm3
explanation | more data
Updated: Today at 2120 UT
X-ray Solar Flares
6-hr max: A8 2000 UT Oct10
24-hr: B4 0940 UT Oct10
explanation | more data
Updated: Today at: 2340 UT
10-9-10  no sunsp0ots

FARSIDE BLAST: Old sunspot 1109 on the farside of the sun erupted during the late hours of Oct 8th, producing a CME and a solar tsunami. NASA's STEREO-A spacecraft recorded this movie of the blast. Earth will not be affected by these events.



Solar wind
speed: 354.3 km/sec
density: 0.5 protons/cm3
explanation | more data
Updated: Today at 2120 UT
X-ray Solar Flares
6-hr max: B2 1755 UT Oct09
24-hr: B2 1755 UT Oct09
explanation | more data
Updated: Today at: 2340 UT

10-8-10  No sunspots today

Solar wind
speed: 312.5 km/sec
density: 0.9 protons/cm3
explanation | more data
Updated: Today at 0005 UT
X-ray Solar Flares
6-hr max: B1 2345 UT Oct07
24-hr: B1 2345 UT Oct07
explanation | more data
Updated: Today at: 2350 UT  

FILAMENT ECLIPSE: At this time of year, near the autumnal equinox, the Earth can pass directly between the sun and NASA's Solar Dynamics Observatory, producing a brief eclipse. Yesterday this happened just as a magnetic filament was flying off the sun's northeastern limb. The advancing edge of the Earth cut the sun in half at the moment of maximum eruption:



filament eclipse

"The decline in ultra-violet radiation is much larger than anticipated. But the visible radiation actually increased as solar activity was declining.

Click here to view the full-sized image

Even by the lofty standards of SDO, this is a shot of rare beauty. A 5 1/2 hour movie sets the scene in motion; you can see the big-picture (5 MB gif) or a close-up (2 MB mpeg) of the filament. Another movie omits the Earth-shadows; it is easier to follow the filament, yet somehow less photogenic.

The eruption hurled a coronal mass ejection into space (SOHO saw it) but not toward Earth. No geomagnetic storms are expected as a result of the blast.


10-11-10  susspot 1112 isi turning toward earth

Solar wind
speed: 356.9 km/sec
density: 1.9 protons/cm3
explanation | more data
Updated: Today at 1136 UT
X-ray Solar Flares
6-hr max: A9 0510 UT Oct11
24-hr: A9 0510 UT Oct11
explanation | more data

Updated: Today at: 1135
UT
10-10-10  sunspot 1112

Solar wind
speed: 327.4 km/sec
density: 6.0 protons/cm3
explanation | more data
Updated: Today at 2120 UT
X-ray Solar Flares
6-hr max: A8 2000 UT Oct10
24-hr: B4 0940 UT Oct10
explanation | more data
Updated: Today at: 2340 UT

ACTIVE REGION 1112: Emerging sunspot 1112 is connected to a vast network of dark magnetic filaments looping around the sun's southeastern limb. NASA's Solar Dynamics Observatory took this picture of the region just hours ago:

sunspot 1112

Filaments such as these have a habit of erupting. Will the fact that they are rooted in a sunspot make them more--or less--stable? No one knows. The magnetohydrodynamics of sunspots is so complex, not even the most powerful supercomputers on Earth can predict when they will erupt. Readers with solar telescopes are encouraged to monitor this region for unexpected developments.

more images: from Ingmar Glass of Bavaria, Germany; from Cai-Uso Wohler of Bispingen, Germany; from Larry Alvarez of Flower Mound, Texas


10-9-10  no sunspots

Solar wind
speed: 354.3 km/sec
density: 0.5 protons/cm3
explanation | more data
Updated: Today at 2120 UT
X-ray Solar Flares
6-hr max: B2 1755 UT Oct09
24-hr: B2 1755 UT Oct09
explanation | more data
Updated: Today at: 2340 UT

FARSIDE BLAST: Old sunspot 1109 on the farside of the sun erupted during the late hours of Oct 8th, producing a CME and a solar tsunami. NASA's STEREO-A spacecraft recorded this movie of the blast. Earth will not be affected by these events.

 

NORTHERN LIGHTS FROM SPACE: A thin band of aurora borealis is running around the Arctic Circle. Click here to see it. Low-light cameras onboard the US military's DMSP F18 weather satellite photographed the display on Oct. 8th, and Paul McCrone of the Fleet Numerical Meteorology and Oceanography Center in Monteray, California, processed the data for spaceweather.com. This is not a major event, but it is a photogenic one from 450 miles overhead.


COMET HARTLEY AND THE DOUBLE CLUSTER: Comet 103P/Hartley 2 continues to put on a good show as it approaches Earth for an 11-million-mile close encounter on Oct. 20th. Last night it passed by the Double Cluster in Perseus. The contrast between the blue stars of the two clusters and the green atmosphere of the comet was remarkable:

Most observers agree that the comet is not yet visible to the naked eye, but it is an easy target for backyard telescopes. In recent nights, astronomers have enjoyed watching Comet Hartley 2 pass a succession of stars and deep-sky objects such as the Pacman nebula and the Double Cluster. Next up is eta Persei (η Per), a 4th-magnitude star that will shine through the comet's atmosphere on Oct 9th and 10th. Details and a sky map are available from from Sky & Telescope.

more images: from Mike Broussard of Maurice, Louisiana; from David A Harvey of Tucson, Arizona; from Tamás Ábrahám of Zsámbék, Hungary; from Nick Howes using the 2 Metre Faulkes North Telescope in Hawaii; from Dr Paolo Candy of Ci.A.O. Cimini Astronomical Observatory - Italy; from Parks Squyres of SaddleBrooke, Arizona; from Gregg Ruppel of Ellisville, MO; from Geir Øye of Ørsta, Norway; from Mohammad Rahimi of Honjan - Esfahan - Iran; from Joe Wheelock of McDonald Observatory, Texas; from Alex Roca of Hortoneda Lleida Spain; from Fredrik Broms of Kvaløya, Norway; from Ehsan Rostamizadeh of Kerman, Iran; from Stefano Moretti of Ravenna, Italy; from Florin Marc of Tg.Mures, Romania;



10-8-10  no sunspots

Solar wind
speed: 351.5 km/sec
density: 1.3 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A7 1930 UT Oct08
24-hr: B1 0500 UT Oct08
explanation | more data
Updated: Today at: 2340 UT

SDO SEES MOUNTAINS ON THE MOON: Yesterday, Oct. 7th, NASA's Solar Dynamics Observatory observed its first lunar transit when the new Moon passed directly between the spacecraft and the sun. SDO's 16 megapixel cameras recorded the event in detail, revealing jagged lunar mountains backlit by solar plasma:


lunar mountains

Beyond the novely of observing a such an event from space, these images have practical value to the SDO science team. Karel Schrijver of Lockheed-Martin's Solar and Astrophysics Lab explains: "The very sharp edge of the lunar limb allows us to measure the in-orbit characteristics of the telescope--e.g., light diffraction on optics and filter support grids. Once these are characterized, we can use that information to correct our data for instrumental effects and sharpen up the images to even more detail."

 

Ralph Seguin, also of Lockheed-Martin, has prepared a movie of the transit which shows the Moon interrupting an eruption on the sun's northwestern horizon. Watch it again. Did you notice the brief blackout near the beginning of the movie? That was the Earth passing in front of the sun just before the Moon did--a double solar eclipse!

 

10-7-10  No sunspots today

Solar wind
speed: 309.2 km/sec
density: 2.7 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: B1 1940 UT Oct07
24-hr: B1 1940 UT Oct07
explanation | more data
Updated: Today at: 2340 UT
10-6-10  No sunspots

Solar wind
speed: 329.1 km/sec
density: 0.3 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A7 1745 UT Oct06
24-hr: B1 0610 UT Oct06
explanation | more data
Updated: Today at: 2340 UT

COMET HARTLEY UPDATE: As comet 103P/Hartley 2 approaches Earth for an 11-million-mile close encounter on Oct. 20th, it grows bigger and bigger in backyard telescopes. The comet's beautiful green atmosphere now subtends an angle approcimately equal to a lunar sea:

hartley comet

Paul Klauninger of Marathon, Ontario, took the picture on Oct. 2nd using a 3-inch refracting telescope. "I photographed the Moon with the same set-up and placed it beside the comet for scale," he says. "In a five minute exposure the comet appears bright green and 7-8 arcminutes across."

Most observers agree that the comet is not yet

10-5-10  sunspot 1109 is disappearing

Solar wind
speed: 348.3 km/sec
density: 0.5 protons/cm3
explanation | more data
Updated: Today at 2253 UT
X-ray Solar Flares
6-hr max: B1 1910 UT Oct05
24-hr: B2 0840 UT Oct05
explanation | more data
Updated: Today at: 2255 UT

COMET HARTLEY AND THE OWL: The comet show continues. After visiting the Pacman nebula on Oct 1st and 22nd, green Comet 103P/Hartley 2 is now paying a call on the Owl cluster. Readers with wide-field telescopes are encouraged to monitor the comet's busy track across Cassiopeia in the nights ahead--especially Oct. 7th and 8th when the comet glides a mere 1o from the photogenic Double Cluster. Details and a sky map are available from from Sky & Telescope.


10-4-10  sunspot 1111

Solar wind
speed: 287.1 km/sec
density: 7.5 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A7 1745 UT Oct04
24-hr: C1 1635 UT Oct04
explanation | more data
Updated: Today at: 2340 UT

BIG GREEN COMET:
The icy nucleus of comet 103P/Hartley 2 measures no more than a couple of kilometers across. That tiny nugget, however, is surrounded by an vast atmosphere of gas more than 150,000 km in diameter--about the same size as the planet Jupiter! And it's coming our way. Amateur astronomer Nick Howes sends this picture of the approaching comet from Cherhill, WIltshire UK

"I photographed the comet on Oct. 1st using a 4-inch refractor," says Howes. "Four hours of exposure time revealed not only the comet's vast green atmosphere but also an emerging tail." Howes describes the processing of the data here.

At present, the comet is a 7th-magnitude object best seen through telescopes. (We recommend the Comet Hunter.) The view will improve, perhaps even to naked-eye visibility, as the comet glides by Earth only 11 million miles away on Oct. 20th.

Two weeks after Comet Hartley has its close encounter with Earth, NASA will have a close encounter with the comet. The Deep Impact/EPOXI spacecraft is hurtling toward Comet Hartley now, and on Nov. 4th it will fly 435 miles from the comet's active icy nucleus. The encounter will mark only the fifth time in history that a spacecraft has been close enough to image a comet's core.

Until then, amateur astronomers can monitor the comet as it glides through the constellation Cassiopeia in the evening sky. A finder chart from Sky and Telescope shows the comet passing by a variety of stars and deep-sky objects, offering many photo-ops in the nights ahead.

more images: from Toni Scarmato of San Costantino di Briatico, Calabria, Italy; from Peter Sherman of Fochabers, Moray, Scotland, UK; from Joao Porto of Ponta Delgada, Azores, Portugal; from Mohamad Soltanolkottabi of Hunejan, Esfahan, Iran; from Artyom Novichonok of Mayhill, NM; from Tony Cook of Ripon, North Yorkshire, UK; from Dr Paolo Candy of Ci.A.O. Cimini Astronomical Observatory, Italy; from Martin McKenna of Maghera, Co. Derry, N. Ireland; from Gary Colwell of Splitrock Observatory, Ardoch, Ontario; from Gregg Ruppel of Ellisville, MO; from Toni Scarmato of San Costantino di Briatico, Calabria, Italy; from the Harford County Astronomical Society of Bel Air, Maryland

 

10-3-10  sybsoit 1111 us growing

Solar wind
speed: 282.1 km/sec
density: 0.1 protons/cm3
explanation | more data
Updated: Today at 2340 UT
X-ray Solar Flares
6-hr max: B1
2145 UT Oct03
24-hr: B2 0435 UT Oct03
explanation | more data
Updated: Today at: 2340 UT

COMET HARTLEY 2 UPDATE: Is Comet Hartley 2 sprouting a tail? A series of five-minute integrations taken last night by Gregg Ruppel of Ellisville, Missouri, seems to show a growing elongation of the comet's atmosphere: images.

10-2-10  sunspot 1109 is large but quiet

Solar wind
speed: 315.6 km/sec
density: 0.2 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: B1 2335 UT Oct02
24-hr: B4 0850 UT Oct02
explanation | more data
Updated: Today at: 2340 UT

FARSIDE SOLAR ACTIVITY: On October 1st a bright coronal mass ejection blasted away from the far side of the sun: SOHO movie. The source appears to be a magnetic active region that formed just a few days ago, invisible from Earth because it is so far over the sun's western limb. However, NASA's STEREO-A spacecraft has a good view of the area. Stay tuned for updates.

APPROACHING COMET: Green comet 103P/Hartley 2 is approaching Earth for a close encounter on Oct. 20th. At that time, the comet will be only 11 million miles from Earth and should be dimly visible to the naked eye from dark sky sites. It already looks great through backyard telescopes:


comet 2010

Amateur astronomer Rolando Ligustri took this picture on Oct. 2nd using a 14-inch Global Rent-a-Scope in New Mexico. It shows Comet Hartley beside the spectacular Pacman Nebula (NGC 281), a star-forming cloud some ten thousand light years from Earth. "This is a very nice comet for telescopes and binoculars," says Martin Gembec who took a similar picture from his backyard observatory in the Czech Republic last night. "It has a [green atmosphere] almost 0.5 degrees wide and shines like a 7th magnitude star."

Two weeks after Comet Hartley has its close encounter with Earth, NASA will have a close encounter with the comet. The EPOXI spacecraft (formerly known as Deep Impact) is hurtling toward Comet Hartley now, and on Nov. 4th it will fly 435 miles from the comet's active icy nucleus. The encounter will mark only the fifth time in history that a spacecraft has been close enough to image a comet's core.

Until then, amateur astronomers can monitor the comet as it glides through the constellation Cassiopeia in the evening sky. A finder chart from Sky and Telescope shows the comet passing by a variety of stars and deep-sky objects, offering many photo-ops in the nights ahead.

more images: from Mike Holloway of Van Buren, Arkansas; from Mike Broussard of Maurice, Louisiana; from Dale Ireland of Silverdale, Washington; from Kevin Black of Winnipeg, Manitoba Canada; from Alan Dyer of near Cluny, Alberta, Canada; from Tamás Ábrahám of Zsámbék, Hungary

10-1-10 sunspot 1109 is decaying

Solar wind
speed: 349.6 km/sec
density: 0.2 protons/cm3
explanation | more data
Updated: Today at 2343 UT
X-ray Solar Flares
6-hr max: B1 1800 UT Oct01
24-hr: B5 1000 UT Oct01
explanation | more data
Updated: Today at: 2340 UT
APPROACHING COMET: Green comet 103P/Hartley 2 is approaching Earth for a close encounter on Oct. 20th. At that time, the comet will be only 11 million miles from Earth and should be dimly visible to the naked eye from dark sky sites. It already looks great through backyard telescopes. Italian amateur astronomer Toni Scarmato took this picture on Sept. 29th using a 10-inch reflector
comet 2010

He caught the comet gliding by lambda Cassiopeia, a 6th magnitude double star. "In 7x50 binoculars, the comet is diffuse and very large," says Scarmato. "I estimate its size around 20-arcminutes and brightness at magnitude +7.5."

Two weeks after Comet Hartley has its close encounter with Earth, NASA will have a close encounter with the comet. The EPOXI spacecraft (formerly known as Deep Impact) is hurtling toward Comet Hartley now, and on Nov. 4th it will fly 435 miles from the comet's active icy nucleus. The encounter will mark only the fifth time in history that a spacecraft has been close enough to image a comet's core.

Until then, amateur astronomers can monitor the comet as it glides through the constellation Cassiopeia in the evening sky. A finder chart from Sky and Telescope shows the comet passing by a variety of stars and deep-sky objects, offering many photo-ops in the nights ahead.

more images: from Michael Jäger of Stixendorf Austria; from P-M Hedén of Vallentuna, Sweden; from Mike Broussard of Maurice, Louisiana; from Rolando Ligustri observing remotely from New Mexico; from Mike Holloway of Van Buren, Arkansas;

 

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