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LOST ASTEROID RETURNS TO EARTH: In Nov. 2010, the Catalina Sky Survey in Arizona discovered a near-Earth asteroid as wide as a football field. Before astronomers could fully trace its orbit, however, the receding space rock faded away. It has been lost ever since--that is, until last week when it reappeared, approaching Earth.
The name of the asteroid is 2010 WC9. Marian Urbanik of Čadca, Slovakia, photographed it on May 12th--a barely visible 17th magnitude speck in the constellation Hercules:
It is about to get much closer and brighter. On May 15th 2010 WC9 will fly past our planet, splitting the distance between Earth and the Moon. At closest approach (203,000 km), it will glow like an 11th magnitude star (~250 times brighter than shown above) as it races through the southern constellation Pavo.
Estimates of 2010 WC9's size range from 60 m to 130 m wide. This puts it in the class of the Tunguska impactor, which leveled a forest in Siberia in 1908. And it is at least 3 times as large as the Chelyabinsk meteoroid, which exploded in the morning sky over Russia on Feb. 15, 2013, shattering windows and knocking people to the ground
There's no danger of a collision this time, though. Analysts are certain 2010 WC9 will not hit Earth--neither this week nor in the foreseeable future. New observations of the asteroid in recent days have extended our knowledge of its orbit and eliminated it as a threat for at least the next 100 years.
2010 WC9 is invisible to the naked eye. Advanced amateur astronomers can photograph it, however, using mid-sized telescopes equipped with low-light video cameras. Southern hemisphere observers are favored, expecially those in South Africa and southern parts of South America where the asteroid will be high in the night sky at closest approach. [ephemeris] [3D orbit]
Realtime Space Weather Photo Gallery
GEOMAGNETIC STORMS POSSIBLE LATER THIS WEEK: NOAA forecasters say that polar geomagnetic storms are possible on May 17th when a stream of solar wind reaches Earth. The gaseous material is flowing from a southern hole in the sun's atmosphere, shown here in a false-color UV image from NASA's Solar Dynamics Observatory:
This is a coronal hole--a place where the sun's magnetic field opens up and allows solar wind to escape. Coronal holes look dark because hot glowing gas normally contained there is missing.
Previous encounters with solar wind from this coronal hole suggest that storm levels could reach category G2 when the fast-moving stream arrives, although a lesser G1 storm is more likely.. High latitude sky watchers should be alert for auroras and, of course, STEVE. Free: Aurora Alerts.
Realtime Aurora Photo Gallery
3D GLOWING MOON GLOBE: Are you looking for a far-out gift? Consider this: In January, the students of Earth to Sky Calculus flew a glowing 3D printed Moon globe to the stratosphere:
You can have it for $149.95. The students are selling these unique globes as a fundraiser for their cosmic ray monitoring program.
The surface of the sphere is an accurate topo-map of lunar terrain, tracing every major crater and mountain range. It is also a night light. A built-in USB-rechargeable battery provides up to 20 hours of illumination.
Each glowing orb comes with a greeting card showing the Moon in flight and telling the story of its journey to the edge of space. All proceeds support Earth to Sky Calculus and hands-on STEM research.
Far Out Gifts: Earth to Sky Store
All proceeds support hands-on STEM education
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 Spaceweather.com.
On May. 14, 2018, the network reported 7 fireballs.
(7 sporadics)
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]
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 14, 2018 there were 1907 potentially hazardous asteroids.
|
Recent & Upcoming Earth-asteroid encounters: Asteroid | Date(UT) | Miss Distance | Velocity (km/s) | Diameter (m) |
2018 JK2 | 2018-May-09 | 9.5 LD | 5.8 | 27 |
388945 | 2018-May-09 | 6.5 LD | 9 | 295 |
2018 JP | 2018-May-09 | 2.1 LD | 7.4 | 12 |
2018 JJ | 2018-May-10 | 13.1 LD | 12.7 | 51 |
2018 JF2 | 2018-May-11 | 13.3 LD | 8.3 | 49 |
2018 GR2 | 2018-May-11 | 13.4 LD | 9.8 | 111 |
2018 JZ | 2018-May-11 | 4.3 LD | 13.2 | 13 |
2016 HP6 | 2018-May-13 | 2.2 LD | 5.6 | 28 |
2018 JA1 | 2018-May-13 | 4.4 LD | 5.8 | 27 |
2018 JL1 | 2018-May-14 | 7.5 LD | 5.7 | 17 |
2018 JY | 2018-May-14 | 8.8 LD | 10.6 | 53 |
1999 LK1 | 2018-May-15 | 13.3 LD | 10 | 141 |
2018 JX1 | 2018-May-15 | 9.4 LD | 7.7 | 18 |
2010 WC9 | 2018-May-15 | 0.5 LD | 12.8 | 71 |
2018 JX | 2018-May-16 | 3.9 LD | 13 | 77 |
2018 JC | 2018-May-17 | 17.7 LD | 9.4 | 77 |
2018 GL1 | 2018-May-18 | 14.3 LD | 5.2 | 69 |
2018 JL2 | 2018-May-19 | 10.9 LD | 13.5 | 40 |
2018 JG1 | 2018-May-20 | 5.3 LD | 8.3 | 44 |
2018 JK | 2018-May-22 | 16.3 LD | 12.5 | 81 |
2018 JG2 | 2018-May-25 | 18.5 LD | 6.9 | 62 |
68347 | 2018-May-29 | 9.5 LD | 13.3 | 389 |
2013 LE7 | 2018-May-31 | 17.8 LD | 1.7 | 12 |
2018 EJ4 | 2018-Jun-10 | 5.6 LD | 6.2 | 195 |
2015 DP155 | 2018-Jun-11 | 9 LD | 4.4 | 170 |
2017 YE5 | 2018-Jun-21 | 15.6 LD | 15.5 | 513 |
467309 | 2018-Jun-23 | 17.9 LD | 14 | 355 |
441987 | 2018-Jun-24 | 7.3 LD | 12.6 | 178 |
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 |
Readers, thank you for your patience while we continue to develop this new section of Spaceweather.com. We've been working to streamline our data reduction, allowing us to post results from balloon flights much more rapidly, and we have developed a new data product, shown here:
This plot displays radiation measurements not only in the stratosphere, but also at aviation altitudes. Dose rates are expessed as multiples of sea level. For instance, we see that boarding a plane that flies at 25,000 feet exposes passengers to dose rates ~10x higher than sea level. At 40,000 feet, the multiplier is closer to 50x. These measurements are made by our usual cosmic ray payload as it passes through aviation altitudes en route to the stratosphere over California.
What is this all about? Approximately once a week, Spaceweather.com 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. Furthermore, there are studies ( #1, #2, #3, #4) linking cosmic rays with cardiac arrhythmias and sudden cardiac death in the general population. Our latest measurements show that cosmic rays are intensifying, with an increase of more than 13% since 2015:
Why are cosmic rays intensifying? The main reason is the sun. Solar storm clouds such as coronal mass ejections (CMEs) sweep aside cosmic rays when they pass by Earth. During Solar Maximum, CMEs are abundant and cosmic rays are held at bay. Now, however, the solar cycle is swinging toward Solar Minimum, allowing cosmic rays to return. Another reason could be the weakening of Earth's magnetic field, which helps protect us from deep-space radiation.
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.
The data points in the graph above correspond to the peak of the Reneger-Pfotzer maximum, which lies about 67,000 feet above central California. When cosmic rays crash into Earth's atmosphere, they produce a spray of secondary particles that is most intense at the entrance to the stratosphere. Physicists Eric Reneger and Georg Pfotzer discovered the maximum using balloons in the 1930s and it is what we are measuring today.
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