Showing posts with label fireballs. Show all posts
Showing posts with label fireballs. Show all posts

Tuesday, November 3, 2015

Earth approaching objects - November 3rd, 2015

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Image Source  NASA
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All Sky Fireball Network

By Dr. Tony Phillips.


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 Nov. 2, 2015, the network reported 37 fireballs.
(22 sporadics, 14 Northern Taurids, 1 Orionid)


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.
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  Earth approaching objects (objects that are known in the next 30 days)
Object NameApporach DateLeftAU DistanceLD DistanceEstimated Diameter*Relative Velocity
(2010 UJ7)02nd November 20150 day(s)0.158261.622 m - 49 m13.31 km/s47916 km/h
(2015 TG238)03rd November 20151 day(s)0.186572.676 m - 170 m12.02 km/s43272 km/h
(2015 TD179)03rd November 20151 day(s)0.027110.635 m - 78 m10.12 km/s36432 km/h
(2009 LD)05th November 20153 day(s)0.139754.415 m - 34 m9.49 km/s34164 km/h
(2002 XY38)05th November 20153 day(s)0.082832.270 m - 160 m8.85 km/s31860 km/h
(2015 TM143)06th November 20154 day(s)0.069026.851 m - 110 m6.37 km/s22932 km/h
(2015 TL143)06th November 20154 day(s)0.065725.670 m - 160 m8.57 km/s30852 km/h
(2008 VA15)06th November 20154 day(s)0.075029.251 m - 110 m5.47 km/s19692 km/h
(2008 WQ2)08th November 20156 day(s)0.067926.437 m - 82 m8.45 km/s30419.999999999996 km/h
(2012 HG8)08th November 20156 day(s)0.192474.9310 m - 680 m19.44 km/s69984 km/h
138852 (2000 WN10)10th November 20158 day(s)0.125949.0240 m - 540 m13.78 km/s49608 km/h
(2010 XC15)10th November 20158 day(s)0.150858.7140 m - 310 m12.75 km/s45900 km/h
(2005 UN)12th November 201510 day(s)0.155060.318 m - 39 m8.59 km/s30924 km/h
(2000 WP19)15th November 201513 day(s)0.058622.880 m - 180 m10.43 km/s37548 km/h
(2012 LA11)16th November 201514 day(s)0.067826.416 m - 36 m4.88 km/s17568 km/h
(2009 WN6)18th November 201516 day(s)0.108742.331 m - 68 m10.02 km/s36072 km/h
(2015 TO178)18th November 201516 day(s)0.091335.533 m - 75 m6.19 km/s22284 km/h
413577 (2005 UL5)19th November 201517 day(s)0.01535.9240 m - 540 m18.99 km/s68364 km/h
(2002 VV17)19th November 201517 day(s)0.158261.6270 m - 590 m10.26 km/s36936 km/h
(2005 UJ6)20th November 201518 day(s)0.158061.5130 m - 300 m17.60 km/s63360.00000000001 km/h
(2005 EW169)21st November 201519 day(s)0.094036.6400 m - 900 m8.90 km/s32040 km/h
(2015 RQ82)23rd November 201521 day(s)0.073928.797 m - 220 m8.24 km/s29664 km/h
(2011 YS62)23rd November 201521 day(s)0.091535.6310 m - 680 m14.10 km/s50760 km/h
(2009 WB105)24th November 201522 day(s)0.038515.058 m - 130 m18.88 km/s67968 km/h
(2010 YC1)26th November 201524 day(s)0.194875.8150 m - 330 m14.08 km/s50688 km/h
(2004 BG41)26th November 201524 day(s)0.077030.035 m - 78 m10.25 km/s36900 km/h
(2012 XA133)26th November 201524 day(s)0.113444.1180 m - 390 m26.99 km/s97164 km/h
(2011 HJ7)26th November 201524 day(s)0.089334.8100 m - 230 m13.57 km/s48852 km/h
(2015 LE21)27th November 201525 day(s)0.112643.831 m - 68 m3.71 km/s13356 km/h
163696 (2003 EB50)28th November 201526 day(s)0.125448.81.4 km - 3.1 km23.68 km/s85248 km/h
(2007 EA26)28th November 201526 day(s)0.111543.4210 m - 470 m8.19 km/s29484 km/h
(1999 VN6)29th November 201527 day(s)0.186572.6350 m - 780 m12.33 km/s44388 km/h
345722 (2007 BG29)30th November 201528 day(s)0.139054.1670 m - 1.5 km11.26 km/s40536 km/h
(2014 WM7)30th November 201528 day(s)0.079631.051 m - 110 m10.08 km/s36288 km/h
(2005 XT77)01st December 201529 day(s)0.167965.3180 m - 390 m9.70 km/s34920 km/h
1 AU = ~150 million kilometers,1 LD = Lunar Distance = ~384,000 kilometersSource: NASA-NEO
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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.
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Friday, October 9, 2015

Signs Of Change 2015 Part 6 September | Devastating Deluge

HawkkeyDavisChannel
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Saturday, December 28, 2013

Meteor over Southern California/Live Radio Show

BPEarthWatch BPEarthWatch·


   



Published on Dec 28, 2013
Reports of a large meteor over the San Diego Area.http://amsmeteors.org/members/firebal....
Live Show Today on Blogtalk http://www.blogtalkradio.com/bpearthw... and Livestreamhttp://new.livestream.com @ 12 noon central 1 pm Eastern.. Look under BPEARTHWATCH.

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Observing
The Quadrantid meteor shower is one of the strongest meteor showers of the year, but observers can be disappointed if conditions are not just right. The point from where the Quadrantid meteors appear to radiate is located within the extinct constellation Quadrans Muralis. On modern star charts, this radiant is located where the constellations Hercules, Boötes, and Draco meet in the sky. The shower can appear almost nonexistent until about 11 p.m. Unfortunately, the radiant does not attain a very high altitude for most Northern Hemisphere observers before morning twilight puts an end to the show. The best observations are actually possible from countries with high northern latitudes, such as Canada, Finland, Sweden, and Norway. The display is virtually nonexistent for observers in the Southern Hemisphere.
The Quadrantids generally begin on December 28 and end on January 7, with maximum generally occurring during the morning hours of January 3/4. The Quadrantids are barely detectable on the beginning and ending dates, but observers in the Northern Hemisphere can see from 10 to around 60 meteors per hour at maximum. The maximum only lasts for a few hours.
There are other, weaker meteor showers going on around the same time as the Quadrantids. The Quadrantids are medium-paced when compared to meteors from other meteor showers. When you see a meteor, mentally trace it backwards. If you end up where Hercules, Boötes, and Draco meet in the sky then you have probably seen a Quadrantid meteor! If you are not sure where the Quadrantid radiant is in the sky, the following chart will help you find it from the Northern Hemisphere:
Location of the Quadrantids
For Northern Hemisphere Observers
This represents the view from mid-northern latitudes at about 1:00 a.m. local time around January 4. The graphic does not represent the view at the time of maximum, but is simply meant to help prospective observers to find the radiant location. The red line across the bottom of the image represents the horizon. (Image produced by the Author using SkyChart III and Adobe Photoshop.)

Read More Here
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timcline.org

FIREBALL 12-26-2013....

The big Iowa fireball on 12-26-2013....
In the image below,,the fireball is the bright streak in the upper right corner,,just above the horizon....This would be north towards Des Moines....
meteor

meteor
Watch Video Here
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Spaceweather.com



 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 Spaceweather.com.
On Dec. 27, 2013, the network reported 16 fireballs.
(13 sporadics, 2 December Leonis Minorids, 1 December Hydrid)
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]
On Dec. 26, 2013, the network reported 24 fireballs.
(21 sporadics, 3 December Leonis Minorids)
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]

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