Confirmation Images of the Near-Earth Object 2015 PK9 on 2015-08-10

The Near-Earth Object  2015 PK9 (Orbit type: Apollo ) was first observed at SONEAR Observatory, Oliveira.(MPC code Y00)  on 2015 08 10.10036. The asteroid has an approximate diameter 49 m - 110 m ( Absolute Magnitude:  H= 23.651). This  asteroid made  a close-approach  to Earth on 2015-08-07 Nominal Distance (AU) : 0.0148213183067307 (5.768 Lunar Distances). The asteroid's  Earth MOID (Minimum Orbit Intersection Distance) is  0.013686 AU (5.326 Lunar Distances). The last published Observations was made at: 2015 08 11.54955. At the time of this 122 observations have been made and the orbit has as uncertainty of  6.

Observing Run of  2015 PK9 of 2015-08-10 from Auberry California USA - MPC U69

While 2015 PK9 was on the NEO Confirmation Page in an effort to help in the confirmation I obtain 55-15 Second Luminance BIN2 Taken using  iTelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD)  Auberry California USA - MPC U69 created 5 stacks 10 images.
.

Astrometrica object verification wind a stack(1 of 5) of 10-15 Second Luminance BIN2 Taken with iTelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD)  Auberry California USA - MPC U69

Astrometrica object verification wind a stack(2 of 5) of 10-15 Second Luminance BIN2 Taken with iTelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD)  Auberry California USA - MPC U69

Astrometrica object verification wind a stack(3 of 5) of 10-15 Second Luminance BIN2 Taken with iTelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD)  Auberry California USA - MPC U69

Astrometrica object verification wind a stack(4 of 5) of 10-15 Second Luminance BIN2 Taken with iTelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD)  Auberry California USA - MPC U69

Astrometrica object verification wind a stack(5 of 5) of 10-15 Second Luminance BIN2 Taken withiTelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD)  Auberry California USA - MPC U69

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Observing Run of  2015 PK9 of 2015-08-10 from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

  I was obtain 22-15 Second Luminance BIN2 Taken using  iTelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD) , at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62) and did did data reduction on four images.

Astrometrica object verification wind a (1 of 22) 15 Second Luminance BIN2 Images on iTelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Astrometrica object verification wind a (7 of 22) 15 Second Luminance BIN2 Images on iTelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Astrometrica object verification wind a (14 of 22) 15 Second Luminance BIN2 Images on iTelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Astrometrica object verification wind a (22 of 22) 15 Second Luminance BIN2 Images oniTelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Other links:

• The Discovery M.P.E.C.:  MPEC 2015-P28 : 2015 PK9
• (MPC) Observations of 2015 PK9
•  JPL Orbit Diagram 2015 PK9  
• Near Earth Objects Dynamic Site--2015 PK9 
• NEO Earth Close Approaches (JPL)
• The Tracking News 
• NEO Coordination Centre

Confirmation Images of the Near-Earth Object 2015 LF on 2015-06-07

The Near-Earth Object 2015 LF (Orbit type: Apollo ) was first observed by the Catalina Sky Survey(MPC code 703) on 2015 06 07. The asteroid has an approximate diameter of 13 m - 31 m ( ~45 foot - 102 foot) ( H=26.4) and will make a close approach to earth on 2015-Jun-08 at ~ 23:49 UT (06:49 PM CDT) at an approximate distance of 0.00131Astronomical Units ( 0.51 Lunar Distances) or 121,772.108 Miles (195,973.211 KM).

While 2015 LF was on the NEO Confirmation Page in an effort to help in the confirmation I ran three series of 30 -- 10 Second Luminance BIN2 Images on itelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD) at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62) and created 4 stacks 15 images (run number one was not used due to poor sky).

Astrometrica object verification wind a stacks 15- 10 Second Luminance BIN2 Images on itelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Astrometrica object verification wind a stacks 15- 10 Second Luminance BIN2 Images on itelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Astrometrica object verification wind a stacks 15- 10 Second Luminance BIN2 Images on itelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Astrometrica object verification wind a stacks 15- 10 Second Luminance BIN2 Images on itelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD)  at Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)

Other links:

• MPEC 2015-L17 : 2015 LF
• Observations(MPC)
• JPL Orbit Diagram
• NEODyS-2 
• NEO Earth Close Approaches
• The Tracking News(Earth's Busy Neighborhood)
• Speed of Light - Space - Distance Calculator

The NEO 2015 KA122 ( Orbit type: Apollo ) on 2015-06-01

The  NEO 2015 KA122 ( Orbit type: Apollo ) on 2015-06-01 — Three Stacks of  5 - 20 Second Luminance BIN2 taken with iTelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD) at Sierra Remote Observatory, Auberry, California, USA (MPC Code U69). By Steven M. Tilley ©

Other links:
 JPL  Orbit Diagram
Observations(MPC)
NEODyS-2

The Near-Earth Object (Orbit type: Apollo [PHA] ) 2015 JJ on 2015 05 16 from AstroCamp Observatory, Nerpio, Spain (MPC Code - I89)

The Near-Earth Object (Orbit type: Apollo [PHA] ) 2015 JJ on 2015 05 16 from  AstroCamp Observatory, Nerpio, Spain (MPC Code - I89) —Three Stack of 7-60 Second Luminance BIN2 using itelescope.net’s  (TEL T7 0.43-m f/6.8 astrograph + CCD)  © Steven M. Tilley 2015

NET UCAC-4
     K15J00J KC2015 05 16.89762 14 50 10.17 +18 07 14.3          19.1 V      I89
     K15J00J KC2015 05 16.90473 14 50 09.89 +18 07 48.5          19.2 V      I89
     K15J00J KC2015 05 16.91182 14 50 09.63 +18 08 22.9          19.2 V      I89
----- end -----

The Asteroid 2015 AZ43 On 2015-02-14 From Mayhill, New Mexico (New Mexico Skies) - MPC H06

The Near-Earth Object(Orbit type: Apollo ) 2015 AZ43 was first observed by Pan-STARRS 1 on 2015-01-11 and has been listed as a Virtual Impactor by SENTRY (JPL). 2015 AZ43 has a VERY SMALL impact risk(0.012%) for the date 2107-02-27.19. With more observations this risk could be rule out. In an effort to help improve the orbit I ran a imaging run from Mayhill, New Mexico (New Mexico Skies) - MPC H06 using itelescope.net's(TEL  T21 0.43-m f/6.8 astrograph + CCD + f/4.5 focal reducer) on 2015-02-14.

A Stack of 20-10 Second Luminance BIN2
Taken with Itelescope.net's
(TEL  T21 0.43-m f/6.8 astrograph + CCD + f/4.5 focal reducer)
Mayhill, New Mexico (New Mexico Skies) - MPC H06

A Stack of 20-10 Second Luminance BIN2
Taken with Itelescope.net's
(TEL  T21 0.43-m f/6.8 astrograph + CCD + f/4.5 focal reducer)
Mayhill, New Mexico (New Mexico Skies) - MPC H06

A Stack of 20-10 Second Luminance BIN2
Taken with Itelescope.net's
(TEL  T21 0.43-m f/6.8 astrograph + CCD + f/4.5 focal reducer)
Mayhill, New Mexico (New Mexico Skies) - MPC H06

Useful links:  
Understanding Risk Pages by Jon Giorgini
 Palermo Scale   
Torino Scale   
The Tracking News   
NEODyS CLOMON2 risk page 
List of removed objects(JPL) 

Note:  At 2015-02-23 22:01 UTC  --  2015 AZ43  was removed from the JPL Sentry Risk list.

 

The Asteroid 2015 AZ43 On 2015-02-13 from Auberry California USA - MPC U69

The Near-Earth Object(Orbit type: Apollo ) 2015 AZ43 was first observed by Pan-STARRS 1 on 2015-01-11 and has been listed as a Virtual Impactor by SENTRY (JPL). 2015 AZ43 has a VERY SMALL impact risk(0.012%) for the date 2107-02-27.19. With more observations this risk could be rule out. In an effort to help improve the orbit I ran a imaging run from Auberry California USA - MPC U69 using itelescope.net's (TEL T24 0.61-m f/6.5 astrograph + CCD) on 2015-02-13.

A Stack of 5-10 Second Luminance BIN2
Taken with Itelescope.net's
(TEL T24 0.61-m f/6.5 astrograph + CCD)
Auberry California USA - MPC U69

A Stack of 5-10 Second Luminance BIN2
Taken with Itelescope.net's
(TEL T24 0.61-m f/6.5 astrograph + CCD)
Auberry California USA - MPC U69

A Stack of 5-10 Second Luminance BIN2
Taken with Itelescope.net's
(TEL T24 0.61-m f/6.5 astrograph + CCD)
Auberry California USA - MPC U69

Useful links:
Understanding Risk Pages by Jon Giorgini
Palermo Scale 
Torino Scale  
The Tracking News   
NEODyS CLOMON2 risk page
 List of removed objects(JPL) 

Note:  At 2015-02-23 22:01 UTC  --  2015 AZ43  was removed from the JPL Sentry Risk list.

The Asteroid 2015 AZ43 On 2015-02-07 and 8 From Mayhill, New Mexico (New Mexico Skies) - MPC H06

 The Near-Earth Object(Orbit type: Apollo ) 2015 AZ43 was first observed by Pan-STARRS 1 on 2015-01-11 and has been listed as a Virtual Impactor by SENTRY (JPL). 2015 AZ43 has a VERY SMALL impact risk(0.017%) for the date 2107-02-27.19. With more observations this risk could be rule out. In an effort to help improve the orbit I made two imaging run from Mayhill, New Mexico (New Mexico Skies) - MPC H06 using itelescope.net's(TEL T11 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer) on two nights one 2015-02-07 and the other on 2015-02-08.

see this on Flickr

Useful links:  
Understanding Risk Pages by Jon Giorgini
 Palermo Scale  
Torino Scale  
The Tracking News  
NEODyS CLOMON2 risk page
 List of removed objects(JPL) 

Note:  At 2015-02-23 22:01 UTC  --  2015 AZ43  was removed from the JPL Sentry Risk list.

 

The Asteroid 2015 AZ43 On 2015-02-06 From Mayhill, New Mexico (New Mexico Skies) - MPC H06

The Near-Earth Object(Orbit type: Apollo ) 2015 AZ43 was first observed by Pan-STARRS 1 on 2015-01-11 and has been listed as a Virtual Impactor by SENTRY (JPL). 2015 AZ43 has a VERY SMALL impact risk(0.013%) for the date 2107-02-27.19. With more observations this risk could be rule out. In an effort to help improve the orbit I made two imaging run from Mayhill, New Mexico (New Mexico Skies) - MPC H06 using itelescope.net's(TEL T11 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer) on 2015-02-06.

see this on Flickr

Useful links:
Understanding Risk Pages by Jon Giorgini
Palermo Scale
Torino Scale
The Tracking News
NEODyS CLOMON2 risk page
List of removed objects(JPL) 

Note:  At 2015-02-23 22:01 UTC  --  2015 AZ43  was removed from the JPL Sentry Risk list.
 

The Asteroid (357439) = 2004 BL86 On 2015-02-03

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) (estimated to be 325  meters in diameter) made a Close-Approach of 3.1 Lunar Distance on 26 January 2015.and was map with Radar Observations.


(Orbit type: Apollo ) [NEO]

38 -- 15 Second Luminance BIN1 Images

from ITelescope.Net

(T11 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer)

MPC Code H06 (Mayhill, New Mexico, USA)

2015-02-03 03:04 UTC to 03:29 UTC


(c) Steven M. Tilley
http://lagniappeobserving.blogspot.com/
Useful Links:

• Remanzacco Observatory - Comets & Neo: Close Approach of Asteroid (357439) 2004 BL86
• Updated Charts for Asteroid 2004 BL86 Earth Flyby on Jan 26, 2015 (JPL)
• Asteroid to fly by Earth safely January 26(Astronomy Magazine)
• Asteroid 2004 BL86 to sweep close on January 26(EarthSky)
• Big Asteroid 2004 BL86 Buzzes Earth on January 26: How to See it in Your Telescop(Universe Today)
• Big Asteroid to Zoom by Earth on Jan. 26(space.com)
• Asteroid to Fly By Earth Safely on January 26 (Jet Propulsion Laboratory, Pasadena, Calif.; January 13, 2015)
• Observations(MPC)
• Orbital Elements (JPL)
• (357439) 2004BL86 -- ESA Space Situational Awareness
• (357439) 2004BL86 Ephemerides for 25 January 2015 through 29 January(NEODyS-2)
• Goldstone Radar Observations Planning
• Goldstone Asteroid Schedule
• Planetary Radar at Arecibo Observatory
• JPL Absolute Magnitude table (H)
• Abstract for Run 3579(Caltech)
• Goldstone Solar System Radar by Marina Brozović,Jet Propulsion Laboratory, California Institute of Technology
• Wikipedia (357439) 2004 BL86

The Asteroid (357439) = 2004 BL86 On 2015-01-25

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) (estimated to be 440–1000 meters in diameter) will safely make a Close-Approach of 3.1 Lunar Distance on 26 January 2015. This will be the closest known Approach by something this large (H = 19.0) until 2027, and will briefly peak at around apparent magnitude 9.0 It has been schedule for Goldstone Observations(2015 Jan 27-Feb 1).
The Asteroid (357439) = 2004 BL86 On 2015-01-25
from Siding Spring Observatory,Coonabarabran, NSW, Australia.(MPC Code Q62)
100 -- 5 Second Luminance BIN1
taken with iTelescope Net's
Telescope T31
2015-01-25 10:36 UTC to 11:20 UT

Object verification windows done with Astrometrica

"(c) Steven M. Tilley http://lagniappeobserving.blogspot.com/"

Useful Links:

• Remanzacco Observatory - Comets & Neo: Close Approach of Asteroid (357439) 2004 BL86
• Updated Charts for Asteroid 2004 BL86 Earth Flyby on Jan 26, 2015 (JPL)
• Asteroid to fly by Earth safely January 26(Astronomy Magazine)
• Asteroid 2004 BL86 to sweep close on January 26(EarthSky)
• Big Asteroid 2004 BL86 Buzzes Earth on January 26: How to See it in Your Telescop(Universe Today)
• Big Asteroid to Zoom by Earth on Jan. 26(space.com)
• Asteroid to Fly By Earth Safely on January 26 (Jet Propulsion Laboratory, Pasadena, Calif.; January 13, 2015)
• Observations(MPC)
• Orbital Elements (JPL)
• (357439) 2004BL86 -- ESA Space Situational Awareness
• (357439) 2004BL86 Ephemerides for 25 January 2015 through 29 January(NEODyS-2)
• Goldstone Radar Observations Planning
• Goldstone Asteroid Schedule
• Planetary Radar at Arecibo Observatory
• JPL Absolute Magnitude table (H)
• Abstract for Run 3579(Caltech)
• Goldstone Solar System Radar by Marina Brozović,Jet Propulsion Laboratory, California Institute of Technology
• Wikipedia (357439) 2004 BL86

Imaging Run on (357439) 2004 BL86 from MPC Q62 Plan for 2015-01-24

On the (2015-01-24) starting at 10:50 UTC, I plan to be imaging (357439) 2004 BL86 from Siding Spring, Australia (MPC Q62) [itelescope.net] on (TEL T30 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer) I will be taking 5 Second Luminance BIN1 Images and hope to get up to 100 of (357439) 2004 BL86.

Background

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) (estimated to be 440–1000 meters in diameter) will safely make a Close-Approach of 3.1 Lunar Distance on 26 January 2015. This will be the closest known Approach by something this large (H = 19.0) until 2027, and will briefly peak at around apparent magnitude 9.0 It has been schedule for Goldstone Observations(2015 Jan 27-Feb 1).

Videos from past runs on  (357439) 2004 BL86:




Useful Links:

• Remanzacco Observatory - Comets & Neo: Close Approach of Asteroid (357439) 2004 BL86
• Updated Charts for Asteroid 2004 BL86 Earth Flyby on Jan 26, 2015 (JPL)
• Asteroid to fly by Earth safely January 26(Astronomy Magazine)
• Asteroid 2004 BL86 to sweep close on January 26(EarthSky)
• Big Asteroid 2004 BL86 Buzzes Earth on January 26: How to See it in Your Telescop(Universe Today)
• Big Asteroid to Zoom by Earth on Jan. 26(space.com)
• Asteroid to Fly By Earth Safely on January 26 (Jet Propulsion Laboratory, Pasadena, Calif.; January 13, 2015)
• Observations(MPC)
• Orbital Elements (JPL)
• (357439) 2004BL86 -- ESA Space Situational Awareness
• (357439) 2004BL86 Ephemerides for 25 January 2015 through 29 January(NEODyS-2)
• Goldstone Radar Observations Planning
• Goldstone Asteroid Schedule
• Planetary Radar at Arecibo Observatory
• JPL Absolute Magnitude table (H)
• Abstract for Run 3579(Caltech)
• Goldstone Solar System Radar by Marina Brozović,Jet Propulsion Laboratory, California Institute of Technology
• Wikipedia (357439) 2004 BL86

The Asteroid (357439) = 2004 BL86 On the Night of 2015-01-17

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) (estimated to be 440–1000 meters in diameter) will safely make a Close-Approach of 3.1 Lunar Distance on 26 January 2015. This will be the closest known Approach by something this large (H = 19.0) until 2027, and will briefly peak at around apparent magnitude 9.0 It has been schedule for Goldstone Observations(2015 Jan 27-Feb 1).


The Asteroid (357439) = 2004 BL86 On the Night of 2015-01-17
For Siding Spring Observatory,Coonabarabran, NSW, Australia.(MPC Code Q62)
50 -- 30 Second Luminance BIN1
taken with iTelescope Net's
Telescope T30
(0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer)
2015-01-17 10:47 UTC to 11:39 UT
(c) Steven M. Tilley


APPROVED for web embedding and media broadcasts with full and complete attribution TO: (c) Steven M. Tilley http://lagniappeobserving.blogspot.com 

The Asteroid (357439) = 2004 BL86 On the Night of 2015-01-17 From Siding Spring Observatory,Coonabarabran, NSW, Australia.(MPC Code Q62)a stack of 50 -- 30 Second Luminance BIN1taken with iTelescope Net  Telescope T30(0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer)2015-01-17 10:47 UTC to 11:39 UT (c) Steven M. Tilley

 Links:
Asteroid to fly by Earth safely January 26(Astronomy Magazine)
Asteroid 2004 BL86 to sweep close on January 26(EarthSky)
Big Asteroid 2004 BL86 Buzzes Earth on January 26: How to See it in Your Telescop(Universe Today)
Big Asteroid to Zoom by Earth on Jan. 26(space.com)
Asteroid to Fly By Earth Safely on January 26 (Jet Propulsion Laboratory, Pasadena, Calif.; January 13, 2015)
Observations(MPC)
Orbital Elements (JPL)
(357439) 2004BL86 -- ESA Space Situational Awareness
(357439) 2004BL86 Ephemerides for 25 January 2015 through 29 January(NEODyS-2)
Goldstone Radar Observations Planning
Goldstone Asteroid Schedule
Planetary Radar at Arecibo Observatory
JPL Absolute Magnitude table (H)
Abstract for Run 3579(Caltech)
Goldstone Solar System Radar by Marina Brozović,Jet Propulsion Laboratory, California Institute of Technology
Wikipedia (357439) 2004 BL86

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) from Siding Spring - Australia - MPC Q62 on 2015-01-17

The NEO (357439) 2004 BL86  (Orbit type: Apollo ) from Siding Spring - Australia - MPC Q62 on 2015-01-17 4 - 30 Second Luminance BIN1 taken with (TEL T30 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer)   [iTelescope.Net ] 

Imaging Run on (357439) 2004 BL86 from MPC Q62 Plan for Tonight

Tonight (2015-01-14) starting at 10:40 UTC, I plan to be imaging (357439) 2004 BL86 from Siding Spring, Australia (MPC Q62) [itelescope.net] on (TEL T27 0.70-m f/6.6 CDK astrograph + CCD). I will be taking 60 Second Luminance BIN1 Images and hope to get up to 90 before (357439) 2004 BL86 dips below the minimum target elevation limit of TEL T27.

The NEO (357439) 2004 BL86 On the Night of 2015-01-03

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) (estimated to be 440–1000 meters in diameter) will safely make a Close-Approach of 3.1 Lunar Distance on 27 January 2015. This will be the closest "known" Approach by something this large (H = 18.8) until 2027, and may will briefly peak at around apparent magnitude 9. It has been schedule for Goldstone Observations(2015 Jan 27-Feb 1).
The NEO (357439) 2004 BL86 On the Night of 2015-01-03 from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62) 3 stacks of 15 - 60 Second Luminance BIN2 Images (Sky Motion 0.510"/min P.A.100.5| 0.524"/min P.A.99.4| 0.541"/min P.A.98.5) taken with iTelescope.Net's (TEL T32 0.43-m f/6.8 astrograph + CCD)
stack 1:2015 01 03.46767(11:13:26 UT)
stack 2:2015 01 03.48579(11:39:32 UT)
stack 3:2015 03 03.50430(12:06:11 UT)
(C) Steven M. Tilley

Links:
Asteroid to Fly By Earth Safely on January 26 (Jet Propulsion Laboratory, Pasadena, Calif.; January 13, 2015)
Observations(MPC)
Orbital Elements (JPL)
(357439) 2004BL86 -- ESA Space Situational Awareness
Goldstone Radar Observations Planning
(357439) 2004BL86 Ephemerides for 25 January 2015 through 29 January(NEODyS-2)
Goldstone Asteroid Schedule
Planetary Radar at Arecibo Observatory
JPL Absolute Magnitude table (H)
Abstract for Run 3579(Caltech)
Goldstone Solar System Radar by Marina Brozović,Jet Propulsion Laboratory, California Institute of Technology
Wikipedia (357439) 2004 BL86

The NEO (357439) 2004 BL86 On the Night of 2015-01-03-Data

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) from Siding Spring - Australia - MPC Q62 on 2015-01-03 3 stacks of 15 - 60 Second Luminance BIN2 (Sky Motion 0.510"/min P.A.100.5| 0.524"/min P.A.99.4| 0.541"/min P.A.98.5) taken with (TEL T32 0.43-m f/6.8 astrograph + CCD) [iTelescope.Net ]

The NEO (357439) 2004 BL86 On the Night of 2014-12-29

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) (estimated to be 440–1000 meters in diameter) will safely make a Close-Approach of 3.1 Lunar Distance on 27 January 2015. This will be the closest "known" Approach by something this large (H = 18.8) until 2027, and may will briefly peak at around apparent magnitude 9. It has been schedule for Goldstone Observations(2015 Jan 27-Feb 1).
The NEO (357439) 2004 BL86 On the Night of 2014-12-29 from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62) 3 stacks of 6 - 60 Second Luminance BIN2 Images (Sky Motion: 0.549"/min P.A.98.4;0.556"/min P.A.98.1;0.562"/min P.A.97.8) taken with iTelescope.Net 's (TEL T30 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer) stack 1:2014 12 29.49558(11:53:38 UT) stack 2:2014 12 29.50487(12:07:01 UT) stack 3:2014 12 29.51289(12:18:34 UT) (C)Steven M. Tilley

Links:
Asteroid to Fly By Earth Safely on January 26 (Jet Propulsion Laboratory, Pasadena, Calif.; January 13, 2015)
Observations(MPC)
 Orbital Elements (JPL) (357439) 2004BL86 -- ESA Space Situational Awareness
Goldstone Radar Observations Planning
(357439) 2004BL86 Ephemerides for 25 January 2015 through 29 January(NEODyS-2)
Goldstone Asteroid Schedule Planetary Radar at Arecibo Observatory
JPL Absolute Magnitude table (H) Abstract for Run 3579(Caltech)
 Goldstone Solar System Radar by Marina Brozović,Jet Propulsion Laboratory, California Institute of Technology
Wikipedia (357439) 2004 BL86

The NEO (357439) 2004 BL86 On the Night of 2014-12-29-Data

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) from Siding Spring - Australia - MPC Q62 on 2014-12-29 3 stacks of 6 - 60 Second Luminance BIN2 (Sky Motion 0.549"/min P.A.98.4, 0.556"/min P.A.98.1, 0.562"/min P.A.97.8) taken with ((TEL T30 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer) [iTelescope.Net ]

The NEO (357439) 2004 BL86 On the Night of 2014-12-20

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) (estimated to be 440–1000 meters in diameter) will safely make a Close-Approach of 3.1 Lunar Distance on 27 January 2015. This will be the closest "known" Approach by something this large (H = 18.8) until 2027, and may will briefly peak at around apparent magnitude 9. It has been schedule for Goldstone Observations(2015 Jan 27-Feb 1).
The NEO (357439) 2004 BL86 On the Night of 2014-12-20 from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62) 3 stacks of 10 - 60 Second Luminance BIN2 Images (Sky Motion 0.605"/min P.A.98.7) taken with itelescope.net's (TEL T27 0.70-m f/6.6 CDK astrograph + CCD) stack 1:2014 12 20.47669(11:26:26 UT) stack 2:2014 12 20.48956(11:44:58 UT) stack 3:2014 12 20.51334(12:19:12 UT) (C)Steven M. Tilley
Links:
Asteroid to Fly By Earth Safely on January 26 (Jet Propulsion Laboratory, Pasadena, Calif.; January 13, 2015)
Observations(MPC)
 Orbital Elements (JPL) (357439) 2004BL86 -- ESA Space Situational Awareness
Goldstone Radar Observations Planning
(357439) 2004BL86 Ephemerides for 25 January 2015 through 29 January(NEODyS-2)
Goldstone Asteroid Schedule Planetary Radar at Arecibo Observatory
JPL Absolute Magnitude table (H) Abstract for Run 3579(Caltech)
 Goldstone Solar System Radar by Marina Brozović,Jet Propulsion Laboratory, California Institute of Technology
Wikipedia (357439) 2004 BL86

The NEO (357439) 2004 BL86 On the Night of 2014-12-20-Data

The NEO (357439) 2004 BL86 (Orbit type: Apollo ) from Siding Spring - Australia - MPC Q62 on 2014-12-20 3 stacks of 10 - 60 Second Luminance BIN2 (Sky Motion 0.605"/min P.A.98.7) taken with (TEL T27 0.70-m f/6.6 CDK astrograph + CCD) [iTelescope.Net ]