Confirmation images of the NEO 2018 HC1

A confirmation image of the NEO 2018 HC1 on
2018-04-21 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 15 - 05 Second Luminance BIN2
images taken with iTelescope.net's
(T30 TEL 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

A confirmation image of the NEO 2018 HC1 on
2018-04-21 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 15 - 05 Second Luminance BIN2
images taken with iTelescope.net's
(T30 TEL 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

A confirmation image of the NEO 2018 HC1 on
2018-04-21 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 15 - 05 Second Luminance BIN2
images taken with iTelescope.net's
(T30 TEL 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

The Artificial Satellite 1983-020D on 2018-04-08

The NEO 2018 BY2 - Information Sheet

The NEO 2018 BY2 on 2018-03-31 from Mayhill, New Mexico
(New Mexico Skies) - (MPC Code H06) a stack of 9 - 20 Second Luminance 
BIN2 Images taken with iTelescope.net's
(T21 TEL 0.43-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

The NEO 2018 BY2 on 2018-03-31 from Mayhill, New Mexico
(New Mexico Skies) - (MPC Code H06) a stack of 9 - 20 Second Luminance 
BIN2 Images taken with iTelescope.net's
(T21 TEL 0.43-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

The NEO 2018 BY2 on 2018-03-31 from Mayhill, New Mexico
(New Mexico Skies) - (MPC Code H06) a stack of 9 - 20 Second Luminance 
BIN2 Images taken with iTelescope.net's
(T21 TEL 0.43-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

The NEO 2018 BY2 on 2018-03-31 from Mayhill, New Mexico
(New Mexico Skies) - (MPC Code H06) a stack of 9 - 20 Second Luminance 
BIN2 Images taken with iTelescope.net's
(T21 TEL 0.43-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-02 from Sierra Remote Observatory,
Auberry, California, USA (MPC U69) a stack of 10 - 15 Second Luminance BIN2 Images
taken with iTelescope.net's (T24 TEL 0.61-m f/6.5 reflector + CCD) 
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-02 from Sierra Remote Observatory,
Auberry, California, USA (MPC U69) a stack of 10 - 15 Second Luminance BIN2 Images 
taken with iTelescope.net's (T24 TEL 0.61-m f/6.5 reflector + CCD) 
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-02 from Sierra Remote Observatory,
Auberry, California, USA (MPC U69) a stack of 10 - 15 Second Luminance BIN2 Images 
taken with iTelescope.net's (T24 TEL 0.61-m f/6.5 reflector + CCD) 
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-02 from Sierra Remote Observatory,
Auberry, California, USA (MPC U69) a stack of 10 - 15 Second Luminance BIN2 Images 
taken with iTelescope.net's (T24 TEL 0.61-m f/6.5 reflector + CCD) 
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-02 from Sierra Remote Observatory,
Auberry, California, USA (MPC U69) a stack of 10 - 15 Second Luminance BIN2 Images 
taken with iTelescope.net's (T24 TEL 0.61-m f/6.5 reflector + CCD) 
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-05 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62) a stack of 20 - 15 Second Luminance BIN2
 Images taken with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-05 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62) a stack of 20 - 15 Second Luminance BIN2
 Images taken with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-05 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62) a stack of 20 - 15 Second Luminance BIN2
 Images taken with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-05 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62) a stack of 20 - 15 Second Luminance BIN2
 Images taken with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD) By Steven M. Tilley

The NEO 2018 BY2 on 2018-04-05 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62) a stack of 20 - 15 Second Luminance BIN2
 Images taken with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley

 Background

(as of 2018-04-06)

• Object: 2018 BY2
• Orbit Type: Apollo [NEO, PHA]
• Approximate Diameter: 210 m - 470 m ( 688.976  feet to 1541.995  feet) (Absolute Magnitude: H= 20.5)
• On the Sentry Risk Table: NO
• On the NEODyS CLOMON2 risk page: NO 
• First(Precovery) Observation was made: 2018 01 03.45659
• Discovery observation was made on: 2018 01 17.31782
• Discovery observation was made by Pan-STARRS 1, Haleakala (MPC Code F51) The Discovery M.P.E.C.:MPEC 2018-B85 : 2018 BY2
• Last Observation (publish): 2018 04 05.42579 (at iTelescope Observatory, Siding Spring,  Australia (MPC Code Q62) )
• Data-Arc Span (publish):  days 92
• Number of Optical Observations(published):146
• Observatories Reporting (Published) Observations(MPC Code):
• (246) Klet Observatory-KLENOT, Czech Republic.
• (474) Mount John Observatory, Lake Tekapo, New Zealand. 
• (568) Mauna Kea, US/Hawaii. 
• (587) Sormano, Italy. 
• (691) Steward Observatory, Kitt Peak - Spacewatch, US/Arizona.
• (703) Catalina Sky Survey, US/Arizona.
• (711) McDonald Observatory, Fort Davis,US/Texas.
• (807) Cerro Tololo Observatory, La Serena,  Chile.
• (A48) Povegliano Veronese, Italy.
• (B74) Santa Maria de Montmagastrell, Spain.
• (F51) Pan-STARRS 1, Haleakala,US/Hawaii.
• (H01) Magdalena Ridge Observatory, Socorro, US/New Mexico. 
• (H06) iTelescope Observatory, Mayhill, US/New Mexico.
• (H21) Astronomical Research Observatory, Westfield, US/Illinois.
• (H36) Sandlot Observatory, Scranton, US/Kansas.
• (H45) Arkansas Sky Obs., Petit Jean Mountain South, US/Arkansas.
• (I52) Steward Observatory, Mt. Lemmon Station,US/Arizona.
• (K61) Rokycany Observatory, Czech Republic.
• (L04) ROASTERR-1 Observatory, Cluj-Napoca, Romania.
• (Q62) iTelescope Observatory, Siding Spring, Australia/NSW.
• (T05) ATLAS-HKO, Haleakala, US/Hawaii.
• (U69) iTelescope SRO Observatory, Auberry,
• (W89) Cerro Tololo-LCO Aqawan A #1, Chile.
• Perihelion Distance 1.014723117954455 (AU)
• Aphelion Distance: 2.264719569328387 (AU)
• Earth MOID (Earth center to NEO center): 0.04159 AU ((16.186 LD)), ( 975.57 Earth radii) or 3,866,032.024  miles ( 6,221,775.442 ( KM))
• Next Close-Approach to Earth:  Will safely pass Earth on 2018-Apr-11:
• Minimum Distance(Earth center to NEO center) of  0.0609381959952516 (AU) ( 23.715 (LD)), 1429.89 (Earth radii) or  5,664,559.202  miles ( 9,116,224.365(KM)) 
• Nominal Distance(Earth center to NEO center) of 0.0609437887594874 (AU) ( 23.718 (LD)), (1430.02  Earth radii) or 5,665,079.082 miles ( 9,117,061.03 (KM))
• Maximum Distance(Earth center to NEO center) of  0.0609493815227982 (AU) ( 23.72 (LD)), (1430.156443 Earth radii) or 5,665,598.962 miles (9,117,897.696 (KM))   

Confirmation of the NEO 2018 FC1

The NEOCP object ZF278E4(now the NEO 2018 FC1) on 2018-03-19
a stack of 20-30 second luminance BIN2 images taken with
 iTelescope.net's (T17 TEL 0.43-m f/6.8 reflector + CCD)
 at Siding Spring Observatory, Coonabarabran, NSW, Australia
(MPC code Q62) 
By Steven M. Tilley

The NEOCP object ZF278E4(now the NEO 2018 FC1) on 2018-03-19
a stack of 20-30 second luminance BIN2 images taken with
 iTelescope.net's (T17 TEL 0.43-m f/6.8 reflector + CCD)
 at Siding Spring Observatory, Coonabarabran, NSW, Australia
(MPC code Q62) 
By Steven M. Tilley

The NEOCP object ZF278E4(now the NEO 2018 FC1) on 2018-03-19
a stack of 20-30 second luminance BIN2 images taken with
 iTelescope.net's (T17 TEL 0.43-m f/6.8 reflector + CCD)
 at Siding Spring Observatory, Coonabarabran, NSW, Australia
(MPC code Q62) 
By Steven M. Tilley

 Background

(as of 2018-02-19)

• Object: 2018 FC1
• Orbit Type: Amor [NEO]
• Approximate Diameter: 120 m - 260 m (393.701 feet to 853.018 feet) (Absolute Magnitude: H= 21.766)
• On the Sentry Risk Table: NO
• On the NEODyS CLOMON2 risk page: NO 
• Discovery observation was made on: 2018 03 17.33572
• Discovery observation was made by Catalina Sky Survey (MPC Code 703) The Discovery M.P.E.C.:MPEC 2018-F40 : 2018 FC1
• Last Observation (publish): 2018 03 19.53148 (at iTelescope Observatory, Siding Spring,  Australia (MPC Code Q62) )
• Data-Arc Span (publish): 2 days 
• Number of Optical Observations(published):42
• Observatories Reporting (Published) Observations(MPC Code):
• (033) Karl Schwarzschild Observatory, Tautenburg, Germany.
• (474) Mount John Observatory, Lake Tekapo, New Zealand.
• (703) Catalina Sky Survey, US/Arizona.
• (734) Farpoint Observatory, Eskridge, US/Kansas.
• (807) Cerro Tololo Observatory, La Serena, Chile.
• (E23) Arcadia, Australia/NSW.
• (I52) Steward Observatory, Mt. Lemmon Station, US/Arizona.
• (Q62) iTelescope Observatory, Siding Spring,  Australia/NSW. 
• Perihelion Distance:1.106589693409455(AU)
• Aphelion Distance: 2.130212399099761(AU)
• Earth MOID (Earth center to NEO center): 0.19123 AU (( 74.421 LD)), (4490.28 Earth radii) or  17775939 miles (  (28607600 KM))
• Next Close-Approach to Earth:  Will safely pass Earth on 2018-Mar-30 at a 
• Minimum Distance(Earth center to NEO center) of 0.192881774004264 (AU) (75.064 (LD)), (4,516.07 Earth radii) or  17,878,004 miles ( (28,854,702 KM)) 
• Nominal Distance(Earth center to NEO center) of 0.196815739374881(AU) ( 76.595 (LD)), ( 4,621.44 Earth radii) or 18,295,166 miles (29,443,216 (KM))
• Maximum Distance(Earth center to NEO center) of 0.20074975749401 (AU) ( 78.126 (LD)), ( 4,713.82 Earth radii) or  18,660,856 miles (30,031,736 (KM))   

Confirmation Images of The Asteroid 2018 BT6

A confirmation image of the asteroid 2018 BT6 (a NEO with an estimated diameter of 150 m to 340 m)
 on 2018-01-30 from from Mayhill, New Mexico [New Mexico Skies] - (MPC Code H06)
a Stack of 12 - 5 Second Luminance BIN2 images taken withitelescope.net's
(T11 TEL 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

A confirmation image of the asteroid 2018 BT6 (a NEO with an estimated diameter of 150 m to 340 m)
 on 2018-01-30 from from Mayhill, New Mexico [New Mexico Skies] - (MPC Code H06) 
a Stack of 12 - 5 Second Luminance BIN2 images taken withitelescope.net's
(T11 TEL 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

A confirmation image of the asteroid 2018 BT6 (a NEO with an estimated diameter of 150 m to 340 m)
 on 2018-01-30 from from Mayhill, New Mexico [New Mexico Skies] - (MPC Code H06) 
a Stack of 12 - 5 Second Luminance BIN2 images taken withitelescope.net's
(T11 TEL 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

A confirmation image of the asteroid 2018 BT6 (a NEO with an estimated diameter of 150 m to 340 m)
 on 2018-01-30 from from Mayhill, New Mexico [New Mexico Skies] - (MPC Code H06) 
a Stack of 73 - 5 Second Luminance BIN2 images taken withitelescope.net's
(T11 TEL 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
By Steven M. Tilley

The asteroid 2018 BT6 (a NEO with an estimated diameter of 150 m to 340 m) made a closest approach to Earth at a distance of 0.05 AU or 18 Lunar Distances(7 million km or 4 million miles) at 2018-01-26.91133. 2018. BT6 was discovered by the Catalina Sky Survey at 2018-01-27.40491.

 Background

(as of 2018-01-30)

• Object: 2018 BT6
• Orbit Type: Apollo [NEO PHA]
• Approximate Diameter: 150 m - 340 m (492.126 feet to 1115.49 feet) (Absolute Magnitude: H= 21.2)
• On the Sentry Risk Table: NO
• On the NEODyS CLOMON2 risk page: NO 
• Discovery observation was made on:2018 01 27.4049
• Discovery observation was made by Catalina Sky Survey (MPC Code 703) The Discovery M.P.E.C.:MPEC 2018-B166: 2018 BT6
• Last Observation (publish):2018 01 30.53575 (by Tenagra II (MPC Code 926) )
• Data-Arc Span (publish): 3 days 
• Number of Optical Observations(published):93
• Observatories Reporting (Published) Observations(MPC Code):
• (104) San Marcello Pistoiese, Italy. 
• (204) Schiaparelli Observatory, Italy
• (703) Catalina Sky Survey, Arizona,US 
• (926) Tenagra II Observatory, Arizona,US
• (C95) SATINO Remote Observatory, Haute Provence, France. 
• (G48) Harlingten Research Observatory, Rancho Hildalgo, New Mexico, US. 
• (H01) Magdalena Ridge Observatory, Socorro, New Mexico, US.
• (H06) iTelescope Observatory, Mayhill, New Mexico, US.
• (H36) Sandlot Observatory, Scranton, Kansas, US. 
• (I52) Steward Observatory, Mt. Lemmon Station, Arizona, US. 
• (J69) North Observatory, Clanfield, UK 
• (J95) Great Shefford, UK 
• (K63) G. Pascoli Observatory, Castelvecchio Pascoli, Italy. 
• (R57) Aorangi Iti Observatory, Lake Tekapo, New Zealand. 
• (W88) Slooh.com Chile Observatory, La Dehesa, Chile. 
• (X31) Galileo Galilei Observatory, Oro Verde, Argentina. 
• (Y00) SONEAR Observatory, Oliveira, Brazil. 
• (Z80) Northolt Branch Observatory, UK
• Perihelion Distance: 0..3877305354221541(AU)
• Aphelion Distance: 4.130577089564944(AU)
• Earth MOID (Earth center to NEO center): AU 0.00153454((0.597 LD)), (36.03 Earth radii) or 142,644.404 miles (229,563.916  (KM))

The Moon Live 2017-11-27

Tonight(2017-11-27)  was bad night my cell phone fell off the telescope then bounce of my second floor balcony...now it stop working.

The Moon Live 2017 11 26

The Moon Live 2017 11 24 Try 2