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Showing posts with label MPC Code Q62. Show all posts
Showing posts with label MPC Code Q62. Show all posts

Jun 9, 2018

Confirmation Images of the COMET C/2018 L2 (ATLAS) on 2018-06-07

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A confirmation image of the COMET C/2018 L2 (ATLAS)
on 2018-06-07 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 second luminance BIN2 images taken
with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley


A confirmation image of the COMET C/2018 L2 (ATLAS)
on 2018-06-07 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 second luminance BIN2 images taken
with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley


A confirmation image of the COMET C/2018 L2 (ATLAS)
on 2018-06-07 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 second luminance BIN2 images taken
with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley

A confirmation image of the COMET C/2018 L2 (ATLAS)
on 2018-06-07 from Siding Spring Observatory,
Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 second luminance BIN2 images taken
with iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley



Jun 1, 2018

Confirmation Images of the COMET C/2018 K1 (Weiland)

On 2018 05 25 Henry Weiland an observer with ATLAS-MLO(Asteroid Terrestrial-impact Last Alert System ---Mauna Loa) reported a possible comet to the Minor Planet Center in Cambridge, Massachusetts, USA.  This possible comet was reported using the observer-assigned temporary designation "A1072Wf".  It was posted to the Possible Comet Confirmation Page(PCCP) and came to the attention of observer around the world. On 2018-05-26 I woke up, check iTelescope.net and saw that their facility in Siding Spring Observatory, AU was open. So had T30 started an imaging run of  60 - 60-second luminance BIN2 images and went out to eat breakfast. I got back made four stacks of 5 so can work around "stars that were in the way." I submitted my observations, as more observations came in and as the morning change to the afternoon, I saw my observations had poor residuals, so I did imaging run of  60 - 60-second luminance BIN2 images on T27.

A confirmation image of COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 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 COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 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 COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 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 COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 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 COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 second luminance BIN2 images taken with iTelescope.net's
(T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley
A confirmation image of COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 second luminance BIN2 images taken with iTelescope.net's
(T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley
A confirmation image of COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 second luminance BIN2 images taken with iTelescope.net's
(T27 TEL 0.70-m f/6.6 reflector + CCD)
By Steven M. Tilley
A confirmation image of COMET C/2018 K1 (Weiland)
[was the PCCP(Possible Comet Confirmation Page)object A1072Wf] on 2018-05-26
from Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 5 - 60 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 2018-05-31)

  • Object: COMET C/2018 K1 (Weiland) 
  • Orbit Type: Halley-type Comet
  • First(Precovery) observation was made on: 2017 11 06.24388
  • First(Precovery) observation was made by:  Pan-STARRS 1, Haleakala (MPC Code F51)
  • Discovery observation was made on: 2018 05 25.54194
  • Discovery observation was made by : ATLAS-MLO, Mauna Loa  (MPC Code T08)
  • The Discovery M.P.E.C.: MPEC 2018-K117: COMET C/2018 K1 (Weiland)
  • Last Observation (publish): 2018 05 30.34974  (from Steward Observatory, Kitt Peak - Spacewatch  (MPC Code 691) ) 
  • Data-Arc Span (publish):  205 days 
  • Number of Optical Observations(published):  91
  • Observatories reporting (published) observations(MPC Code): 
    • (349) Ageo, Japan. 
    • (372) Geisei, Japan. 
    • (691) Steward Observatory, Kitt Peak - Spacewatch, US/Arizona. 
    • (E23) Arcadia, Australia/NSW. 
    • (F51) Pan-STARRS 1, Haleakala, US/Hawaii 
    • (H06) iTelescope Observatory, Mayhill, US/New Mexico 
    • (H47) Vicksburg, US/Mississippi. 
    • (I47) Pierre Auger Observatory, Malarg├╝e, Argentina. 
    • (I52) Steward Observatory, Mt. Lemmon Station US/Arizona. 
    • (Q62) iTelescope Observatory, Siding Spring, Australia/NSW.
    • (T08) ATLAS-MLO, Mauna Loa, US/Hawaii.
    • (W88) Slooh.com Chile Observatory, La Dehesa, Chile. 
    • (W96) CAO, San Pedro de Atacama (since 2013), Chile. 
    • (Y00) SONEAR Observatory, Oliveira, Brazil. 
  • Perihelion Distance 1.879151252869776 (AU) 
  • Aphelion Distance:  57.90074646767503 (AU) 
  • Earth MOID (Earth center to NEO center): 0.886103 AU (( 344.846 LD)), (20,806.64 Earth radii) or miles 82,368,419.687 ( 132,559,122.013 ( KM))[If the Earth was the size of a basketball this would be 8,210.36 Feet( 2,502.52 Meters)]

May 29, 2018

Re-Observing 2015 FP118 Another Look Almost Three Years later

When I am looking objects to observer, I try to find something within the capabilities of the telescope, interesting, and 'needing" observation. To these ends I check following lists:
On 2018-05-28 I saw  that 2015 FP118 was on both the Arecibo and Goldstone lists, needing astrometry,  and it was within the capabilities of iTelescope.net's (T27 TEL 0.70-m f/6.6 reflector + CCD) so I went for it. As I was create a directory so I could downloading the .FITS(Flexible Image Transport System) files I found out that I observed 2015 FP118  for  19.6 min on  2015-06-06.

The NEO 2015 FP118 on 2018-05-28 from
Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
a stack of 45 - 60 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 2015 FP118 on 2015-06-06 from
 Siding Spring Observatory, Coonabarabran, NSW, Australia. (MPC Q62)
 a stack of 22 - 60 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 2018-05-29)
  • Object: 2015 FP118
  • Orbit Type: Apollo [NEO, PHA]
  • Approximate Diameter: 370 m - 820 m(1213.911 feet to 2690.289 feet) (Absolute Magnitude: H= 19.3)
  • On the Sentry Risk Table: NO( Removed 2015-04-02 15:53:35)
  • On the NEODyS CLOMON2 risk page: NO 
  • Discovery observation was made on: 2015 03 21.57498
  • Discovery observation was made by Pan-STARRS 1, Haleakala (MPC Code F51) The Discovery M.P.E.C.:MPEC 2015-F132: 2015 FP118
  • Last Observation (publish): 2018 05 28.56107 (at iTelescope Observatory, Siding Spring, Australia (MPC Code Q62) )
  • Data-Arc Span (publish): 1164 days (3.19 yr) 
  • Number of Optical Observations(published):133
  • Observatories Reporting (Published) Observations(MPC Code):
    • (204) Schiaparelli Observatory,Italy. 
    • (290) Mt. Graham-VATT,US/Arizona.
    • (291) LPL/Spacewatch II,US/Arizona. 
    • (568) Mauna Kea, US/Hawaii.
    • (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.
    • (926) Tenagra II, US/Arizona.
    • (D29) Purple Mountain Observatory, XuYi Station 
    • (F51) Pan-STARRS 1, Haleakala US/Hawaii. 
    • (G96) Mt. Lemmon Survey, US/Arizona.
    • (Q62) iTelescope Observatory, Siding Spring
  • Perihelion Distance 0.9541884017671265 (AU)
  • Aphelion Distance: 3.28765938878308 (AU)
  • Earth MOID (Earth center to NEO center): 0.029858 AU ((11.62 LD)), ( 701.09 Earth radii) or 2,775,474.494 miles ( 4,466,693.22 ( KM))[If the Earth was the size of a Basketball this would be 276.261 Feet(84.204 Meters)]
  • Next Close-Approach to Earth: Will safely pass Earth on 2018-Sep-03:
    • Minimum Distance(Earth center to NEO center) of 0.0314378825351047 (AU) (12.235  (LD)),  (738.195 Earth radii) or  2,922,333.75 miles ( 4,703,040.286 (KM)) 
    • Nominal Distance(Earth center to NEO center) of   0.031438612821003 (AU) (12.235 (LD)), (738.212 Earth radii) or  2,922,401.634  miles (4,703,149.536 (KM))
    • Maximum Distance(Earth center to NEO center) of  0.0314393431490244 (AU) (12.235 (LD)), (738.229 Earth radii) or  2,922,469.522 miles (4,703,258.791 (KM))
  • Goldstone Asteroid Schedule: Yes 2018 Sep (Needs Astrometry: Yes Needs Physical Observations: Yes)
  • On the Arecibo Asteroid Schedule:  YES,  Dates 2018 Aug (Request Optical Astrometry: YES , Request Optical  Lightcurve:YES, Request Optical Characterization YES) 

Apr 23, 2018

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

Apr 6, 2018

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))   

Mar 19, 2018

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))   

Jun 19, 2017

Confirmation Images of The NEO 2017 MC

A confirmation images of the NEO 2017 MC on 2017-06-18
from Mayhill, New Mexico (New Mexico Skies) (MPC Code H06),
a stack of 5-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T11 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Mayhill, New Mexico (New Mexico Skies) (MPC Code H06),
a stack of 5-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T11 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Mayhill, New Mexico (New Mexico Skies) (MPC Code H06),
a stack of 5-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T11 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Mayhill, New Mexico (New Mexico Skies) (MPC Code H06),
a stack of 5-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T11 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Mayhill, New Mexico (New Mexico Skies) (MPC Code H06),
a stack of 50-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T11 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Siding Spring Observatory, Coonabarabran, NSW, Australia (MPC Code Q62),
a stack of 20-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T31 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Siding Spring Observatory, Coonabarabran, NSW, Australia (MPC Code Q62),
a stack of 20-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T31 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Siding Spring Observatory, Coonabarabran, NSW, Australia (MPC Code Q62),
a stack of 20-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T31 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley
A confirmation images of the NEO 2017 MC on 2017-06-18
from Siding Spring Observatory, Coonabarabran, NSW, Australia (MPC Code Q62),
a stack of 60-30 Second Luminance BIN2 Images taken with itelescope.net's
(TEL T31 0.50-m f/6.8 reflector + CCD + f/4.5 focal reducer)
(c) Steven M. Tilley

Background

(as of 2017-06-18)
  • Object: 2017 MC
  • Approximate Diameter:  150 m - 380 m ( 492.126 feet to feet 1246.72)(Absolute Magnitude: H= 21.021)
  • Orbit Type: Apollo [NEO] Potentially Hazardous Asteroid
  • On the Sentry Risk Table: NO
  • On the NEODyS CLOMON2 risk page: NO
  • Discovery (First) observation was made: 2017 06 16.53663
  • Discovery (First )observation was made by:  ATLAS-MLO(Asteroid Terrestrial-impact Last Alert System)(MPC Code  T08) The Discovery M.P.E.C.: MPEC 2017-M15 : 2017 MC
  • Last Observation(publish) was made: 2017 06 18.64005 (by iTelescope Observatory, Siding Spring   (MPC Code Q62 )
  • Data-Arc Span(publish) :  2 days
  • Number of Optical Observations(published) : 76 
  • Observatories Reporting (Published) Observations(MPC Code):
    • (104) San Marcello Pistoiese, Italy.
    • (160) Castelmartini, Italy.
    • (204) Schiaparelli Observatory, Italy.
    • (595) Farra d'Isonzo, Italy.
    • (926) Tenagra II Observatory, Nogales, US/Arizona.
    • (B49) Paus Observatory, Sabadell, Spain.
    • (B74) Santa Maria de Montmagastrell, Spain.
    • (C23) Olmen,Belgium.
    • (H06) iTelescope Observatory, Mayhill, US/New Mexico.
    • (I93) St Pardon de Conques (N44.558708 W0.203000) France.
    • (J69) North Observatory, Clanfield (N50.939011 W1.019700) UK.
    • (J95) Great Shefford,UK.
    • (K38) M57 Observatory, Saltrio, Italy.
    • (K63) G. Pascoli Observatory, Castelvecchio Pascoli, Italy.
    • (K88) GINOP-KHK, Piszkesteto, Hungary.
    • (Q62) iTelescope Observatory, Siding Spring, Australia/NSW.
    • (T08) ATLAS-MLO, Mauna Loa,US/Hawaii.
    • (W25) RMS Observatory, Cincinnati,US/Ohio.
    • (W34) Squirrel Valley Observatory, Columbus, US/North Carolina.
    • (Y00) SONEAR Observatory, Oliveira, Brazil.