- Object: COMET C/2018 L2 (ATLAS)
- Orbit Type:Parabolic Comet
- Discovery observation was made by:ATLAS-MLO, Mauna Loa (MPC Code T08)
- The Discovery M.P.E.C.: MPEC 2018-L37 : COMET C/2018 L2 (ATLAS)
- JPL Orbit Diagram
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Showing posts with label NEOCP Confirmation Page. Show all posts
Showing posts with label NEOCP Confirmation Page. Show all posts
Jun 9, 2018
Confirmation Images of the COMET C/2018 L2 (ATLAS) on 2018-06-07
...
Jun 3, 2018
A Rock Designated ZLAF9B2(now 2018 LA) Social Media and Fireball Reports
On 2018-06-02 Richard A. Kowalski, with the Catalina Sky Survey reported observations of a "new" object, given the observ3er-assigned temporary designation "ZLAF9B2", to Minor Planet Center in Cambridge, Massachusetts, USA. It was posted to the NEOCP(NEO Confirmation Page) making the observations available to asteroid and comet researcher around the world. The data was analyzed and posted JPL's Scout: NEOCP Hazard Assessment, independently analyzed and posted to Bill Gray's Current NEOCP summary page. Then emails to mailing list post to social madia started going out. It was know to be small at the start.
When wroke up on 2018-06-02 I check iTelescope.net and saw their facility in Siding Spring Observatory, AU was clouded out than I went out to eat breakfast. When got back just to see what I would observe if I could observe, I check the NEOCP and saw that ZLAF9B2 was "bright", and then check "The Minor Planet Mailing List {MPML}" Some of the asteroid and comet researchers where talking. The Bill Gray sent and a number of carefully worded emails to email list stating ZLAF9B2 should be a "Priority Target".
When wroke up on 2018-06-02 I check iTelescope.net and saw their facility in Siding Spring Observatory, AU was clouded out than I went out to eat breakfast. When got back just to see what I would observe if I could observe, I check the NEOCP and saw that ZLAF9B2 was "bright", and then check "The Minor Planet Mailing List {MPML}" Some of the asteroid and comet researchers where talking. The Bill Gray sent and a number of carefully worded emails to email list stating ZLAF9B2 should be a "Priority Target".
One of the programs available to asteroid and comet researchers is Find_Orb
it is useful for calculating approximate ephemeris, determining approximate
orbits, residuals, generating virtual asteroids, virtual impactors, predicting impact locations, and many other things. It should be noted IF one uses wrong setting one get a totally wrong solution. One things Find_Orb can be use for is generating a "asteroid risk corridor" with the help of Guide 9.1. This should be done with care because of uncertainties in observations how one sets the over-observing parameters as well with other setting can the effect the results. Bill Gray posted post a risk corridor for ZLAF9B2 and I thought I would give it a try. I had Find_Orb generated virtual asteroids and virtual impactors using a monte carlo process.
Here is my TEST with Find_Orb using a monte carlo process see the files here |
Here is my TEST with Find_Orb using a monte carlo process see the files here |
Test with the newly added ATLAS observations with Find_Orb using a monte carlo process see the files here |
"that the objectreached 50-km height above the Earth's surface around 16:51 UTC over southern Africa."
Timeline of SOME of the Post to Social Media
{MPML} ZLAF9B2 = priority target (from Bill Gray):— Asteroid Initiatives (@AsteroidEnergy) June 2, 2018
Based on eleven observations from Catalina, this is
looking to be coming quite close, probably about 50000
km or so. It's mag 17.2 and getting brighter, too, so it shouldn't be
too tough to get.
A tiny (3-metre?) asteroid, ZLAF9B2, making a close approach to Earth within twice GEO distance, perhaps much closer. Some solutions by Bill Gray suggest possible impact over Indonesia around now - look out for fireball reports! Not big enough to be a worry.— Jonathan McDowell (@planet4589) June 2, 2018
It looks like there is a good probability the newly discovered small object ZLAF9B2 will impact the Earth's atmosphere within the next few hours. (Plot from MPML and Peter Birtwhistle) https://t.co/As7RgDseLA— Asteroid Initiatives (@AsteroidEnergy) June 2, 2018
It looks like there is a good probability ZLAF9B2 will impact the Earth within the next few hours. (Plot from MPML and Peter Birtwhistle) https://t.co/As7RgDseLA pic.twitter.com/XKktXbLNFn— Asteroid Initiatives (@AsteroidEnergy) June 2, 2018
ZLAF9B2 is very close.— Neil Norman FRAS. (@telescopecomet1) June 2, 2018
and then there's ZLAF9B2 https://t.co/YXiBEdQqqC— Asteroid Initiatives (@AsteroidEnergy) June 2, 2018
Update of the possible times of impact (UTC) for ZLAF9B2 from Bill Gray. pic.twitter.com/TEp9oF4Dcw— Asteroid Initiatives (@AsteroidEnergy) June 2, 2018
Analysis on the Minor Planet Mailing List suggests that the ZLAF9B2 object reentered and burnt up over Botswana at 1644UTC— Jonathan McDowell (@planet4589) June 2, 2018
Newly-disovered asteroid #ZLAF9B2 likely hit the Earth a few hours ago.https://t.co/fwx3eAVMX7 pic.twitter.com/C3rBgE07js— Tony Dunn (@tony873004) June 3, 2018
Strong infrasound detection of a bolide at station I47 in South Africa today at 1730 UT. Origin time between 1645-17 UT over Botswana. Yield 0.3-0.5 kT, corresponding to 2m diameter asteroid. #fireball #neoimpacts pic.twitter.com/fVe5GtwTtb— Peter Brown (@pgbrown) June 3, 2018
Yes, this was ZLAF9B2. I obviously left Germany too early— Peter Brown (@pgbrown) June 3, 2018
My Test with with Find_Orb and Guide 9--14 observations; 2018 June 2 (3.8 hr) (including newly added ATLAS observations) Monte Carlo noise set to 2 and Physical set to Standard #ZLAF9B2 pic.twitter.com/QqBBzXsOB2— Steven M. Tilley (@StevearenoBR) June 3, 2018
Just for fun, here’s my estimated fireball track from the Deelpan video alongside the @StevearenoBR candidate line. 800km is a surprise (I guessed 400km) but it’s calculated correctly if 50km altitude burst & it’s a v bright fireball. Atmospheric speed from @tony873004. #ZLAF9B2 pic.twitter.com/b9DWcezuST— Andy Cooper (@scute1133) June 3, 2018
{MPML} The object ZLAF9B2 is (given that it exploded in the air over Botswana yesterday) "posthumously" going to be named 2018 LA. https://t.co/JxTT8jwSGX— Asteroid Initiatives (@AsteroidEnergy) June 3, 2018
Apr 26, 2018
Confirmation Images of the NEO 2018 HH2
See: MPEC 2018-H89 : 2018 HH2
Apr 23, 2018
Confirmation images of the NEO 2018 HC1
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.
Jan 17, 2017
A NEO Re-Confirmation for the Asteroid 2016 VM4
Jan 9, 2017
Confirmation images of the NEO 2017 AF5
Background
(as of 2017-01-09 )
- Object: 2017 AF5
- Orbit Type: Apollo [NEO]
- Discovery (First) observation was made: 2017 01 04.59742
- Discovery (First )observation by: ATLAS-HKO, Haleakala(MPC Code T05) The Discovery M.P.E.C.: MPEC 2017-A53 : 2017 AF5
- Last Observation(publish): 2017 01 08.59190 (by ATLAS-HKO, Haleakala (MPC Code T05))
- Data-Arc Span(publish) : 4 days
- Number of Optical Observations(published): 79
- Observatories Reporting (Published) Observations(MPC Code):
- (104) San Marcello Pistoiese, Italy.
- (107) Cavezzo, Italy.
- (160) Castelmartini, Italy.
- (204) Schiaparelli Observatory, Italy.
- (300) Bisei Spaceguard Center-BATTeRS, Japan.
- (587) Sormano, Italy.
- (595) Farra d'Isonzo, Italy.
- (703) Catalina Sky Survey, US/Arizona.
- (926) Tenagra II Observatory, Nogales, US/Arizona.
- (C44) A. Volta Observatory, Lanzo d'Intelvi, Italy.
- (H36) Sandlot Observatory, Scranton, US/Kansas.
- (I52) Steward Observatory, Mt. Lemmon Station, US/Arizona.
- (I89) iTelescope Observatory, Nerpio, Spain.
- (I93) St Pardon de Conques, France.
- (J95) Great Shefford, UK.
- (K63) G. Pascoli Observatory, Castelvecchio Pascoli, Italy.
- (T05) ATLAS-HKO, Haleakala, US/Hawaii.
- Perihelion Distance: 0.1296403396428067 (AU)
- Aphelion Distance: 4.659873602813798 (AU)
- Earth MOID: 0.154461 AU ( 60.112 (LD)) or 14,358,046.946 miles (23,107,036.705 (KM))
- Last Close-Approach to Earth: Passed the Earth on 2017-Jan-03 at a Nominal Distance of 0.440916363577703 (AU), (171.592 Lunar Distance (LD)), or 40,985,736.514 miles ( 65,960,149.144 (KM))
Useful Links:
- NEO Earth Close Approaches (JPL) (up coming)
- JPL's NEO Earth Close-Approaches (Between 1900 A.D. and 2200 A.D- limited to encounters with reasonably low uncertainty)
- The Tracking News
- NEO Coordination Centre
- Speed of Light - Space - Distance Calculator
- Asteroid Hazards: The View from Space(MPC)
- Don’t fear apocalyptic asteroids: you’re safer than you think
- Understanding Risk Pages By Jon Giorgini
- Revised asteroid scale aids understanding of impact risk
- Near Earth Objects Scale Helps Risk Communication
- Dealing With the Impact Hazard: An International Project
- The Palermo Technical Impact Hazard Scale
- An Asteroid as Entered the Blogosphere… Should I Be Worried? A commentary by Steven M. Tilley
- International Asteroid Warning Network
- Impact Risk Assessment: An Introduction - Near-Earth Object Program
- Hazardous NEO Technical Reviews
- Frequently Asked Questions For Impact Risk Assessment
- How to Find an Impact Orbit for the Earth-Asteroid Collision
- The Asteroid/Comet Impact Hazard
- Whom should we call? Data policy for immediate impactors announcements
- NEO Search & Follow-Up
- NEOs' Science pages by Livia Giacomini
- Torino Scale(JPL)
- Find_Orb --- Orbit determination software - Project Pluto
- Guide to Minor Body Astrometry(MPC)
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