Observing Runs Looking for 2011 YS62 from 2015-08-26 to 2015-08-28
When
it comes to target selection there two criteria I use first is would additional
observations be useful, the second is the target in range of the telescope's
capability. To find targets I check one or all of the lists (see below) and see
if the target is range of the telescope's capability (if it is important I will
push the limit of the range) Then I will plan an observing run. Recently I checked the Arecibo Asteroid
Schedule and I saw they had requested optical astrometry for 2011 YS62. At the time this asteroid had a data-arc span
of 89 days and had been unobserved for 1314 days (3.597 years)
First Night
I first did run of 15 - 120 Second Luminance BIN2 Images on itelescope.net's (TEL T27), with no luck,. Next I used Find_Orb to generate new orbital elements with Epoch 2015 Sep 26.0 and did a another run 15. I also used Find_Orb's Monte Carlo function to generate a lot of clones(virtual asteroids) orbital elements and then manually add them to Astrometrica's MPCOrb.dat file. Then I created 3 stacks of 5 images and found a moving object near the known object box of one of the clones. I assigned a temporary designation to the object and submitted night one's observations to the Minor Planet Center.
Astrometrica object verification window a stack (1 of 3 First Night ) a stacks 5 - 120 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 window a stack (2 of 3 First Night ) a stacks 5 - 120 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 window a stack (1 of 3 First Night ) a stacks 5 - 120 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) |
Second Night
Using Find_Orb I generated two
orbits one was with just night one’s observations, the other with 2011 YS62 and
night one's observations (“updated orbit”) and manually replaced the
"clones" orbital elements. Next I ran a series of 6-120
Second Luminance BIN2 Images on itelescope.net's
(TEL T27) and created a stacks of 5 images and found an object at
the known object box for the "updated orbit". Then I ran a second run of 6 images and created
a stack of 5 and saw that the object was moving. Later on I ran another run of 15 images
and created a 3 more stacks of 5 images. I assigned a (new) temporary
designation to the object and submitted the second night’s observations to
the Minor Planet Center. Shortly thereafter the object was listed on the
NEO Confirmation Page.
Astrometrica object verification window a stack (1 of 5 Second Night ) a stacks 5 - 120 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 window a stack (2 of 5 Second Night ) a stacks 5- 120 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 window a stack (3 of 5 Second Night ) a stacks 5- 120 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 window a stack (4 of 5 Second Night ) a stacks 5- 120 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 window a stack (3 of 5 Second Night ) a stacks 5- 120 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) |
Third Night
I did the same orbit update has I did the night before then, I obtain 32--120 Second Luminance BIN2 images with itelescope.net's (TEL T27) and created 3 stacks of 10 image and submitted the third night observations to the Minor Planet Center using the designation that was on the NEO Confirmation Page.
Astrometrica object verification window a stack (1 of 3 First Night ) a stacks 10 - 120 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 window a stack (2 of 3 First Night ) a stacks 10 - 120 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 window a stack (3 of 3 First Night ) a stacks 10 - 120 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) |
Background
(as of 2015-09-30)
- Object: 2011 YS62
- Approximate Diameter: 310 m - 680 m (1017.06 feet to 2230.97 feet) ( Absolute Magnitude: H= 19.7 )
- Orbit Type: Amor
- First Observed was made on: 2011 12 29.15398
- First Observed By: Pan-STARRS 1 (MPC Code F51)
- Assignment of asterisk: Catalina Sky Survey (MPC Code 703) For infomation on how discoverer is defined read MPEC 2010-U20 : EDITORIAL NOTICE
- Last Observed: 2015 09 28.58389
- Data-Arc Span: 1405 days (3.85 yr)
- Number Oppositions :2
- Number of Observations Made: 85
- Next Close-Approach: Will safely pass Earth on 2015-Nov-2 at Nominal Distance of 0.0914513682160852 AU (35.59(LD)) or 8,500,935.758 miles or ( 13,680,929.957 KM)
- On the Goldstone Asteroid Schedule: NO
- On the Arecibo Asteroid Schedule: YES, Dates: 2015 Nov 29 (Request Optical Astrometry: No(It was request before recovery was made), Request Optical Lightcurve:NO, Request Optical Characterization NO)
- The NEO Confirmation Page
- The Possible Comet Confirmation Page
- JPL's Sentry Risk Table
- the NEODyS CLOMON2 risk page:
- Spaceguard Central Node's Priority List
- Near-Earth Object Human Space Flight Accessible Targets Study (NHATS)
- The Goldstone Asteroid Schedule
- The Arecibo Asteroid Schedule
- The Minor Planet Center(has some useful tools)
- Near Earth Objects Dynamic Site--2011 YS62
- (MPC) Observations 2011 YS62
- JPL Orbit Diagram 2011 YS62
- NEO Earth Close Approaches (JPL)
- The Tracking News
- NEO Coordination Centre
- MPC's Guide to Minor Body Astronomy
- MPC Editorial Notice 2011-E67
- List of removed objects
- Palermo Technical Impact Hazard Scale
- The Torino Impact Hazard Scale
- Impact Risk Assessment: An Introduction
- Practical guide on how to observe NEOCP object
- Understanding Risk Pages by Jon Giorgini