Near-Earth Asteroid Astrometry with Gaia David BANCELIN IMCCE, - - PowerPoint PPT Presentation

near earth asteroid astrometry with gaia
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Near-Earth Asteroid Astrometry with Gaia David BANCELIN IMCCE, - - PowerPoint PPT Presentation

Near-Earth Asteroid Astrometry with Gaia David BANCELIN IMCCE, Paris Observatory GREAT-SSO, Pisa, May 4-6 2011 Outline Gaia Mission Scientific goals Nominal Scanning Law Astrometry for known NEAs Impact on current and long


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Near-Earth Asteroid Astrometry with Gaia

David BANCELIN IMCCE, Paris Observatory

GREAT-SSO, Pisa, May 4-6 2011

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Outline

 Gaia Mission

 Scientific goals  Nominal Scanning Law

 Astrometry for known NEAs

 Impact on current and long term uncertainty  Collision probability

 Astrometry for unknown NEAs

 Alert Mode  Combination space/ground-based data

GREAT-SSO, Pisa, May 4-6 2011

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GAIA Mission

 Scientific goals

GREAT-SSO, Pisa, May 4-6 2011

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GAIA Mission

 Scientific goals

GREAT-SSO, Pisa, May 4-6 2011

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GAIA Mission

 Nominal Scanning Law

GREAT-SSO, Pisa, May 4-6 2011 Influence on date of observations Influence on the number of

  • bservations
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GAIA Mission

 Statistic of observations

GREAT-SSO, Pisa, May 4-6 2011

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Astrometry or known NEAs

Apophis case

Why Apophis?

 PHA (Potentially Hazardous Asteroid) discovered

in 2004

 MOID ≤ 0.05 A.U. and H ≤ 22.0  1213 PHAs known (~ 15% NEAs) and 148 with

diameter ≥ 1 km

 Deep close-approach with Earth in 2029 (~ 38 000

km)

 Choatic orbit  Impact trajectories

GREAT-SSO, Pisa, May 4-6 2011

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Astrometry for known PHAs

Apophis case

 Gaia observations of Apophis

 Inhomogenous size of

sets.

 Set with longuest arc

used for simulations.

GREAT-SSO, Pisa, May 4-6 2011

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Astrometry for known PHAs

Apophis case

 Impact on keplerian elements uncertainty

G.B. Only G.B.+ Gaia Gain σO σO

+ G

σO/σO

+ G

a (A.U.) 1.9E-08 6.8E-11 275 e 6.9E-08 3.9E-09 18 i (°) 1.8E-06 1.2E-07 15 Ω (°) 9.9E-05 2.2E-06 45 ω (°) 9.9E-05 2.3E-06 43 M (°) 7.4E-05 6.5E-07 114

 Ground-Based data : Optical

(1366) and Radar (5)

 Gaia data : 9 observations with

5 mas accuracy

GREAT-SSO, Pisa, May 4-6 2011

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Astrometry for known PHAs

Apophis case

 Impact on position uncertainty

GREAT-SSO, Pisa, May 4-6 2011

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Astrometry for known PHAs

Apophis case

 Impact on 2029 b-plane uncertainty

b-plane uncertainty Nominal Orbit Nominal orbit + Gaia data σξ (km) 10.5 0.3 σζ (km) 87 1.4

 3σ ellipse uncertainty in (ξ, ζ) in 2029

b-plane

 Primary (✳) and Secondary keyholes at

ascending (◾) and descending (◾) node. With Gaia data Without Gaia data GREAT-SSO, Pisa, May 4-6 2011

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Astrometry for newly discovered objects

 Number of alerts expected

Family Number Percentage (%) Amor 379 1.9 Apollo 1313 6.6 Atens 205 1 IEO 24 0.1 PHAs 583 2.9 Total 2614 12.5

GREAT-SSO, Pisa, May 4-6 2011

Statistic on a 20000 synthetic NEAs population

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Astrometry for newly discovered PHAs

 Recovery Strategy

GREAT-SSO, Pisa, May 4-6 2011

Hypothetical Geographos (PHA) detected

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Astrometry for newly discovered PHAs

 (α,δ) prediction

GREAT-SSO, Pisa, May 4-6 2011

12'x12' field of view centered in ML

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Astrometry for newly discovered PHA

 Combination space and ground-based data

One night observation

GREAT-SSO, Pisa, May 4-6 2011 x

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Astrometry for newly discovered PHA

 Combination space and ground-based data

GREAT-SSO, Pisa, May 4-6 2011

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Conclusion

 Good improvement of PHAs orbits (even with faint

number of observations)

 Useful data for Earth-impact threat study  Necessity of a useful strategy for recovery  Necessity of a Follow-up for G.B. observations

GREAT-SSO, Pisa, May 4-6 2011

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THANK YOU