hidden pixel

Flyby Anomaly Information

The flyby anomaly is an unexpected energy increase during Earth-flybys of spacecraft. This anomaly has been observed as shifts in the S-Band and X-Band Doppler and ranging telemetry. Taken together it causes a significant unaccounted velocity increase of over 13 mm/s during flybys.[1]

Contents

Observations

Gravitational assists are valuable techniques for solar system exploration. Because the success of these flyby maneuvers depends on the geometry of the trajectory, the position and velocity of a spacecraft is continually tracked during its encounter with a planet by the Deep Space Network (DSN).

Range residuals during the Earth-flyby of NEAR

The flyby anomaly was first noticed during a careful inspection of DSN Doppler data shortly after the Earth-flyby of the Galileo spacecraft on 8 December 1990. While the Doppler residuals (observed minus computed data) were expected to remain flat, the analysis revealed an unexpected 66 mHz shift, which corresponds to a velocity increase of 3.92 mm/s at perigee. An investigation of this effect at the Jet Propulsion Laboratory (JPL), the Goddard Space Flight Center (GSFC) and the University of Texas has not yielded a satisfactory explanation. No anomaly was detected after the second Earth-flyby of the Galileo spacecraft in December 1992, because any possible velocity increase was masked by atmospheric drag of the lower altitude of 303 km.

On 23 January 1998 the Near Earth Asteroid Rendezvous (NEAR) spacecraft experienced an anomalous velocity increase of 13.46 mm/s after its Earth encounter. Cassini–Huygens gained ~0.11 mm/s in August 1999 and Rosetta 1.82 mm/s after its Earth-flyby in March 2005.

An analysis of the MESSENGER spacecraft (studying Mercury) did not reveal any significant unexpected velocity increase. This may be that MESSENGER both approached and departed earth symmetrically about the equator (see data and proposed equation below). This may suggest that the anomaly is related to Earth's rotation.

Summary of Earth-flyby spacecraft is provided in table below.[2] The Rosetta data is for its first flyby in 2005; the second flyby produced no significant anomalous increase, and the third a negligible decrease.[3]

Quantity Galileo I Galileo II NEAR Cassini Rosetta-I Messenger Rosetta-II Rosetta-III
Date 12/8/1990 12/12/1992 01/23/1998 08/18/1999 03/04/2005 08/02/2005 11/13/2007 11/13/2009
Speed at infinity, km/s 8.949 8.877 6.851 16.01 3.863 4.056
Speed at perigee, km/s 13.738 --- 12.739 19.03 10.517 10.389 12.49 13.34
Impact parameter, km 11261 12850 8973 22680.49 22319
Minimal altitude, km 956 303 532 1172 1954 2336 5322 2483
Spacecraft mass, kg 2497.1 730.40 4612.1 2895.2 1085.6 2895 2895
Trajectory inclination to equator, degrees 142.9 138.9 108.8 25.4 144.9 133.1
Deflection angle, degrees 47.46 51.1 66.92 19.66 99.396 94.7
Speed increment at infinity, mm/s 3.92±0.08 -4.60± 1.00 13.46±0.13 −2±1 1.82±0.05 0.02±0.01
Speed increment at perigee, mm/s 2.56±0.05 7.21±0.07 −1.7±0.9 0.67±0.02 0.008±0.004 ~0 −0.004±0.044
Gained energy, J/kg 35.1±0.7 92.2±0.9 7.03±0.19

Upcoming missions with Earth flybys include Juno and BepiColombo.

Proposed equation

An empirical equation for the anomalous flyby velocity change was proposed by J.D. Anderson et al.:

where ωe is the angular frequency of the Earth, Re is the Earth radius, and φi and φo are the inbound and outbound equatorial angles of the spacecraft.[4]

In November 2009, ESA's Rosetta spacecraft was tracked closely during flyby in order to precisely measure its velocity, in an effort to gather further data about the anomaly, but no significant anomaly was found.[3]

Possible explanations

It is not known whether the flyby anomaly is related to the Pioneer anomaly. In the case of spacecraft that transit over Earth's rotational or magnetic polar regions, the flyby anomaly is an acceleration rather than a deceleration. It is possible that during an equatorial transit an unmeasured small (relative to Earth) deceleration occurs; this is very similar to the Pioneer spacecraft's deceleration relative to the Sun.

Possible explanations of the flyby anomaly include:

References

  1. ^ "ESA's Rosetta spacecraft may help unravel cosmic mystery". European Space Agency. November 12, 2009. http://www.spaceref.com/news/viewpr.html?pid=29609. Retrieved 13 March 2010.
  2. ^ Anderson, John D.; James K. Campbell, Michael Martin Nieto (July 2007), "The energy transfer process in planetary flybys", New Astronomy 12 (5): 383–397, arXiv:astro-ph/0608087, Bibcode 2007NewA...12..383A, doi:10.1016/j.newast.2006.11.004
  3. ^ a b "Mystery remains: Rosetta fails to observe swingby anomaly". ESA. http://webservices.esa.int/blog/post/5/916.
  4. ^ Anderson, et. al. (7 March 2008), "Anomalous Orbital-Energy Changes Observed during Spacecraft Flybys of Earth", Phys. Rev. Lett., http://virgo.lal.in2p3.fr/NPAC/relativite_fichiers/anderson_2.pdf.
  5. ^ J. P. Mbelek (2008). "Special relativity may account for the spacecraft flyby anomalies". arXiv:0809.1888 [gr-qc]. Bibcode 2008arXiv0809.1888M
  6. ^ S.L.Adler (2008), "Can the flyby anomaly be attributed to Earth-bound dark matter?", Physical Review D 79 (2), arXiv:0805.2895, Bibcode 2009PhRvD..79b3505A, doi:10.1103/PhysRevD.79.023505
  7. ^ M.E. McCulloch (2008), "Modelling the flyby anomalies using a modification of inertia", MNRAS Letters 389 (1): L57–L60, arXiv:0806.4159, Bibcode 2008MNRAS.389L..57M, doi:10.1111/j.1745-3933.2008.00523.x
  8. ^ L. Iorio (2009), "The Effect of General Relativity on Hyperbolic Orbits and Its Application to the Flyby Anomaly", Scholarly Research Exchange 2009: 1, Bibcode 2009ScReE2009.7695I, doi:10.3814/2009/807695, 807695
  9. ^ Marcelo Samuel Berman; Fernando de Mello Gomide (2010). "General Relativistic Treatment of the Pioneers Anomaly". arXiv:1011.4627 [physics.gen-ph].

External links

Categories: Unsolved problems in physics | Gravitation

 

The above information uses material from Wikipedia and is licensed under the GNU Free Documentation License.
Some facts may not have been fully verified for accuracy. [Disclaimers]
This page was last archived by our server on Sat Sep 24 10:09:59 2011.
Displaying this page or its contents does not use any Wikimedia Foundation's resources.
The owners of this site proudly support the Wikimedia Foundation.


MESSENGER at Mercury Image Credit NASA Johns Hopkins University
universetoday.com
MESSENGER at Mercury Image Credit NASA Johns Hopkins University
300px x 377px | 95.80kB

[source page]

Scientists from the messenger mission continue to analyze the data from the spacecraft s first flyby of Mercury on January 14 2008 Initial data about the

Google Images Search: flyby anomaly,
Sat Sep 24 10:10:00 2011
Entire staff of brokers' accreditation unit fired - Business Mirror
businessmirror.com.ph
Entire staff of brokers' accreditation unit fired - Business Mirror
Sun, 15 Aug 2010 13:41:15 GMT+00:00
Business Mirror Alvarez said in a statement that CAS was abolished as a result of several anomalies in its operation, one of which was allowing fly-by -night entities to be ...
Google News Search: flyby anomaly,
Sat Sep 24 10:10:03 2011