The radiator shield on the Wide Field and Planetary Camera 2 (WFPC2) was subject to optical inspection following return from the Hubble Space Telescope (HST) in 2009. The survey revealed over 600 impact features of > 300 micrometers diameter, from exposure in space for 16 years. Subsequently, an international collaborative programme of analysis was organized to determine the origin of hypervelocity particles responsible for the damage. Here we describe examples of the numerous smaller micrometeoroid (MM) impact features (< 700 micrometers diameter) which excavated zinc orthotitanate (ZOT) paint from the radiator surface, but did not incorporate material from underlying Al alloy; larger impacts are described by [3]. We discuss recognition an...
Dust-sized olivine particles were fired at a copper plate using the Space Power Institute hyperveloc...
The Chemistry of Micrometeoroids Experiment (LDEF instrument A0187-1) exposed witness plates of high...
Two experiments within the French Cooperative Payload (FRECOPA) and devoted to the detection of cosm...
The Wide Field and Planetary Camera 2 (WFPC2) was returned from the Hubble Space Telescope (HST) by ...
Postflight surveys of the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope ha...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Recognition of origin for particles responsible for impact damage on spacecraft such as the Hubble S...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Prior to their retrieval from low Earth orbit (LEO), the individual solar cells that make up the 'V2...
This paper discusses the results of an attempt to use laboratory test data and empirically derived m...
Prior to the retrieval in 1993 from low Earth orbit (LEO), the "—V2" Solar Array wing of the Hubble ...
Objectives: I.) Conduct micrometeoroid and orbital debris (MMOD) impact inspection of the Hubble Spa...
The Ion Beam textured and coated surfaces EXperiment (IBEX), designated S1003, was flown on LDEF at ...
Dust-sized olivine particles were fired at a copper plate using the Space Power Institute hyperveloc...
The Chemistry of Micrometeoroids Experiment (LDEF instrument A0187-1) exposed witness plates of high...
Two experiments within the French Cooperative Payload (FRECOPA) and devoted to the detection of cosm...
The Wide Field and Planetary Camera 2 (WFPC2) was returned from the Hubble Space Telescope (HST) by ...
Postflight surveys of the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope ha...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Recognition of origin for particles responsible for impact damage on spacecraft such as the Hubble S...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Return of materials from the Hubble Space Telescope (HST) during shuttle orbiter service missions ha...
Prior to their retrieval from low Earth orbit (LEO), the individual solar cells that make up the 'V2...
This paper discusses the results of an attempt to use laboratory test data and empirically derived m...
Prior to the retrieval in 1993 from low Earth orbit (LEO), the "—V2" Solar Array wing of the Hubble ...
Objectives: I.) Conduct micrometeoroid and orbital debris (MMOD) impact inspection of the Hubble Spa...
The Ion Beam textured and coated surfaces EXperiment (IBEX), designated S1003, was flown on LDEF at ...
Dust-sized olivine particles were fired at a copper plate using the Space Power Institute hyperveloc...
The Chemistry of Micrometeoroids Experiment (LDEF instrument A0187-1) exposed witness plates of high...
Two experiments within the French Cooperative Payload (FRECOPA) and devoted to the detection of cosm...