On 11 March 2021, 17 fragments (~0.5 to 8 mm in size, from site 1) of the Winchcombe meteorite were mounted using cleaned stainless-steel tweezers onto carbon-based electrically conductive, double-sided adhesive discs, also known as Leit tabs, stuck to the flat surface of two aluminum SEM pin stubs. The uncoated and unpolished fragments were then quickly transferred to an FEI Quanta 650 FE-SEM at the IAC of the NHM.
The FE-SEM is equipped with a Bruker
Quantax EDS system with a high-sensitivity, annular, four-channel Bruker FlatQUAD SDD inserted between the pole piece and sample within the main chamber of the SEM. The annular geometry allows sufficient data collection on uncoated, beam-sensitive, and nonconductive samples with substantial surface topography using ultralow beam currents under high vacuum (
65 ). An accelerating voltage of 6 and 9 kV and a beam current of 30 to 190 pA were used, resulting in an input count rate up to 55 kcps. Several of the fragments were initially mapped at 3- and 4-μm pixel resolution using automated stage control to identify features of interest, which were then further analyzed at a pixel resolution down to 16 nm. Follow-up SEM imaging of the features of interest was carried out in the variable pressure mode of the SEM using a low-vacuum cone.
King A.J., Daly L., Rowe J., Joy K.H., Greenwood R.C., Devillepoix H.A., Suttle M.D., Chan Q.H., Russell S.S., Bates H.C., Bryson J.F., Clay P.L., Vida D., Lee M.R., O’Brien Á., Hallis L.J., Stephen N.R., Tartèse R., Sansom E.K., Towner M.C., Cupak M., Shober P.M., Bland P.A., Findlay R., Franchi I.A., Verchovsky A.B., Abernethy F.A., Grady M.M., Floyd C.J., Van Ginneken M., Bridges J., Hicks L.J., Jones R.H., Mitchell J.T., Genge M.J., Jenkins L., Martin P.E., Sephton M.A., Watson J.S., Salge T., Shirley K.A., Curtis R.J., Warren T.J., Bowles N.E., Stuart F.M., Di Nicola L., Györe D., Boyce A.J., Shaw K.M., Elliott T., Steele R.C., Povinec P., Laubenstein M., Sanderson D., Cresswell A., Jull A.J., Sýkora I., Sridhar S., Harrison R.J., Willcocks F.M., Harrison C.S., Hallatt D., Wozniakiewicz P.J., Burchell M.J., Alesbrook L.S., Dignam A., Almeida N.V., Smith C.L., Clark B., Humphreys-Williams E.R., Schofield P.F., Cornwell L.T., Spathis V., Morgan G.H., Perkins M.J., Kacerek R., Campbell-Burns P., Colas F., Zanda B., Vernazza P., Bouley S., Jeanne S., Hankey M., Collins G.S., Young J.S., Shaw C., Horak J., Jones D., James N., Bosley S., Shuttleworth A., Dickinson P., McMullan I., Robson D., Smedley A.R., Stanley B., Bassom R., McIntyre M., Suttle A.A., Fleet R., Bastiaens L., Ihász M.B., McMullan S., Boazman S.J., Dickeson Z.I., Grindrod P.M., Pickersgill A.E., Weir C.J., Suttle F.M., Farrelly S., Spencer I., Naqvi S., Mayne B., Skilton D., Kirk D., Mounsey A., Mounsey S.E., Mounsey S., Godfrey P., Bond L., Bond V., Wilcock C., Wilcock H, & Wilcock R. (2022). The Winchcombe meteorite, a unique and pristine witness from the outer solar system. Science Advances, 8(46), eabq3925.