Haematological findings in healthy and sick captive rosy flamingos (Phoenicopterus ruber ruber).

Full blood counts and fibrinogen estimations were carried out on 36 clinically normal adult Rosy flamingos (21 males, 15 females) and six juveniles (sex uncertain). No significant sex differences were found but the haemoglobin levels, red cell counts, packed cell volumes and mean cell haemoglobin concentrations were lower and the white cell counts higher in juveniles than in adults. Reference values obtained from the normal birds were used as a basis for assessing the results of blood counts on nine birds showing a variety of abnormal clinical conditions. Heterophilia occurred in individuals with infections, chronic renal lesions, haemorrhage and suspected thrombosis. In one case, morphologically abnormal heterophils were present. A bird with carcinoma and peritonitis showed heteropenia. Several birds had hypochromic, microcytic red cells and severe hypochromic microcytic anaemia was found in a bird with an organising abdominal haematoma associated with chronic renal pathology. Several of the cases also had thrombocytosis and raised fibrinogen levels.

The environs of viking 2 lander.

Forty-six days after Viking 1 landed, Viking 2 landed in Utopia Planitia, about 6500 kilometers away from the landing site of Viking 1. Images show that in the immediate vicinity of the Viking 2 landing site the surface is covered with rocks, some of which are partially buried, and fine-grained materials. The surface sampler, the lander cameras, engineering sensors, and some data from the other lander experiments were used to investigate the properties of the surface. Lander 2 has a more homogeneous surface, more coarse-grained material, an extensive crust, small rocks or clods which seem to be difficult to collect, and more extensive erosion by the retro-engine exhaust gases than lander 1. A report on the physical properties of the martian surface based on data obtained through sol 58 on Viking 2 and a brief description of activities on Viking 1 after sol 36 are given.

The "soil" of Mars (viking 1).

The location of the Viking 1 lander is most ideal for the study of soil properties because it has one footpad in soft material and one on hard material. As each soil sample was acquired, information on soil properties was obtained. Although analysis is still under way, early results on bulk density, particle size, angle of internal friction, cohesion, adhesion, and penetration resistance of the soil of Mars are presented.

Physical properties of the martian surface from the viking 1 lander: preliminary results.

The purpose of the physical properties experiment is to determine the characteristics of the martian "soil" based on the use of the Viking lander imaging system, the surface sampler, and engineering sensors. Viking 1 lander made physical contact with the surface of Mars at 11:53:07.1 hours on 20 July 1976 G.M.T. Twenty-five seconds later a high-resolution image sequence of the area around a footpad was started which contained the first information about surface conditions on Mars. The next image is a survey of the martian landscape in front of the lander, including a view of the top support of two of the landing legs. Each leg has a stroke gauge which extends from the top of the leg support an amount equal to the crushing experienced by the shock absorbers during touchdown. Subsequent images provided views of all three stroke gauges which, together with the knowledge of the impact velocity, allow determination of "soil" properties. In the images there is evidence of surface erosion from the engines. Several laboratory tests were carried out prior to the mission with a descent engine to determine what surface alterations might occur during a Mars landing. On sol 2 the shroud, which protected the surface sampler collector head from biological contamination, was ejected onto the surface. Later a cylindrical pin which dropped from the boom housing of the surface sampler during the modified unlatching sequence produced a crater (the second Mars penetrometer experiment). These two experiments provided further insight into the physical properties of the martian surface.

Surveyor v: lunar surface mechanical properties.

The mechanical properties of the lunar soil at the Surveyor V landing site seem to be generally consistent with values determined for soils at the landing sites of Surveyor I and III. These three maria sites are hundreds of kilometers apart. However, the static bearing capability may be somewhat lower than that at the previous landing sites (2 x 10(5) to 6 x 10(5) dynes per square centimeter or 3 to 8 pounds per square inch). The results of the erosion experiment, the spacecraft landing effects, and other observations indicate that the soil has significant amounts of fine-grained material and a measurable cohesion.