Are there any additional mechanisms for haemolysis in HELLP syndrome?

HELLP syndrome is a microangiopathy that leads to severe maternal complications. The objective of this study was to identify any additional mechanisms that could have contributed to HELLP syndrome-induced haemolysis. This is a pilot, prospective and observational study that lasted 9months. All patients with HELLP syndrome treated at academic tertiary care women hospital accepted to participate. Sixteen patients were included. In ten patients (63%), schizocytes were detected following a blood smear test. Six patients (38%) were diagnosed with a partial expression deficiency of proteins regulating the complement system (CD 55 or CD 59). In nine patients (56%), an activation of the complement classical pathway was detected. In two patients (13%), an ADAMTS 13 activity below 30% was detected. Three patients (19%) were diagnosed with a folate deficiency and one (6%) with an antiphospholipid syndrome. All patients developed maternal or fetal morbidity including nine (56%) an acute kidney injury. All patients but one had at least one additional mechanism that could contribute to haemolysis, besides a simple physical injury. Larger studies should be promoted to understand haemolysis in HELLP syndrome.

Clostridium difficile colitis acquired in the intensive care unit: outcome and prognostic factors.

PURPOSE: We assessed factors associated with mortality and complicated course in the case of Clostridium difficile infection (CDI) acquired in the intensive care unit (ICU). METHOD: Retrospective cohort study conducted from 1 January 2002 through 1 January 2012. All patients who acquired CDI in our ICU were included. RESULTS: Thirty-one patients were included. Twenty patients (65 %) had mild colitis, 8 (25 %) moderate colitis, and 3 (10 %) severe colitis. Initial antibiotherapy was metronidazole (n = 30, 97 %) and vancomycin (n = 1, 3 %). Seventeen patients (55 %) experienced at least one complication: failure of initial treatment (n = 16, 52 %), shock (n = 11, 34 %), need for surgery (n = 1, 3 %) or renal replacement (n = 4, 13 %), or death (n = 8, 26 %). Risk factors of ICU mortality were history of corticosteroids prescription, prolonged ICU stay, low serum albumin level, and high Sequential Organ Failure Assessment (SOFA) score at the time of CDI diagnosis. Factors associated with a complicated course were high Simplified Acute Physiology Score (SAPS II), high SOFA score, and low serum albumin level at the time of CDI onset. CONCLUSION: Risk factors of poor outcome in patients with CDI acquired in the ICU are different from those in the general population suffering from CDI. The implementation of treatment algorithms taking into account these factors may reduce complication rates in this specific population.

Images of asteroid 21 Lutetia: a remnant planetesimal from the early Solar System.

Images obtained by the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) cameras onboard the Rosetta spacecraft reveal that asteroid 21 Lutetia has a complex geology and one of the highest asteroid densities measured so far, 3.4 ± 0.3 grams per cubic centimeter. The north pole region is covered by a thick layer of regolith, which is seen to flow in major landslides associated with albedo variation. Its geologically complex surface, ancient surface age, and high density suggest that Lutetia is most likely a primordial planetesimal. This contrasts with smaller asteroids visited by previous spacecraft, which are probably shattered bodies, fragments of larger parents, or reaccumulated rubble piles.

E-type asteroid (2867) Steins as imaged by OSIRIS on board Rosetta.

The European Space Agency's Rosetta mission encountered the main-belt asteroid (2867) Steins while on its way to rendezvous with comet 67P/Churyumov-Gerasimenko. Images taken with the OSIRIS (optical, spectroscopic, and infrared remote( )imaging system) cameras on board Rosetta show that Steins is an oblate body with an effective spherical diameter of 5.3 kilometers. Its surface does not show color variations. The morphology of Steins is dominated by linear faults and a large 2.1-kilometer-diameter crater near its south pole. Crater counts reveal a distinct lack of small craters. Steins is not solid rock but a rubble pile and has a conical appearance that is probably the result of reshaping due to Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) spin-up. The OSIRIS images constitute direct evidence for the YORP effect on a main-belt asteroid.