The geology and geophysics of Kuiper Belt object (486958) Arrokoth.

The Cold Classical Kuiper Belt, a class of small bodies in undisturbed orbits beyond Neptune, is composed of primitive objects preserving information about Solar System formation. In January 2019, the New Horizons spacecraft flew past one of these objects, the 36-kilometer-long contact binary (486958) Arrokoth (provisional designation 2014 MU69). Images from the flyby show that Arrokoth has no detectable rings, and no satellites (larger than 180 meters in diameter) within a radius of 8000 kilometers. Arrokoth has a lightly cratered, smooth surface with complex geological features, unlike those on previously visited Solar System bodies. The density of impact craters indicates the surface dates from the formation of the Solar System. The two lobes of the contact binary have closely aligned poles and equators, constraining their accretion mechanism.

The predictive and prognostic significance of liquid biopsy in advanced epidermal growth factor receptor-mutated non-small cell lung cancer: A prospective study.

OBJECTIVE: To determine the predictive and prognostic roles of three blood-based biomarkers: circulating tumour DNA (ctDNA), circulating tumour cells (CTC) and carcinoembryonic antigen (CEA), in patients with advanced epidermal growth factor receptor-mutated (EGFR+) lung cancer. MATERIALS AND METHODS: We recruited 28 patients with 103 serial blood samples. We performed mutational analyses for EGFR mutations using droplet digital PCR (ddPCR) on ctDNA. We evaluated the accuracy of EGFR mutation detection in ctDNA compared with tissue biopsy. We also quantified CTCs, ctDNA and CEA in serially collected blood samples, and evaluated the baseline and changes in these blood-based biomarkers with clinical outcomes. RESULTS: EGFR mutation detection in plasma was highly concordant as compared with tissue biopsy. Detectable baseline ctDNA was associated with higher disease burden (p < 0.01). Early disappearance of ctDNA at 4 weeks was associated with radiological response at 12 weeks of treatment (p = 0.01) and improved progression free survival (PFS) (HR 5.47, 95%CI 1.32-22.72, p = 0.02) and overall survival (OS) (HR 5.46, 95%CI 1.28-23.22, p = 0.02). A decrease in CTC count at 4 weeks was associated with improved PFS (HR 3.81, 95%CI 1.13-12.79, p = 0.03) but not OS. 85% of patients with radiological progression had a ctDNA rise compared with 22% of patients with stable disease (p=0.01). ctDNA rise was seen on average 170 days prior to radiological progression. There is a significant association between the rise of CEA level with radiological progression (p=0.001). CONCLUSION: Early change in ctDNA, CTC and CEA levels may be long-term predictors of treatment benefit and failure prior to availability of radiological response data.

Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt object.

The Kuiper Belt is a distant region of the outer Solar System. On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU69, a cold classical Kuiper Belt object approximately 30 kilometers in diameter. Such objects have never been substantially heated by the Sun and are therefore well preserved since their formation. We describe initial results from these encounter observations. MU69 is a bilobed contact binary with a flattened shape, discrete geological units, and noticeable albedo heterogeneity. However, there is little surface color or compositional heterogeneity. No evidence for satellites, rings or other dust structures, a gas coma, or solar wind interactions was detected. MU69's origin appears consistent with pebble cloud collapse followed by a low-velocity merger of its two lobes.

Impact craters on Pluto and Charon indicate a deficit of small Kuiper belt objects.

The flyby of Pluto and Charon by the New Horizons spacecraft provided high-resolution images of cratered surfaces embedded in the Kuiper belt, an extensive region of bodies orbiting beyond Neptune. Impact craters on Pluto and Charon were formed by collisions with other Kuiper belt objects (KBOs) with diameters from ~40 kilometers to ~300 meters, smaller than most KBOs observed directly by telescopes. We find a relative paucity of small craters ≲13 kilometers in diameter, which cannot be explained solely by geological resurfacing. This implies a deficit of small KBOs (≲1 to 2 kilometers in diameter). Some surfaces on Pluto and Charon are likely ≳4 billion years old, thus their crater records provide information on the size-frequency distribution of KBOs in the early Solar System.

Prebiotic Chemistry of Pluto.

We present the case for the presence of complex organic molecules, such as amino acids and nucleobases, formed by abiotic processes on the surface and in near-subsurface regions of Pluto. Pluto's surface is tinted with a range of non-ice substances with colors ranging from light yellow to red to dark brown; the colors match those of laboratory organic residues called tholins. Tholins are broadly characterized as complex, macromolecular organic solids consisting of a network of aromatic structures connected by aliphatic bridging units (e.g., Imanaka et al., 2004; Materese et al., 2014, 2015). The synthesis of tholins in planetary atmospheres and in surface ices has been explored in numerous laboratory experiments, and both gas- and solid-phase varieties are found on Pluto. A third variety of tholins, exposed at a site of tectonic surface fracturing called Virgil Fossae, appears to have come from a reservoir in the subsurface. Eruptions of tholin-laden liquid H2O from a subsurface aqueous repository appear to have covered portions of Virgil Fossae and its surroundings with a uniquely colored deposit (D.P. Cruikshank, personal communication) that is geographically correlated with an exposure of H2O ice that includes spectroscopically detected NH3 (C.M. Dalle Ore, personal communication). The subsurface organic material could have been derived from presolar or solar nebula processes, or might have formed in situ. Photolysis and radiolysis of a mixture of ices relevant to Pluto's surface composition (N2, CH4, CO) have produced strongly colored, complex organics with a significant aromatic content having a high degree of nitrogen substitution similar to the aromatic heterocycles pyrimidine and purine (Materese et al., 2014, 2015; Cruikshank et al., 2016). Experiments with pyrimidines and purines frozen in H2O-NH3 ice resulted in the formation of numerous nucleobases, including the biologically relevant guanine, cytosine, adenine, uracil, and thymine (Materese et al., 2017). The red material associated with the H2O ice may contain nucleobases resulting from energetic processing on Pluto's surface or in the interior. Some other Kuiper Belt objects also exhibit red colors similar to those found on Pluto and may therefore carry similar inventories of complex organic materials. The widespread and ubiquitous nature of similarly complex organic materials observed in a variety of astronomical settings drives the need for additional laboratory and modeling efforts to explain the origin and evolution of organic molecules. Pluto observations reveal complex organics on a small body that remains close to its place of origin in the outermost regions of the Solar System.

Seismicity on tidally active solid-surface worlds.

Tidal interactions between planets or stars and the bodies that orbit them dissipate energy in their interiors. The dissipated energy heats the interior and a fraction of that energy will be released as seismic energy. Here we formalize a model to describe the tidally-driven seismic activity on planetary bodies based on tidal dissipation. To constrain the parameters of our model we use the seismic activity of the Moon, driven by tidal dissipation from the Earth-Moon interactions. We then apply this model to predict the amount of seismic energy release and largest seismic events on other moons in our Solar System and exoplanetary bodies. We find that many moons in the Solar System should be more seismically active than the Earth's Moon and many exoplanets should exhibit more seismic activity than the Earth. Finally, we examine how temporal-spatial variations in tidal dissipation manifest as variations in the locations and timing of seismic events on these bodies.

Statistical controversies in cancer research: using standardized effect size graphs to enhance interpretability of cancer-related clinical trials with patient-reported outcomes.

Patient reported outcomes (PROs) are becoming increasingly important in cancer studies, particularly with the emphasis on patient centered outcome research. However, multiple PROs, using different scales, with different directions of favorability are often used within a trial, making interpretation difficult. To enhance interpretability, we propose the use of a standardized effect size graph, which shows all PROs from a study on the same figure, on the same scale. Plotting standardized effects with their 95% confidence intervals (CIs) on a single graph clearly showing the null value conveys a comprehensive picture of trial results. We demonstrate how to create such a graph using data from a randomized controlled trial that measured 12 PROs at two time points. The 24 effect sizes and CIs are shown on one graph and clearly indicate that the intervention is effective and sustained.

The formation of Charon's red poles from seasonally cold-trapped volatiles.

A unique feature of Pluto's large satellite Charon is its dark red northern polar cap. Similar colours on Pluto's surface have been attributed to tholin-like organic macromolecules produced by energetic radiation processing of hydrocarbons. The polar location on Charon implicates the temperature extremes that result from Charon's high obliquity and long seasons in the production of this material. The escape of Pluto's atmosphere provides a potential feedstock for a complex chemistry. Gas from Pluto that is transiently cold-trapped and processed at Charon's winter pole was proposed as an explanation for the dark coloration on the basis of an image of Charon's northern hemisphere, but not modelled quantitatively. Here we report images of the southern hemisphere illuminated by Pluto-shine and also images taken during the approach phase that show the northern polar cap over a range of longitudes. We model the surface thermal environment on Charon and the supply and temporary cold-trapping of material escaping from Pluto, as well as the photolytic processing of this material into more complex and less volatile molecules while cold-trapped. The model results are consistent with the proposed mechanism for producing the observed colour pattern on Charon.

The small satellites of Pluto as observed by New Horizons.

The New Horizons mission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra. All four are small, with equivalent spherical diameters of ~40 kilometers for Nix and Hydra and ~10 kilometers for Styx and Kerberos. They are also highly elongated, with maximum to minimum axis ratios of ~2. All four moons have high albedos (~50 to 90%) suggestive of a water-ice surface composition. Crater densities on Nix and Hydra imply surface ages of at least 4 billion years. The small moons rotate much faster than synchronous, with rotational poles clustered nearly orthogonal to the common pole directions of Pluto and Charon. These results reinforce the hypothesis that the small moons formed in the aftermath of a collision that produced the Pluto-Charon binary.

The Pluto system: Initial results from its exploration by New Horizons.

The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition; its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected.

Disseminated intravascular coagulation in Still's disease.

Still's disease is characterized by arthritis, fever, rash, lymphoid hypertrophy, leukocytosis, and anemia, often in association with thrombocytosis. We describe a patient with Still's disease and thrombocytopenia secondary to disseminated intravascular coagulation (DIC). Fifteen definite cases of DIC complicating Still's disease have been reported in the English literature. Most developed this complication while receiving high doses of salicylates in association with hepatic dysfunction. In a few, the coagulopathy has been associated with gold therapy. Our patient is only the second reported to develop DIC in the absence of drug therapy and the fourth reported to die from this complication. The clinical features of these 16 patients are summarized and proposed mechanisms of pathogenesis are reviewed.

Antihistone antibody profile in sulfasalazine induced lupus.

Two patients developed drug induced lupus secondary to sulfasalazine (SSZ). One patient was receiving SSZ for Crohn's disease and was subsequently treated with olsalazine, which lacks the sulfapyridine component of SSZ. Her inflammatory bowel disease (IBD) remained controlled and she did not develop a recurrence of lupus, suggesting that olsalazine is safe in patients with IBD and a history of SSZ induced lupus. The SSZ induced antibodies were predominantly IgG against the (H2A-H2B)-DNA complex. Since lupus induced by 7 other drugs was associated with a similar antibody response, our findings support the existence of a common pathway for autoantibody induction.

Simultaneous presentation of thrombotic thrombocytopenic purpura and systemic lupus erythematosus.

An 18-year-old woman with thrombotic thrombocytopenic purpura (TTP) had recurrent thrombocytopenia due to antiplatelet antibodies associated with systemic lupus erythematosus (SLE). The simultaneous occurrence of TTP and SLE is rare. We briefly summarize eight previously reported cases in which these two diseases have developed in the same patient within a 12-month period. The possibility of a common pathogenesis is discussed.

The significance of hematuria in the anticoagulated patient.

BACKGROUND: There have been many case reports of substantial renal disease in association with anticoagulation, yet the intensity of anticoagulation has changed over the years. In 1986, the American College of Chest Physicians and the Heart, Lung, and Blood Institute recommended a decrease in anticoagulation intensity. In addition, a variety of new methods to investigate hematuria have evolved, including computed tomography and red blood cell morphologic analysis. Because of these developments, we initiated a prospective study to evaluate the relationship between anticoagulation, microscopic hematuria, and major genitourinary tract disease. METHODS: To determine the incidence, prevalence, and cause of microscopic hematuria, patients receiving long-term anticoagulation therapy and controls not receiving such therapy were monitored with monthly urinalyses in a 2-year prospective study. Patients who developed hematuria were further studied for genitourinary tract disease. The incidence of hematuria was analyzed with regard to relative levels of anticoagulation. RESULTS: The incidence of hematuria in the anticoagulated and control groups was 0.05 and 0.08 per 100 patient-months, respectively. The prevalence of hematuria was 3.2% in the anticoagulated group and 4.8% in the control group. Genitourinary tract disease was identified in 81% of patients with more than one episode of microscopic hematuria, and the cause of hematuria did not vary between groups. There was no correlation between the level of anticoagulation and the incidence of hematuria. CONCLUSIONS: Anticoagulation at currently recommended levels does not predispose patients to hematuria. Identifiable genitourinary tract disease is present in the majority of anticoagulated patients with microscopic hematuria.

Prostatic involvement in Wegener's granulomatosis.

Two cases of Wegener's granulomatosis presenting with prostatic involvement are described and compiled with the five previously detailed cases. Each of these patients presented with obstructive symptoms, proteinuria, leukocyturia, and hematuria. The urinary sediment normalized with treatment of the underlying granulomatous vasculitis. Wegener's granulomatosis is a rare cause of prostatic obstructive symptoms, but should be considered whenever the relatively unusual entity of granulomatous prostatitis is diagnosed. One patient was initially treated exclusively with trimethoprim-sulfamethoxazole (TMP-SMX). He responded, but noted recurrence during the 15th month of treatment. We also report on this patient's antineutrophil cytoplasmic antibody (ANCA) titers, which correlated with clinical assessment and predicted recurrence 2 months before elevation of the Westergren sedimentation rate (WSR) and clinical diagnosis.

Bioassays of smooth muscle contracting agents in cotton mill dust and bract extracts: arachidonic acid metabolites as possible mediators of the acute byssinotic reaction.

Byssinosis is an occupational respiratory disease contracted by cotton mill workers who inhale cotton mill dust. The acute byssinotic reaction is characterized by a drop in the 1-sec forced expiratory volume (FEV1.0) on Monday following a weekend's absence from work. This physiological reaction is the result of the contraction of bronchial smooth muscle, which causes narrowing of small airways. An isolated tissue bath technique was used to assay smooth muscle contractions induced by cotton dust extract (CDE) and cotton bract extract (CBE). CBE-induced contractions of rat stomach smooth muscle were blocked (82%) by 100 ng/ml methysergide (blocks 5-hydroxytryptamine (5HT) 100%); CDE was not significantly blocked by methysergide (13%). CDE-induced contractions were blocked (100%) by 25 micrograms/ml indomethacin and 100 micrograms/ml salicylic acid (blocks prostaglandin F2 alpha (PGF2 alpha) 100%). The portion of CBE contracting ability not blocked by methysergide was blocked totally by indomethacin. Blocking agents ineffective against CDE or CBE include atropine (acetylcholine blocker), pyrilamine maleate and diphenhydramine (histamine blockers), imidazole and 7-(1-imidazolyl)heptanoic acid (7IHA) (thromboxane blockers), and carboxypeptidase B2 (kinin blocker). The data suggest that cotton bract contains 5HT, which is responsible for a majority of the CBE-induced contraction and a minority of the CDE-induced contraction. The data also suggest that cotton dust and bract contain a substance which causes the release of PGF2 alpha which in turn causes the contraction of smooth muscle. This substance is responsible for a majority of the CDE-induced and a minority of the CBE-induced contractions. Radioimmunoassay (RIA) confirmed PGF2 alpha release from rat fundal smooth muscle when exposed to CDE and CBE. Increased synthesis and release of arachidonic acid metabolites might be a major mechanism in the bronchoconstriction observed in the acute byssinotic reaction.