Status of the James Webb Space Telescope

The James Webb Space Telescope (JWST) is a large aperture (6.5 meter), cryogenic space telescope with a suite of near and mid-infrared instruments covering the wavelength range of 0.6 J,Jm to 28 J,Jm. JWST's primary science goal is to detect and characterize the first galaxies. It will also study the assembly of galaxies, star formation, and the formation of evolution of planetary systems. JWST is a segmented mirror telescope operating at approx.40K, a temperature achieved by passive cooling of the observatory, via a large, 5-layer membrane-based sunshield. We present an overview of the observatory design, the mission science objectives, the integration and test program and review the concept for science operations of JWST. With construction of the observatory progressing rapidly across all elements of the observatory, we will report on recent highlights such as the completion of the first JWST primary mirror segment. We will also review the predicted performance of the JWST observatory, based on initial measurements of the telescope optics and instrumentation

Overview of the James Webb Space Telescope

The James Webb Space Telescope (JWST) is ulxve uperk/rc (6.5 meter), cryogenic space telescope with a suite of near and mid-infrared instruments covering the wavelength range of 0.6 prnio 28 pn). JWS7 s primaryacicoce goal is k) detect and characterize the first galaxies. U will also study the uascrob|y of galaxies, uiur bzcrou1ion, and the formation of evolution of planetary systems. Recent progress in hardware development for the observatory will he presented, including a discussion of the status of JWST's optical system and Beryllium mirror fabrication, progress with sunshield prototypes, and the integration and test configuration. We also review the expected scientific performance of the observatory for observations of exosolar planets by means of transit imaging and spectroscopy. We will review the science goals, the capabilities of each science instrument, and the design and operation of the telescope

Toward Metal Complexes That Can Directionally Walk Along Tracks: Controlled Stepping of a Molecular Biped with a Palladium(II) Foot

We report on the design, synthesis, and operation of a bimetallic molecular biped on a three-foothold track. The “walker” features a palladium­(II) complex “foot” that can be selectively stepped between 4-dimethylaminopyridine and pyridine ligand sites on the track via reversible protonation while the walker remains attached to the track throughout by means of a kinetically inert platinum­(II) complex foot. The substitution pattern of the three ligand binding sites, together with the kinetic stability of the metal–ligand coordination bonds, affords the two positional isomers a high degree of metastability, meaning that altering the chemical state of the track does not automatically instigate stepping in the absence of an additional stimulus (heat in the presence of a coordinating solvent). The use of metastable metal complexes for foot–track interactions offers a promising alternative to dynamic covalent chemistry for the design of small-molecule synthetic molecular walkers