James Webb Space Telescope Feed Post

A JWST survey of the Trapezium Cluster & inner Orion Nebula. I. Observations & overview

A selection of well-known silhouette disks in the Orion Nebula as imaged in the near-infrared with JWST. In this figure, a section of the main SW colour composite (Figure 3) has been extracted. Each panel is a 7.8 arcsec square and a 1 arcsec (390 au) scale bar is shown. N is up and E left in all panels. The names in the top left corner encode the coordinate following the scheme of O’Dell & Wen (1994) with the prefix ‘d’ to indicate a disk: all objects have been previously catalogued from the various HST surveys (e.g., Bally et al. 2000; Ricci et al. 2008). The local brightness and contrast has adjusted to maximise the visibility of relevant features, but the colour mix has not been altered. Thus as in the main SW colour composite, purple and blue reveal ionised gas and reflection nebulosity, red shows H2 emission at 2.12 µm, and green shows [Fe II] emission at 1.64 µm. The features seen in the individual images are discussed in the text. Abstract: We present a near-IR survey of the Trapezium Cluster and inner Orion Nebula using the NASA/ESA/CSA James Webb Space Telescope. The survey with the NIRCam instrument covers 10.9 x 7.5 arcminutes (~1.25 x 0.85 pc) in twelve wide-, medium-, and narrow-band filters from 1-5 microns and is diffraction-limited at all wavelengths, providing a maximum spatial resolution of 0.063 arcsec at 2 microns, corresponding to ~25 au at Orion. The suite of filters chosen was designed to address a number of scientific questions including the form of the extreme low-mass end of the IMF into the planetary-mass range to 1 Jupiter mass and below; the nature of ionised and non-ionised circumstellar disks and associated proplyds in the near-IR with a similar resolution to prior HST studies; to examine the large fragmented outflow from the embedded BN-KL region at very high resolution and fidelity; and to search for new jets and outflows from young stars in the Trapezium Cluster and the Orion Molecular Cloud 1 behind. In this paper, we present a description of the design of the observational programme, explaining the rationale for the filter set chosen and the telescope and detector modes used to make the survey; the reduction of the data using the JWST pipeline and other tools; the creation of large colour mosaics covering the region; and an overview of the discoveries made in the colour images and in the individual filter mosaics. Highlights include the discovery of large numbers of free-floating planetary-mass candidates as low as 0.6 Jupiter masses, a significant fraction of which are in wide binaries; new emission phenomena associated with the explosive outflow from the BN-KL region; and a mysterious "dark absorber" associated with a number of disparate features in the region, but which is seen exclusively in the F115W filter. Further papers will examine those discoveries and others in more detail.