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See what James Webb and Hubble are observing right now with this tool

If you’re looking for a relaxing way to peruse the fascinating sights of space on your lunch break, then a newly updated tool from NASA has you covered. The Space Telescope Live tools show the current targets of the James Webb Space Telescope and the Hubble Space Telescope, letting you browse the cosmos from the perspective of two of the hardest-working telescopes out there.

You can visit the web-based tools at WebbTelescope for the James Webb Space Telescope and HubbleSite for the Hubble Space Telescope. Clicking on a link will bring you to a portal showing the current and past observations of the telescope and a ton of detail about the observations.

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At time of writing, for example, the tracker shows James Webb observing a region called HST10 using its NIRSpec and MIRI instruments. This particular observation is part of a project using MIRI’s integral field unit (IFU), a spectroscopy mode that can observe either single stars or larger targets like nebulae. The study is looking at gas, dust, and molecules called polycyclic aromatic hydrocarbons (PAHs) in protoplanetary disks, which are the disks of matter from which planets form.

A screenshot of Webb's current observation target, HST10.
A screenshot of Webb’s current observation target, HST10. Space Telescope Live: NASA, ESA, CSA, STScI, and CDS.

The images you see on the tracker aren’t the live images being pulled straight from the telescope, as that data still needs to be processed. Instead, they use existing data from projects like the Two Micron All Sky Survey and the Digitized Sky Survey 2 that show images of the region that the telescope is currently pointed at.

When you see the current target through the tracker, you can use the Observation Details button at the top right to pull up information about the instruments being used, the science topics being researched, and the particular project and principal investigator of the research.

You can also see a schedule of when observations started and ended, and their total duration — they are often shorter than you might imagine. The above observation, for example, lasted less than 90 minutes. Typically, projects have multiple observation blocks over a period of months, but with many different researchers wanting precious time on the telescope, the project planners have to be very efficient with the time they are allotted.

You can also click through older observations using the Previous Target and Next Target buttons. In addition to showing you the variety of objects that the telescopes observe, from nebulae to stars to galaxies, this also gives you a sense of how the telescope tracks its targets across the sky — and it also shows how many different observations get squeezed into a day.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb Telescope captures gorgeous galaxy with a hungry monster at its heart
Featured in this new image from the NASA/ESA/CSA James Webb Space Telescope is Messier 106, also known as NGC 4258. This is a nearby spiral galaxy that resides roughly 23 million light-years away in the constellation Canes Venatici, practically a neighbour by cosmic standards. Messier 106 is one of the brightest and nearest spiral galaxies to our own and two supernovae have been observed in this galaxy in 1981 and 2014.

A new image from the James Webb Space Telescope shows off a nearby galaxy called Messier 106 -- a spiral galaxy that is particularly bright. At just 23 million light-years away (that's relatively close by galactic standards), this galaxy is of particular interest to astronomers due to its bustling central region, called an active galactic nucleus.

The high level of activity in this central region is thought to be due to the monster that lurks at the galaxy's heart. Like most galaxies including our own, Messier 106 has an enormous black hole called a supermassive black hole at its center. However, the supermassive black hole in Messier 106 is particularly active, gobbling up material like dust and gas from the surrounding area. In fact, this black hole eats so much matter that as it spins, it warps the disk of gas around it, which creates streamers of gas flying out from this central region.

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James Webb takes rare direct image of a nearby super-Jupiter
Artist’s impression of a cold gas giant orbiting a red dwarf. Only a point of light is visible on the JWST/MIRI images. Nevertheless, the initial analysis suggests the presence of a gaseous planet that may have properties similar to Jupiter.

Even with huge ground-based observatories and the latest technology in space-based telescopes, it's still relatively rare for astronomers to take an image of an exoplanet. Planets outside our solar system are so far away and so small and dim compared to the stars they orbit that it's extremely difficult to study them directly. That's why most observations of exoplanets are made by studying their host stars. Now, though, the James Webb Space Telescope has directly imaged a gas giant -- and it's one of the coldest exoplanets observed so far.

The planet, named Epsilon Indi Ab, is located 12 light-years away and has an estimated temperature of just 35 degrees Fahrenheit (2 degrees Celsius). The fact it is so cool compared to most exoplanets meant that Webb's sensitive instruments were needed to study it.

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One half of this wild exoplanet reaches temperatures of 1,450 degrees Fahrenheit
webb wasp 39b dayside nightside stsci 01j2f12rm1s3n39yj938nhsf93 png

This artist’s concept shows what the exoplanet WASP-39 b could look like based on indirect transit observations from JWST and other space- and ground-based telescopes. Data collected by its NIRSpec (Near-Infrared Spectrograph) show variations between the morning and evening atmosphere of the planet. NASA, ESA, CSA, Ralf Crawford (STScI)

One of the ground-breaking abilities of the James Webb Space Telescope is that researchers can use it to not only detect distant planets but also to peer into their atmosphere. Now, new research using Webb has uncovered differing conditions between morning and evening on a distant exoplanet, the first time such differences have been observed on a planet outside our solar system.

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