It resembles artwork from the '80s. The image above is very cool.

The first light image to be captured by the GHOST instrument is a star. The whole optical spectrum of light emitted by a star named HD 222925 is shown.

The director of the Gemini Observatory said that this is an exciting milestone for the astronomy community.

GHOST will be an essential component of the astronomer's toolkit once this next- generation instrument is commissioned.

The light we can see coming from stars is full of details about the distant sun's features.

It is possible to learn a lot about the star, such as how old it is, and where it formed, by looking at the entire spectrum.

Different elements absorb and re-emit light differently Calculating which elements are present in a star's atmosphere can be done with the help of brighter and dimmer wavelength information.

The absorption lines look similar in the image below.

The labeled spectrum of HD

There is a really odd star located around 1,460 light-years away. The most elements ever seen in a star's atmosphere were 65, most of which were heavy elements that can only be formed in extremely energetic events.

HD 222925, which is in a very late stage at the end of its life, most likely formed from a cloud that was rich in these elements in the first place.

There is no new information about the star in the new images from GHOST. The first image taken by a new telescope to check the telescope is working is the target of the instrument's first light. Scientists can make any necessary changes to the instrument.

Scientists and technicians are going to put GHOST through its paces to make sure it works as expected.

GHOST is likely to be ready for scientific observation around the first half of next year.

It will be something to watch out for. The GHOST is 10 times more powerful than the GMOS. Scientists say it's the most powerful and sensitive of its kind currently in use.

It is expected that GHOST will be able to provide fascinating insights on stars identified as interesting targets by other telescopes and surveys, and deliver us many more stars, split into their constituent wavelength.

The images were published by NOIR Lab.