Roman Telescope will send more than a million names into space on NASA mission

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Photo: Espaço, estrelas - janush/shutterstock.com

More than 1.3 million people will have their names traveling through space aboard the Nancy Grace Roman space telescope, which the American space agency, NASA, plans to launch on August 30, 2026. In addition to carrying the names of participants and astronauts on a memory card, the telescope will carry a commemorative plaque, paying tribute to the astronomer after whom the equipment is named and to everyone involved in space exploration.

Tribute to a pioneer of space exploration and to the public

The Nancy Grace Roman Telescope is named in honor of NASA’s first chief astronomer, a pivotal figure in the development of the agency’s modern scientific program. The commemorative plaque installed on the equipment seeks to recognize the contribution of scientists and enthusiasts who dedicate their efforts to understanding the universe. It is a symbolic gesture that celebrates the human passion for discovery.

Unlike the previously launched James Webb telescope, the Roman will feature this element that highlights public engagement. The initiative reflects the spirit of other NASA missions, such as robotic missions to Mars, which frequently include the public in their trips to space, reinforcing the connection between science and society.

NASA symbol
NASA symbol – 26ShadesOfGreen/Shutterstock.com

More than a million names on their way to the stars

A digital memory card, containing the names of exactly 1,350,144 people from different parts of the world, will accompany the telescope on its journey. Among the individuals who will have their names sent into space are the astronauts of the future Artemis II and Artemis III missions, highlighting the continuity of human exploration in conjunction with robotics.

This practice of including names on space missions is a way of democratizing participation in science, allowing ordinary citizens to feel part of great scientific endeavors. It’s a reminder that curiosity and the desire to unlock the mysteries of the cosmos are universal.

Mission destination and ambitious scientific objectives

The launch of the Roman telescope will be carried out by a Falcon Heavy rocket, departing from the Kennedy Space Center. After takeoff, the equipment will head to the second Sun-Earth Lagrange point (L2), a gravitationally stable position around 1.5 million kilometers from Earth, the same location as James Webb.

From its vantage point in space, Roman will begin an initial five-year period of operation, focused on three main scientific missions. These efforts are expected to result in the discovery of approximately 100,000 exoplanets, as well as hundreds of millions of galaxies and billions of stars, revealing rare cosmic objects and phenomena.

The telescope’s three main areas of research

About 75% of the Nancy Grace Roman Telescope’s observing time will be devoted to three crucial surveys designed to significantly expand our knowledge of the universe.

  • High-Latitude Wide-Area Survey:This mission’s main goal is to map more than a billion galaxies. The focus will be on regions of space far from the dusty plane of the Milky Way, allowing a clearer view of the large-scale structure of the cosmos.
  • High-Latitude Time-Domain Survey:With the aim of repeatedly observing the same area of ​​space, this survey will seek to document the evolution of cosmic objects and phenomena over time. It will provide valuable data about dynamic changes in the universe.
  • Galactic Bulge Time-Domain Survey:Astronomers will use this effort to capture detailed images of the Milky Way’s central bulge. The goal is to obtain the most in-depth views ever achieved into the heart of our own galaxy, revealing secrets of its formation and evolution.

In addition to these primary missions, the Roman telescope will also dedicate time to the Galactic Plane Survey, which will offer unprecedented images of the Milky Way, and other scientific projects that will be announced in the future, consolidating its role as an essential tool in modern astronomy.

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