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Interstellar Objects: A Look Beyond Our Solar System

Scientists study interstellar objects for clues about their origins and movements.

Shokhruz Kakharov, Abraham Loeb

― 6 min read


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Table of Contents

Over the past few years, scientists have discovered several objects that come from outside our solar system, such as 'Oumuamua and Borisov. These discoveries have led to increased interest in understanding where these objects come from and how they move through our galaxy, the Milky Way. The goal of this exploration is to learn more about their origins and the processes that created them.

To study these Interstellar Objects, researchers track their paths through the gravitational field of the Milky Way. They begin by measuring the speed of each object in relation to the Local Standard of Rest, which is a frame of reference for objects near our Sun. Additionally, they focus on the vertical movement of the objects relative to the plane of the Milky Way. This movement can help estimate the age of the objects since older stars tend to be found farther from the mid-plane of the galaxy.

For instance, 'Oumuamua’s low vertical movement may indicate it originated from a younger region of the Milky Way, suggesting it is less than 1-2 billion years old. On the other hand, Borisov has a vertical movement similar to that of the Sun, which hints it might also be of a similar age. The meteor IM1 shows even greater vertical movement, indicating it likely comes from an older region.

In addition to studying these interstellar objects, scientists also look at human-made probes like Voyager 1 and Pioneer 10. These probes are expected to reach the far side of the Milky Way relative to the Sun in several billion years.

The Discovery of Interstellar Objects

The recent discovery of interstellar objects has raised many questions about their origins. It is crucial to figure out where these objects come from to learn more about their nature and the astrophysical processes that lead to their formation. Researchers aim to identify their potential sources within the Milky Way.

With the help of numerical methods, scientists can trace the paths of these interstellar objects back in time. This allows them to connect the objects to possible stellar populations. They simplify their calculations by ignoring temporary features, such as spiral arms in the Milky Way, which is reasonable for studying orbits in the outer regions.

By retracing the orbits of these objects, researchers can narrow down the possible areas in the Milky Way where they originated. This information also provides important hints about the conditions in the galaxy at the time of their formation.

Methodology

To carry out their study, scientists rely on computer models that simulate the gravitational potential of the Milky Way. They assume certain values for the circular speed around the galactic center and the distance from the center to our Sun. By using the measured speeds of interstellar objects against the Local Standard of Rest, they can plot their paths over billions of years.

The researchers also factor in the movement of the Sun itself, as it also affects observations of these interstellar objects. They analyze past movements of these objects and create visual representations of their paths over time. These graphs help illustrate how far these objects stray from the main plane of the Milky Way and gather information about their velocities.

Individual Interstellar Objects

Comet Borisov

One of the notable interstellar objects is the comet Borisov. Researchers have tracked its distance from the Sun over a period of approximately 3.2 billion years, determining that it was located on the opposite side of the Milky Way relative to the Sun about 1.6 billion years ago. The distance and path of Borisov resemble those of our Sun, suggesting that they might share a similar age.

'Oumuamua

Another famous object is 'Oumuamua, which has shown a different pattern. Its distance from the Sun also varies over time, but it is evident that it was on the other side of the Milky Way relative to the Sun about 1.1 billion years ago. Due to its lower vertical movement, 'Oumuamua is thought to be younger, with estimates suggesting it is less than 1-2 billion years old.

Meteor IM1

IM1 is yet another interstellar object being studied. Its path indicates it was on the opposite side of the Milky Way relative to the Sun around 2.15 billion years ago. IM1 has a greater vertical movement compared to the others, suggesting it likely comes from an older region of the galaxy.

Estimating the Ages of the Objects

By analyzing the vertical movements of these interstellar objects, researchers can estimate their ages. They utilize data about star formation in the Milky Way to inform their models. The relationship between the vertical height of stars and their ages allows scientists to gauge how long each interstellar object has been moving through space.

Star formation rates in the Milky Way have been studied and divided into several segments, with some periods showing consistent star formation while others reveal bursts of activity. By combining this information with the measured vertical heights of the interstellar objects, researchers can create a probability distribution for the likely ages of each object.

Age Distribution Insights

Different interstellar objects show varying age distributions based on their vertical movements. For example, Borisov displays an age distribution that is close to that of the Sun, while 'Oumuamua appears to be much younger. On the other hand, IM1 follows a broader age distribution, suggesting it may originate from a diverse stellar population.

Future of Human-Made Probes

Aside from studying natural interstellar objects, researchers have also looked at the future paths of human-made probes such as Voyager 1 and Voyager 2. Unlike the interstellar objects, these probes have been traveling out of our solar system for decades. Scientists predict that in the coming billions of years, these probes will reach the far side of the Milky Way relative to the Sun.

The distances that these probes will travel over time have been calculated, and their movement will take them far away, only to return to our solar vicinity well before our Sun transforms into a red giant star. This long journey illustrates both the possibilities and challenges of space exploration.

Conclusion

In summary, the study of interstellar objects and their orbits offers valuable insights into the workings of our galaxy. By understanding where these objects come from and how they move, researchers can gain a better understanding of the nature of the Milky Way itself. The comparisons made between interstellar objects and human-made probes highlight the ongoing quest for knowledge and exploration in space.

As scientists continue to study these fascinating objects, they contribute to a broader understanding of cosmic processes and the potential for discovering more about our universe. Each new discovery brings us one step closer to unraveling the mysteries of the stars and the paths they travel.

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