TM completed segments: 4

Other segments: 11

TM completed words: 62

Other words: 271

TM Completed sentences

Original Translated
Regular editor pl Regular editor
Nam liber tempor cum soluta nobis eleifend option congue nihil imperdiet doming id quod mazim placerat facer possim assum. pl Nam liber tempor cum soluta nobis eleifend option congue nihil imperdiet doming id quod mazim placerat facer possim assum.
Lorem ipsum dolor sit amet, consectetuer adipiscing elit, sed diam nonummy nibh euismod tincidunt ut laoreet dolore magna aliquam erat volutpat. pl Lorem ipsum dolor sit amet, consectetuer adipiscing elit, sed diam nonummy nibh euismod tincidunt ut laoreet dolore magna aliquam erat volutpat.
Ut wisi enim ad minim veniam, quis nostrud exerci tation ullamcorper suscipit lobortis nisl ut aliquip ex ea commodo consequat. pl Ut wisi enim ad minim veniam, quis nostrud exerci tation ullamcorper suscipit lobortis nisl ut aliquip ex ea commodo consequat.

Other sentences

Original Similar TM records
The sun, a massive star located at the center of our solar system, is the ultimate source of energy for Earth.
It is a nearly perfect sphere of hot plasma, with internal convective motions that generate a magnetic field via a dynamo process.
Approximately 109 times wider than Earth, the sun's vast size accounts for about 99.86% of the total mass of the solar system.
This immense gravity holds the solar system together, keeping everything from the largest planets to the smallest particles in orbit.
From a scientific perspective, the sun is classified as a G-type main-sequence star (G2V), often referred to as a yellow dwarf.
Its core is incredibly hot and dense, where nuclear fusion converts hydrogen into helium, releasing energy that powers the sun and provides light and warmth to our planet.
This energy is critical for climate and weather systems on Earth and drives the basic processes of all living organisms through photosynthesis in plants.
Despite its ubiquitous influence, the sun is considered a middle-aged star, at about 4.6 billion years old, and is expected to continue burning hydrogen for another 5 billion years.
The sun also plays a key role in shaping the conditions of space weather, with phenomena such as solar flares and coronal mass ejections impacting Earth's magnetic field and atmosphere.
These solar events can lead to beautiful natural displays like auroras, but they also pose risks to satellites, communications systems, and even power grids.
Understanding the sun's behavior is crucial for predicting and mitigating these effects, making solar science a vital field in both astronomical and applied research domains.