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Protostar

101 Sentences | 9 Meanings

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The powerful jets of the protostar can create shockwaves in the surrounding gas and dust.
In the early stages of its formation, a protostar is still accumulating mass and heating up from the gravitational energy of its collapsing material.
The protostar in the center of the nebula emits powerful jets of gas and dust.
A protostar is a stage in the evolution of a star.
A protostar is a stage in the life cycle of a star.
A protostar is a large, dense cloud of gas and dust.
The formation of a protostar is a critical step in the creation of a new solar system.
A protostar is a young star that has not yet begun to shine.
The jets emanating from the protostar create spectacular celestial displays.
The accretion disk around a protostar is a hotbed of activity, with material constantly falling onto the star.
Observations of the protostar reveal that it is undergoing rapid accretion and emitting strong jets of material.
The young protostar emits powerful jets of gas and dust that are carving out a cavity in the surrounding cloud.
The protostar is the earliest stage in the formation of a star.
The protostar is still in its early stages and is not yet a full-fledged star.
The protostar is an important object for understanding the process of star formation.
The protostar is located at the center of a dense cloud of interstellar gas and dust.
The intense heat and pressure within the protostar causes it to emit strong radiation.
The astronomers discovered a protostar in the Orion Nebula using an infrared telescope.
The formation of a protostar can take millions of years as the gas and dust slowly collapses under its own gravity.
The protoplanetary disk surrounding the protostar began to cool and coalesce, forming planets.
The young protostar is surrounded by a dense disk of material and emits powerful jets.
The protostar is still accreting matter from the disk and has not yet reached its final size.
The protostar is surrounded by a flattened disk of gas and dust, from which planets may eventually form.
The protostar is accreting gas and dust from its surrounding disk and ejecting powerful jets of material.
The protostar begins as a small, dense core within a larger cloud of gas and dust.
The protostar will continue to grow in size and brightness as it evolves into a full-fledged star.
The protostar is surrounded by a cloud of gas and dust that will eventually form a planetary system.
The protostar gradually heats up as it continues to collapse, eventually reaching temperatures of millions of degrees.
A protostar can take millions of years to fully form into a main-sequence star.
The protostar V350 Cephei is known for its strong episodic accretion events.
The protostar is surrounded by a rotating disk of gas and dust.
The gravitational force within a protostar is so intense that it attracts gas and dust from its surroundings.
The scientists observed the protostar spewing out jets of gas and dust from its poles.
A protostar is an object in space that has not yet begun to generate energy through nuclear fusion.
The formation of a protostar involves the gravitational collapse of a dense cloud of gas and dust.
The protostar is approximately one million years old.
A protostar is a young star that hasn't reached the necessary mass for nuclear fusion.
The protostar will eventually become a main-sequence star.
The protostar will eventually develop nuclear fusion and become a full-fledged star.
The accretion disk around a protostar can provide clues about the materials that will eventually form planets.
A protostar can take millions of years to fully form and become a star.
The discovery of a protostar in our galaxy could help us learn more about the formation of stars.
The presence of a protostar in a molecular cloud can lead to the formation of planets.
The protostar is located in a star-forming region of the galaxy.
The protostar is a critical stage in the formation of a star.
A protostar is a stage in the formation of a star.
A protostar is a baby star that will grow up to shine brightly.
A protostar is a theoretical object that astronomers study to better understand the process of star formation.
The discovery of a protostar in a distant galaxy indicates that star formation is ongoing.
The protostar began to contract and increase in temperature, signaling the start of its evolution.
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