Scientists Find 27 New Planets Around Two Stars

A2

Scientists Find 27 New Planets Around Two Stars

Introduction

Scientists used a NASA satellite to find 27 possible planets. These planets move around two stars instead of one.

Main Body

Most planets move around one star. It is hard to find planets that move around two stars. Scientists used a new way to look for them. They looked at how the stars move and change time. They looked at 1,590 star systems. They found 27 possible planets. Some planets are small like Neptune. Other planets are very big. These stars are far from Earth. Scientists think there are many more planets in space. Old ways did not find them. Now, they can find thousands of new planets. They need to use big telescopes on Earth to be sure.

Conclusion

The study found many new possible planets. Now, scientists must check them again to be sure.

Learning

🌌 The 'Comparing' Trick

To reach A2, you need to show how things are different. Look at these words from the text:

  • Small \rightarrow Big
  • One \rightarrow Many
  • Old \rightarrow New

How to use this in a sentence: Instead of saying "The planet is big," try comparing it:

  • "Some planets are small, but others are very big."

🛠️ Simple Action Words

The text uses simple words to describe a complex job. Notice how they repeat the word "Find":

  1. Find planets (Discover)
  2. Find thousands (Locate)

A2 Tip: You don't need fancy words like "discover" yet. Use "Find" for everything you locate in the world. It is clear and correct.

Vocabulary Learning

scientists
people who study and research science
Example:The scientists collected data from the experiment.
satellite
a small object that travels around a larger object in space
Example:The satellite sent pictures of the Earth.
find
to discover or locate something
Example:They find new planets using a telescope.
possible
able to be done or achieved
Example:There are many possible ways to solve the problem.
planets
large round bodies that orbit stars
Example:The planets in our solar system include Earth and Mars.
move
to change position or location
Example:The planets move around the stars.
around
surrounding or in the area of
Example:The planets orbit around the sun.
stars
bright balls of gas that shine in space
Example:The night sky is full of stars.
hard
difficult or not easy
Example:It is hard to find planets that orbit two stars.
new
recently made or discovered
Example:They used a new method to find planets.
look
to observe or examine
Example:They looked at how the stars move.
time
the ongoing sequence of events
Example:The stars change over time.
B2

Researchers Find 27 Potential Planets Orbiting Two Stars

Introduction

Scientists have used data from NASA's Transiting Exoplanet Survey Satellite (TESS) to find 27 potential exoplanets that orbit binary star systems.

Main Body

In the past, finding circumbinary planets—planets that orbit two stars—was difficult because the planet had to align perfectly with the observer's line of sight. This method has only found about 18 confirmed planets, which is far fewer than the 6,000 planets found orbiting single stars. To solve this problem, a team led by Margo Thornton from the University of New South Wales used a different technique called apsidal precession. This method focuses on measuring timing changes in stellar eclipses, which can show the gravitational pull of a hidden third body. After analyzing 1,590 binary systems using TESS data from at least two years, the researchers found 36 systems with unusual behavior. After removing other possible causes, such as rotational effects, they determined that 27 of these candidates have masses similar to planets. These candidates vary greatly in size, ranging from about 12 Earth masses (similar to Neptune) to 3,200 Earth masses (ten times the mass of Jupiter). These systems are located between 650 and 18,000 light-years away from Earth. If these findings are confirmed, the 1.7% detection rate suggests that many circumbinary planets have been missed. The researchers emphasized that the current lack of known planets is likely due to the limits of our detection tools rather than a lack of planets in space. Consequently, applying this method to larger datasets could reveal thousands of new planets. However, final confirmation requires ground-based measurements to determine the exact masses of these objects.

Conclusion

This study has increased the number of potential circumbinary planets, although further verification is needed to confirm their status.

Learning

🚀 From Simple Lists to Complex Connections

An A2 student says: "The method is new. It finds more planets." A B2 student says: "Applying this method to larger datasets could reveal thousands of new planets."

🔍 The Magic of 'Nominalization'

Look at the phrase "Applying this method."

Instead of starting with a person (The scientists apply...), the author turns the action apply into a noun applying. This is the secret bridge to B2 fluency. It allows you to discuss concepts rather than just actions.

How to shift your level:

  • A2 (Action-based): We analyzed the data and found 36 systems.
  • B2 (Concept-based): After analyzing 1,590 binary systems, the researchers found 36 systems.

🛠️ Precision Modifiers

B2 speakers don't just use "very" or "big." They use specific adjectives to show the exact relationship between things. Notice these from the text:

  • "Potential" (Not just 'maybe', but 'having the possibility to become')
  • "Unusual" (Not just 'strange', but 'differing from the norm')
  • "Ground-based" (A compound adjective that provides a specific location/method)

💡 The "Likely" Logic

In the article, the author writes: "...is likely due to the limits of our detection tools."

Stop using "maybe" for everything. Use "likely due to" when you want to explain a probable cause. It transforms your English from a basic conversation to an academic observation.

Example Transformation:Maybe I am late because of traffic. (A2) ✅ My lateness is likely due to the heavy traffic. (B2)

Vocabulary Learning

circumbinary
adj: orbiting around a pair of stars
Example:Circumbinary planets can only be seen when they transit both stars in a binary system.
exoplanet
noun: a planet that orbits a star outside our solar system
Example:The TESS telescope has identified thousands of exoplanets around distant stars.
binary
adj: consisting of two parts; noun: a system of two stars orbiting each other
Example:A binary star system consists of two stars orbiting a common centre of mass.
apsidal precession
noun: the slow rotation of a planet's orbit around a star, causing its closest point to shift over time
Example:Astronomers use apsidal precession to detect unseen planets in binary systems.
gravitational
adj: relating to the force of attraction between masses
Example:The gravitational pull of a planet can cause tiny variations in a star's brightness.
hidden
adj: not visible or known, concealed
Example:Scientists suspect there is a hidden third body affecting the eclipses.
rotational
adj: relating to rotation or spinning
Example:Rotational effects can mimic the signals that astronomers look for in planet detection.
masses
noun: the quantity of matter in an object
Example:The masses of the candidates were compared with those of known planets.
detection
noun: the act of discovering or identifying something
Example:The detection rate of circumbinary planets remains low compared to single-star planets.
dataset
noun: a structured set of data collected for analysis
Example:Analyzing larger datasets could uncover many more planets.
verification
noun: the process of confirming that something is true or correct
Example:Ground-based measurements are required for verification of the candidates.
line of sight
noun: the straight path from an observer to an object
Example:The planet must be aligned with the observer's line of sight to be detected.
C2

Identification of Twenty-Seven Circumbinary Planet Candidates via Apsidal Precession Analysis

Introduction

Researchers have utilized data from NASA's Transiting Exoplanet Survey Satellite (TESS) to identify 27 potential exoplanets orbiting binary star systems.

Main Body

Historically, the detection of circumbinary planets—celestial bodies orbiting two stars—has been constrained by the requirement of precise orbital alignment relative to the observer's line of sight. This transit-based methodology has yielded approximately 18 confirmed circumbinary worlds, a figure significantly lower than the 6,000-plus planets identified orbiting single stars. To mitigate this observational bias, a research team led by Margo Thornton of the University of New South Wales implemented a survey focusing on apsidal precession. This technique involves the precise measurement of timing variations in mutual stellar eclipses, which may indicate the gravitational influence of a non-luminous third body. Upon the analysis of 1,590 binary systems utilizing TESS data spanning at least two years, the researchers identified 36 systems exhibiting anomalous behavior. After accounting for tidal interactions, rotational effects, and general relativity, 27 of these candidates were determined to possess masses consistent with planetary bodies. These candidates exhibit a wide mass range, estimated between 12 Earth masses (approximately Neptune-sized) and 3,200 Earth masses (roughly ten times the mass of Jupiter). The identified systems are located at distances ranging from 650 to 18,000 light-years from Earth. Should these findings be validated, the resulting 1.7% detection rate suggests a substantial undercounting of circumbinary planets. The researchers posit that the current paucity of known circumbinary worlds is a function of detection limitations rather than a lack of physical occurrence. Consequently, the application of this method across larger datasets may reveal a population of thousands of previously undetected planets. Final confirmation of these candidates necessitates ground-based radial velocity measurements to determine precise stellar oscillations and planetary masses.

Conclusion

The study has expanded the known catalog of potential circumbinary planets, awaiting further spectroscopic verification to confirm their planetary status.

Learning

The Architecture of 'Academic Hedging' and Causal Nuance

To move from B2 (competent) to C2 (mastery), a student must transition from stating facts to constructing arguments using probabilistic language. This text is a masterclass in epistemic modality—the linguistic expression of how certain a writer is about their claims.

1. The 'Conditional Logic' of Scientific Validation

Observe the structural pivot: "Should these findings be validated..."

  • The C2 Shift: Instead of using a standard first-conditional ("If these findings are validated"), the author employs inverted conditionals. By omitting "if" and shifting the auxiliary verb "should" to the front, the prose achieves a formal, detached tone that is quintessential to high-level academic discourse. This suggests a hypothetical scenario with a degree of professional caution.

2. Lexical Precision in Quantifying Absence

Consider the phrase: "...the current paucity of known circumbinary worlds is a function of detection limitations..."

  • Paucity vs. Lack: While a B2 student uses "lack" or "small number," the C2 writer uses paucity. This doesn't just mean "few"; it implies a scarcity that is perhaps unexpected or problematic.
  • "Is a function of": This is a sophisticated replacement for "is caused by." It frames the relationship not as a simple A \rightarrow B cause, but as a mathematical or systemic correlation. This is the hallmark of precise, multi-disciplinary English.

3. The Nuance of 'Positing' vs. 'Suggesting'

  • "The researchers posit that..."

In C2 English, positing is distinct from suggesting or claiming. To posit is to put forward a premise as the basis for further argument. It is a more assertive intellectual move than "suggesting," yet it remains shielded from the arrogance of "proving."


Linguistic Synthesis for the Learner: To emulate this level of mastery, avoid direct causal verbs (cause, make, lead to). Instead, utilize systemic framing (is a function of, is contingent upon) and inverted hypotheticals (Should X occur, Were Y to be) to create a layer of professional distance and analytical rigor.

Vocabulary Learning

circumbinary (adj.)
Describing a planet that orbits around two stars instead of one.
Example:Circumbinary planets challenge traditional models of planetary formation.
constrained (adj.)
Limited or restricted by specific conditions or requirements.
Example:The detection of circumbinary planets has been constrained by observational limitations.
transit-based (adj.)
Methods that rely on observing the dimming of starlight as a planet passes in front of its host star.
Example:Transit-based techniques are the most common way to discover exoplanets.
methodology (n.)
A system of methods used in a particular area of study or activity.
Example:The researchers employed a novel methodology to analyze apsidal precession.
yielded (v.)
Produced or gave as a result.
Example:The survey yielded 18 confirmed circumbinary worlds.
confirmed (adj.)
Verified as being true or accurate.
Example:Only 18 of the detected planets were confirmed as circumbinary.
bias (n.)
A systematic error that leads to an incorrect conclusion.
Example:Observational bias can skew the perceived frequency of exoplanets.
mitigate (v.)
To reduce or alleviate the severity of something.
Example:They designed the study to mitigate the effects of detection bias.
apsidal precession (n.)
The gradual rotation of an orbit's major axis over time.
Example:Apsidal precession can reveal hidden gravitational influences.
precise (adj.)
Exact or accurate to a very fine degree.
Example:Precise timing measurements are essential for detecting subtle variations.
measurement (n.)
The act of determining the size, amount, or degree of something.
Example:Accurate measurement of eclipse timing is crucial.
timing variations (n.)
Changes in the expected times of events, often indicating external influences.
Example:Timing variations in eclipses can signal the presence of a third body.
mutual (adj.)
Shared or common between two parties or objects.
Example:Mutual eclipses occur when both stars eclipse each other.
eclipses (n.)
An event where one celestial body moves into the shadow of another.
Example:Eclipses provide valuable data about orbital dynamics.
non-luminous (adj.)
Lacking visible light emission.
Example:A non-luminous third body would not emit detectable light.
anomalous (adj.)
Deviating from what is standard, normal, or expected.
Example:The system exhibited anomalous behavior in its light curve.
tidal interactions (n.)
Gravitational effects between bodies that can alter their orbits and rotations.
Example:Tidal interactions can alter the orbits of binary stars.
rotational effects (n.)
Influences caused by the rotation of a celestial body.
Example:Rotational effects influence the shape of the stars.
general relativity (n.)
Einstein's theory describing gravity as the curvature of spacetime.
Example:General relativity predicts subtle orbital precessions.
masses (n.)
The amount of matter in an object.
Example:The candidates' masses were consistent with planetary bodies.
consistent (adj.)
In agreement or harmony with something else.
Example:Their masses were consistent with those of known planets.
planetary bodies (n.)
Objects such as planets that orbit a star.
Example:Planetary bodies orbiting binary stars are rare.
mass range (n.)
The span between the smallest and largest masses considered.
Example:The mass range spanned from 12 to 3,200 Earth masses.
estimated (adj.)
Calculated or approximated based on available data.
Example:The mass was estimated using dynamical models.
approximately (adv.)
Near to or about a certain value.
Example:The mass was approximately Neptune-sized.
roughly (adv.)
In a rough or approximate sense.
Example:The mass was roughly ten times Jupiter's.
distances (n.)
The space between two points or objects.
Example:The systems lie at distances ranging from 650 to 18,000 light-years.
validated (adj.)
Confirmed as correct or reliable.
Example:The findings would be validated by further observations.
detection rate (n.)
The proportion of successful detections relative to the total number of attempts.
Example:The detection rate was only 1.7%.
substantial (adj.)
Large in amount, degree, or importance.
Example:The study suggests a substantial undercounting.
undercounting (n.)
The act of counting fewer items than actually exist.
Example:Undercounting may hide many hidden planets.
paucity (n.)
A scarcity or lack of something.
Example:There is a paucity of known circumbinary worlds.
function (n.)
A particular role or purpose that something serves.
Example:The paucity is a function of detection limitations.
detection limitations (n.)
Constraints that reduce the ability to detect objects.
Example:Detection limitations hinder discovery.
physical occurrence (n.)
The actual existence of an event or object in reality.
Example:The physical occurrence of such planets may be common.
population (n.)
A group of individuals or objects of the same type.
Example:The population of circumbinary planets could be large.
previously undetected (adj.)
Not noticed or identified before.
Example:Many planets may have been previously undetected.
confirmation (n.)
The act of verifying or establishing the truth of something.
Example:Confirmation requires radial velocity measurements.
ground-based (adj.)
Operated from the Earth's surface rather than from space.
Example:Ground-based telescopes provide complementary data.
radial velocity (n.)
The component of an object's motion directed toward or away from the observer.
Example:Radial velocity measurements reveal stellar wobble.
oscillations (n.)
Regular variations or fluctuations in a system.
Example:Stellar oscillations help determine mass.
spectroscopic verification (n.)
Confirmation of an object's properties through analysis of its spectrum.
Example:Spectroscopic verification confirms planetary status.
catalog (n.)
A systematic list or record of items.
Example:The catalog now includes 27 new candidates.