After a successful launch in April this year, NASA’s newest planet hunter, the Transiting Exoplanet Survey Satellite (TESS), has now started its search for planets around nearby stars.
Officially beginning science operations on July 25, TESS is expected to transmit its first series of science data back to Earth in August, and thereafter periodically every 13.5 days, once per orbit, as the spacecraft makes it closest approach to Earth, NASA said in a statement.
“I’m thrilled that our new planet hunter mission is ready to start scouring our solar system’s neighborhood for new worlds,” said NASA Astrophysics Division Director Paul Hertz.
“Now that we know there are more planets than stars in our universe, I look forward to the strange, fantastic worlds we’re bound to discover,” Hertz added.
TESS is NASA’s latest satellite to search for planets outside our solar system, known as exoplanets.
The mission will spend the next two years monitoring the nearest and brightest stars for periodic dips in their light.
Using NASA’s Hubble Space Telescope, astronomers have found that violent outbursts, or superflares, from red dwarf stars could affect the habitability of any planets orbiting it.
Young low-mass stars flare much more frequently and more energetically than old stars and middle-age stars like our Sun, the findings of the study published in the Astrophysical Journal showed.
The findings are based on observations of the flare frequency of 12 red dwarfs.
Hubble is observing such stars through a large programme called HAZMAT — Habitable Zones and M dwarf Activity across Time.
“M dwarf” is the astronomical term for a red dwarf star — the smallest, most abundant and longest-living type of star in our galaxy.
The HAZMAT programme is an ultraviolet survey of red dwarfs at three different ages — young, intermediate, and old.
“The goal of the HAZMAT programme is to help understand the habitability of planets around low-mass stars,” explained the programme’s principal investigator, Evgenya Shkolnik from Arizona State University.
“These low-mass stars are critically important in understanding planetary atmospheres,” Shkolnik added.
Stellar flares from red dwarfs are particularly bright in ultraviolet wavelengths, compared with Sun-like stars.
Hubble’s ultraviolet sensitivity makes the telescope very valuable for observing these flares.
The flares are believed to be powered by intense magnetic fields that get tangled by the roiling motions of the stellar atmosphere.
When the tangling gets too intense, the fields break and reconnect, unleashing tremendous amounts of energy.
The team found that the flares from the youngest red dwarfs they surveyed — just about 40 million years old — are 100 to 1,000 times more energetic than when the stars are older.
This younger age is when terrestrial planets are forming around their stars.
About three-quarters of the stars in our Milky Way galaxy are red dwarfs. Most of the galaxy’s “habitable-zone” planets — planets orbiting their stars at a distance where temperatures are moderate enough for liquid water to exist on their surface — orbit red dwarfs.
In fact, the nearest star to our Sun, a red dwarf named Proxima Centauri, has an Earth-size planet in its habitable zone.
However, red dwarfs — especially young red dwarfs — are active stars, producing flares that could blast out so much energy that it disrupts and possibly strips off the atmospheres of these fledgling planets. (IANS)