A new system has been discovered in June 2020. The star known as Gliese 887 or Lacaille 9352 is only located at a distance of about 10.74 light-years from Earth. That makes it the eleventh closest star system to our solar system. The star is a low mass M-type star half the size of our Sun and is the brightest M-type star in the sky. The star is still too faint to see with the naked eye but can be seen with a small telescope. The star has the fourth known highest velocity and is moving at 6.9 arcseconds per year (0.000277778 degrees). The discovery was made by using the HARPS spectrograph at the European Southern Observatory in Chile and HIRES in Hawaii. By using the radial velocity method.
Image credit: NASA/JPL-Caltech
The system has two confirmed planets both super-earth sized. Gliese 887 b has a mass of 4.2 of Earth and an orbit period of 9 days and Gliese 887 c has a mass of 7.6 of Earth and an orbit period of 22 days. Both planets are closer to the star than the inner edge of the habitable zone. Gliese 887 c has an estimated temperature of 70 degrees celsius. There was a third signal with a period of 50.7 days in the data that suggest that there is a third planet in the habitable zone, but that may be due to stellar activity.
The good news is that the star is a so-called quiet star with not too much stellar activity much lower than our Sun. Which means that the planets will be able to retain their atmosphere. The brightness of the star is almost constant and that would make it easier to detect any atmospheres on the planet. This makes the new system a candidate for more studies for the upcoming James Webb Space telescope.
It is extremely hard to get a direct image of an exoplanet because our instruments are completely blinded by the bright light from the star. For that reason exoplanets are mostly measured by indirect methods like the transit method or radial velocity or gravitational lensing. Direct imaging is the holy grail of exoplanet studies. When astronomers can study exoplanets in detail we can find out information about the planet's atmosphere and composition and even search for biosignature.
One way to solve it is to use an old technique coronagraph invented by the French astronomer Bernard Lyot in 1930 to study the sun's atmosphere. The coronagraph is a telescopic attachment that is designed to block the light from the star.
Some exoplanets have already been directly imaged by blocking the blinding light from the star. An image was taken of the multi-exoplanet system HR 8799 in September 2008. Three planets with masses of ten to seven times Jupiter were observed. The system is young 30 million years and the planets were still glowing from the formation. A fourth planet was discovered around the same system in 2010.
The very first direct image of an exoplanet was already taken in 2004 when a group of astronomers used the VLT telescope to take a picture of a planet (also this planet was several times the size of Jupiter) orbiting a brown dwarf called 2MASS J12073346-3932539 (don't forget the name).
Direct imaging has also been used on Proxima Centauri, our nearest star at 4.25 light-years away. In 2016 an Earth-like planet was discovered in the habitable zone of the system. Measurement by radial velocity in 2019 suggested that the system also has a larger planet Proxima c outside the habitable zone. The image was taken earlier this year by Raffaele Gratton and his colleagues using a VLT telescope and an instrument called SPHERE. The image has some noise and it could be a planet, but the point is brighter than expected. As the planet would not be that large if it exists. One explanation could be that the planet is surrounded by rings like Saturn but with a smaller planet and bigger rings.
One of the most recent news (May 20 2020) is that an image of an exoplanet being born around the star AB Aurigae 520 light-years from Earth has been taken by VLT using SPHERE.
Credit: ESO/Boccaletti et al.
The planet is formatting at the same distance as Neptune from the Sun.
A new Earth-sized exoplanet has been discovered. Kepler-1649 c has a radius of 1.06 times earth. And just like the name suggests the discovery comes from the Kepler data. The Kepler telescope was retired on October 2018 30, 2018. The planet was originally analyzed by Kepler's Robovetter algorithm. Robovetter is open-source software that automates the process to distinguish between likely planet candidates and false positives in the Kepler dataset.
Image Credit: NASA/Ames Research Center/Daniel Rutter
Robovetter labeled Kepler-1649 c as a false positive. A computer algorithm could make mistakes when it comes to analyzing tricky signals. Therefore a group of scientists called the Kepler False Positive Working Group has the mission to manually review and confirm all those false positives. They discovered that Kepler-1649 c is not a false positive and published these findings in April 2020.
Earlier in 2017 an earth size planet Kepler-1649 b was discovered around the star the planet orbits closer to the star. The interesting thing is how these two exoplanets are interacting with each other when the first planet makes 4 revolutions around its star the second one makes 9. This makes it a very stable system. Kepler-1649 c is in the habitable zone of its star and could have the same temperature as Earth while Kepler-1649 b could be more similar to Venus.
The star Kepler-1649 is 300 light-years away and is a red dwarf star with 0.22 times the mass of our sun. The problem with red dwarfs is that they could have a very high stellar activity that gives violent flares, no flares have been observed around Kepler-1649 so far. This is a very interesting discovery that confirms Earth-size planets in the habitable zone are very common around red dwarf stars. And it increases the possibility that one will have the same condition as Earth
Enceladus is the sixth biggest moon of Saturn. The moon that was discovered by William Herschel in 1789 is named after the giant Enceladus of Greek mythology. It won't live up to its name when it comes to size. With a diameter of 500 km, the moon would fit within the north sea. But it will live up to its name when it comes to being one of the strongest candidates for finding non-terrestrial microbial life in our Solar system. Studies have shown half of Earth's biomass lives long under the surface. As microbial life is not just a surface phenomenon the chances of finding this kind of organism outside the so-called goldilocks zone of a star increases. The strongest candidates are moons around gas giants that under their thick icy surface has oceans heated with volcanic activity. One of those candidates is Jupiter's moon Europa that I wrote about in this . And the other is Enceladus.
Image credit: NASA/JPL-Caltech
On January 16th, 2005 Nasa's probe Cassini's was on a flyby pass Saturn when it captured a very unusual event on Enceladus. There was a bright light coming from the south pole of the moon shining out into space. There were enormous geysers plumbing out vapor into space, more than 8000 times larger than geyser on Earth. Nasa immediately decided that Cassini should have a new mission. To study Enceladus. The probe was reprogrammed from earth to fly into these plumbs and find out was the vapor was made of. It took three years of reprogramming until Cassini was able to do that and the result showed that the vapor was liquid water. Some of the water will fall back on Enceladus as snow but the most will make of the material in Saturn's E ring. The result also showed that the water contains salt which is a very important ingredient for life. The chemicals in the water were very similar to earth and it also showed that something inside Enceladus was heating the water. On June 27, 2018, scientists reported the detection of complex organics compounds from the Cassini data. The Cassini mission ended in September 2017 with the probe crashing into Saturn's atmosphere.
It is very hard getting a probe to investigate Enceladus within a reasonable budget. Several future missions to Enceladus that have been proposed has been canceled. Here is are a list of candidates that are under study and could be our next mission to the icy moon:
TESS has recently found a new Earth-like planet around the star TOI 700. TOI stands for Tess Object of Interest. This is the first discovery of an Earth-like planet done by TESS. The star has three planets called TOI 700 b,TOI 700 c,TOI 700 d. The first planet is TOI 700 b that has the same size as Earth but is very hot and is more like an Earth-size Mercury. The second planet is a Super-Earth eight times the size of Earth. The planet is too hot and would be more like a Super Venus. The third planet is a little larger than Earth with 1.7 the mass of Earth and is in the inner edge of the habitable zone of the star. Technically the planet could have liquid water and support life. The planet would not be an Earth twin as it orbiting an M type star a red dwarf with 40 percent of the mass of our Sun. All the planets will probably have tidally locked orbits were one side of the planet would always face the star and be hot and the other side never gets any light from the star and is cold. Perhaps humans could survive in the area between the cold and hot part of TOI 700 d if the planet has a correct atmosphere.
Image credit: NASA's Goddard Space Flight Center
A problem with red dwarf stars is that they usually have violent flares that could strip any planet of its atmosphere. The good news is that TOI 700 does not show a single flare. There are several indications that the star has low stellar activity and simulations of the planet have shown that it is a strong candidate for being a habitable world. We can not be sure if the star had higher stellar activity and flares in the past. The discovery was also confirmed by NASA’s Spitzer Space Telescope. TOI 700 is located 100 light-years from Earth in the Dorado constellation. We will not be able to visit soon, but next year when James Webb telescope is in use that has a sharper instrument we can receive more information about the composition of the planet.