Posts Tagged ‘callisto’
[NEWS] Five science links: He Jiankui clones, submoons, ayahuasca, planetary nebulas, black holes
- Chinese scientist He Jiankui, responsible for genetically engineering babies, is along with his team facing serious legal consequences from the Chinese government. SCMP reports.
- A new paper suggests that submoons, moons of a world that is itself a moon, is not only theoretically possible but imaginable in orbit of known worlds including the Moon, Callisto, and Titan. Where are these?
- Is ayahuasca becoming a drug of widespread and legitimate mainstream usage? VICE reports.
- Planetary nebulas, Universe Today reports, are visible for only ten thousand years before their beautiful gases dissipate.
- The interiors of black holes apparently continue to grow indefinitely. (The physics is complicated, as one might expect.) Nautilus has the article.
[LINK] “ESA, Airbus Formalize Jupiter Icy Moons Contract”
The Dragon’s Tales linked to Space News’ report showing that the ESA is set to join NASA in the ranks of deep-space explorers.
The European Space Agency on Dec. 9 signed a contract with Airbus Defence and Space for the construction of ESA’s Juice – Jupiter Icy Moons – orbiter, scheduled for launch in 2022 aboard a European Ariane 5 rocket.
The contract had been expected since ESA’s July decision to approve a contract valued at 350.8 million euros ($374 million) with Airbus after a competition with Thales Alenia Space of France and Italy and OHB SE of Germany, which had submitted a joint bid.
Francois Auque, head of Airbus Space Systems, said Juice hardware will be produced as early as mid-2016, with the full contracting team from 60 companies lined up by 2017. Some 150 people will be working on the prime contractor’s project team at the program’s peak in 2017-2018, he said.
Juice will spend 7.5 years after launch making its way to the Jupiter system, where it will investigate the Europa, Ganymede and Callisto moons. Its mission is expected to last 3.5 years.
[LINK] On why the Galilean moons, unlike Titan, lack atmospheres
The Dragon’s Tales links to a paper, “The formation of the Galilean moons and Titan in the Grand Tack scenario”, that provides an explanation for why Galilean moons like Ganymede and Callisto lack atmospheres despite being as massive as densely-shrouded Titan. Migration in the early solar system explains this.
In the “Grand Tack” (GT) scenario for the young solar system, Jupiter formed beyond 3.5 AU from the Sun and migrated as close as 1.5 AU until it encountered an orbital resonance with Saturn. Both planets then supposedly migrated outward for several 105 yr, with Jupiter ending up at ~5 AU. The initial conditions of the GT and the timing between Jupiter’s migration and the formation of the Galilean satellites remain unexplored. We study the formation of Ganymede and Callisto, both of which consist of ~50% water and rock, respectively, in the GT scenario. We examine why they lack dense atmospheres, while Titan is surrounded by a thick nitrogen envelope. We model an axially symmetric circumplanetary disk (CPD) in hydrostatic equilibrium around Jupiter. The CPD is warmed by viscous heating, Jupiter’s luminosity, accretional heating, and the Sun. The position of the water ice line in the CPD, which is crucial for the formation of massive moons, is computed at various solar distances. We assess the loss of Galilean atmospheres due to high-energy radiation from the young Sun. Ganymede and Callisto cannot have accreted their water during Jupiter’s supposed GT, because its CPD (if still active) was too warm to host ices and much smaller than Ganymede’s contemporary orbit. From a thermal perspective, the Galilean moons might have had significant atmospheres, but these would probably have been eroded during the GT in < 105 yr by solar XUV radiation. Jupiter and the Galilean moons formed beyond 4.5 (+/-0.5) AU and prior to the proposed GT. Thereafter, Jupiter's CPD would have been dry, and delayed accretion of planetesimals should have created water-rich Io and Europa. While Galilean atmospheres would have been lost during the GT, Titan would have formed after Saturn's own tack, because Saturn still accreted substantially for ~106 yr after its closest solar approach, ending up at about 7 AU.
[LINK] “JUICE: Europe’s next mission to Jupiter?”
The Planetary Society Blog’s Emily Lakdawalla noted earlier that JUICE, the proposed European Space Agency unmanned mission to Jupiter and its icy moons that I blogged about last December, has been officially selected and will likely be adopted. This is certainly of note, not only because JUICE is a major expedition that’s the European Space Agency’s attempt to salvage its part of a joint NASA-ESA mission canceled by the American agency, but because this is the first ESA mission into the outer solar system, to this point an exclusive preserve of NASA.
The Twitterverse is buzzing this morning with news that the Science Programme Committee of the European Space Agency has recommended that the next large European mission be JUICE, a mission to explore the three icy Galilean satellites and eventually to orbit Ganymede. The recommendation is not binding; it must be voted upon (a simple majority vote, according to BBC News), at a meeting of the Science Programme Committee, consisting of representatives of all 19 ESA member states, on May 2. The committee is likely to green-light this recommendation, but it shouldn’t be taken as a certain decision just yet.
JUICE is being recommended over ATHENA (an x-ray observatory) and NGO (a gravitational wave observatory). It would launch in June 2022, enter Jupiter orbit in January 2030, and end in Ganymede orbit in June 2033. It is a concept that has been modified from JGO, the Jupiter Ganymede Orbiter, originally conceived as Europe’s half of a US-Europe two-spacecraft mission to Jupiter, where NASA had originally proposed to provide a Jupiter Europa Orbiter. NASA canceled its plans to participate in that mission just as it canceled its participation in ExoMars more recently, and as with ExoMars, ESA appears ready to go forward without the USA. In fact, ESA has modified the originally proposed JGO mission to incorporate some of the science goals that would have been accomplished by NASA’s Europa mission.
Here’s the mission description and profile from the ESA document:
Science goals
The JUICE mission will visit the Jupiter system concentrating on the characterization of Ganymede, Europa and Callisto as planetary objects and potential habitats and on the exploration of the Jupiter system considered as an archetype for gas giants in the solar system and elsewhere. The focus of JUICE is to characterize the conditions that may have led to the emergence of habitable environments among the Jovian icy satellites, with special emphasis on the three ocean-bearing worlds, Ganymede, Europa, and Callisto. The mission will also focus on characterizing the diversity of processes in the Jupiter system which may be required in order to provide a stable environment at Ganymede, Europa and Callisto on geologic time scales, including gravitational coupling between the Galilean satellites and their long term tidal influence on the system as a whole.
Mission profile
The mission will be launched in June 2022 by an Ariane 5 ECA and will perform a 7.5 yr cruise toward Jupiter based on an Earth-Venus-Earth-Earth gravitational assist. The Jupiter orbit insertion will be performed in January 2030, and will be followed by a tour of the Jupiter system, comprising a transfer to Callisto (11 months), a phase studying Europa (with 2 flybys) and Callisto (with 3 flybys) lasting one month, a “Jupiter high-latitude phase” that includes 9 Callisto flybys (lasting 9 months) and the transfer to Ganymede (lasting 11 months). In September 2032 the spacecraft is inserted into orbit around Ganymede, starting with elliptical and high altitude circular orbits (for 5 months) followed by a phase in a medium altitude (500 km) circular orbit (3 months) and by a final phase in low altitude (200 km) circular orbit (1 month). The end of the nominal mission is foreseen in June 2033.
[. . .]
This selection — if it is accepted — represents a big win for planetary science and a big loss for space-based astrophysics in Europe. Which is, one can’t help but notice, opposite to what the currently-proposed NASA budget represents.
I’m pretty ignorant of the internal and external politics involved in these decisions, and also of the relative merits of JUICE, ATHENA, and NGO, so while I admit I’m happy the planetary mission got selected, I don’t feel qualified to comment on whether it should have or shouldn’t have been the one that ESA picked. But, as a member of the American public, I can’t help but see this decision as Europe stepping in to the sucking vacuum left by NASA in the exploration of the outer planets. NASA’s inability to follow up on decades of spectacular successes in outer solar system exploration with any mission beyond Cassini’s end in 2017 leaves an opportunity for Europe to take over the leadership of Earth’s exploration of the solar system beyond the asteroid belt. It remains a challenge that Europe doesn’t currently have the capability to produce radioisotope power sources for spacecraft; limited to solar power at present, that means Europe can’t get beyond Jupiter. But Jupiter is far enough, for now.
The outer planets science community is a small and international one, so for sure there will be American participation in the science team, and probably also in the payload; the ESA document says specifically that “NASA has expressed an interest in contributing to the payload.” Science instruments on ESA missions work differently from NASA. They aren’t paid for by ESA; ESA builds and pays for the spacecraft, but different member states propose, build, and operate the science instruments using their own funds. ESA estimates that the spacecraft will cost €830 million and that ESA member states will spend an estimated €241 million to build instruments. NASA may contribute up to €68 million toward the payload. I hope it contributes the full amount; it’d be hard to imagine a way to get more bang for one’s bucks than to pay for a couple of instruments and 10 or 20 scientists to work on a mission being built, developed, launched, and operated by someone else.
[LINK] “JUICE: Europe’s next mission to Jupiter?”
The Planetary Society Blog’s Emily Lakdawalla noted earlier that JUICE, the proposed European Space Agency unmanned mission to Jupiter and its icy moons that I blogged about last December, has been officially selected and will likely be adopted. This is certainly of note, not only because JUICE is a major expedition that’s the European Space Agency’s attempt to salvage its part of a joint NASA-ESA mission canceled by the American agency, but because this is the first ESA mission into the outer solar system, to this point an exclusive preserve of NASA.
The Twitterverse is buzzing this morning with news that the Science Programme Committee of the European Space Agency has recommended that the next large European mission be JUICE, a mission to explore the three icy Galilean satellites and eventually to orbit Ganymede. The recommendation is not binding; it must be voted upon (a simple majority vote, according to BBC News), at a meeting of the Science Programme Committee, consisting of representatives of all 19 ESA member states, on May 2. The committee is likely to green-light this recommendation, but it shouldn’t be taken as a certain decision just yet.
JUICE is being recommended over ATHENA (an x-ray observatory) and NGO (a gravitational wave observatory). It would launch in June 2022, enter Jupiter orbit in January 2030, and end in Ganymede orbit in June 2033. It is a concept that has been modified from JGO, the Jupiter Ganymede Orbiter, originally conceived as Europe’s half of a US-Europe two-spacecraft mission to Jupiter, where NASA had originally proposed to provide a Jupiter Europa Orbiter. NASA canceled its plans to participate in that mission just as it canceled its participation in ExoMars more recently, and as with ExoMars, ESA appears ready to go forward without the USA. In fact, ESA has modified the originally proposed JGO mission to incorporate some of the science goals that would have been accomplished by NASA’s Europa mission.
Here’s the mission description and profile from the ESA document:
Science goals
The JUICE mission will visit the Jupiter system concentrating on the characterization of Ganymede, Europa and Callisto as planetary objects and potential habitats and on the exploration of the Jupiter system considered as an archetype for gas giants in the solar system and elsewhere. The focus of JUICE is to characterize the conditions that may have led to the emergence of habitable environments among the Jovian icy satellites, with special emphasis on the three ocean-bearing worlds, Ganymede, Europa, and Callisto. The mission will also focus on characterizing the diversity of processes in the Jupiter system which may be required in order to provide a stable environment at Ganymede, Europa and Callisto on geologic time scales, including gravitational coupling between the Galilean satellites and their long term tidal influence on the system as a whole.
Mission profile
The mission will be launched in June 2022 by an Ariane 5 ECA and will perform a 7.5 yr cruise toward Jupiter based on an Earth-Venus-Earth-Earth gravitational assist. The Jupiter orbit insertion will be performed in January 2030, and will be followed by a tour of the Jupiter system, comprising a transfer to Callisto (11 months), a phase studying Europa (with 2 flybys) and Callisto (with 3 flybys) lasting one month, a “Jupiter high-latitude phase” that includes 9 Callisto flybys (lasting 9 months) and the transfer to Ganymede (lasting 11 months). In September 2032 the spacecraft is inserted into orbit around Ganymede, starting with elliptical and high altitude circular orbits (for 5 months) followed by a phase in a medium altitude (500 km) circular orbit (3 months) and by a final phase in low altitude (200 km) circular orbit (1 month). The end of the nominal mission is foreseen in June 2033.
[. . .]
This selection — if it is accepted — represents a big win for planetary science and a big loss for space-based astrophysics in Europe. Which is, one can’t help but notice, opposite to what the currently-proposed NASA budget represents.
I’m pretty ignorant of the internal and external politics involved in these decisions, and also of the relative merits of JUICE, ATHENA, and NGO, so while I admit I’m happy the planetary mission got selected, I don’t feel qualified to comment on whether it should have or shouldn’t have been the one that ESA picked. But, as a member of the American public, I can’t help but see this decision as Europe stepping in to the sucking vacuum left by NASA in the exploration of the outer planets. NASA’s inability to follow up on decades of spectacular successes in outer solar system exploration with any mission beyond Cassini’s end in 2017 leaves an opportunity for Europe to take over the leadership of Earth’s exploration of the solar system beyond the asteroid belt. It remains a challenge that Europe doesn’t currently have the capability to produce radioisotope power sources for spacecraft; limited to solar power at present, that means Europe can’t get beyond Jupiter. But Jupiter is far enough, for now.
The outer planets science community is a small and international one, so for sure there will be American participation in the science team, and probably also in the payload; the ESA document says specifically that “NASA has expressed an interest in contributing to the payload.” Science instruments on ESA missions work differently from NASA. They aren’t paid for by ESA; ESA builds and pays for the spacecraft, but different member states propose, build, and operate the science instruments using their own funds. ESA estimates that the spacecraft will cost €830 million and that ESA member states will spend an estimated €241 million to build instruments. NASA may contribute up to €68 million toward the payload. I hope it contributes the full amount; it’d be hard to imagine a way to get more bang for one’s bucks than to pay for a couple of instruments and 10 or 20 scientists to work on a mission being built, developed, launched, and operated by someone else.