List of interstellar and circumstellar molecules
Template:Short description Template:Featured list Template:Use British English
This is a list of molecules that have been detected in the interstellar medium and circumstellar envelopes, grouped by the number of component atoms. The chemical formula is listed for each detected compound, along with any ionized form that has also been observed.
BackgroundEdit
The molecules listed below were detected through astronomical spectroscopy. Their spectral features arise because molecules either absorb or emit a photon of light when they transition between two molecular energy levels. The energy (and thus the wavelength) of the photon matches the energy difference between the levels involved. Molecular electronic transitions occur when one of the molecule's electrons moves between molecular orbitals, producing a spectral line in the ultraviolet, optical or near-infrared parts of the electromagnetic spectrum. Alternatively, a vibrational transition transfers quanta of energy to (or from) vibrations of molecular bonds, producing signatures in the mid- or far-infrared. Gas-phase molecules also have quantised rotational levels, leading to transitions at microwave or radio wavelengths.<ref name=shu82/>
Sometimes a transition can involve more than one of these types of energy level e.g. ro-vibrational spectroscopy changes both the rotational and vibrational energy level. Occasionally all three occur together, as in the Phillips band of C2 (diatomic carbon), in which an electronic transition produces a line in the near-infrared, which is then split into several vibronic bands by a simultaneous change in vibrational level, which in turn are split again into rotational branches.<ref>Template:Cite journal</ref>
The spectrum of a particular molecule is governed by the selection rules of quantum chemistry and by its molecular symmetry. Some molecules have simple spectra which are easy to identify, whilst others (even some small molecules) have extremely complex spectra with flux spread among many different lines, making them far harder to detect.<ref name=mcguire_review>Template:Cite journal</ref> Interactions between the atomic nuclei and the electrons sometimes cause further hyperfine structure of the spectral lines. If the molecule exists in multiple isotopologues (versions containing different atomic isotopes), the spectrum is further complicated by isotope shifts.
Detection of a new interstellar or circumstellar molecule requires identifying a suitable astronomical object where it is likely to be present, then observing it with a telescope equipped with a spectrograph working at the required wavelength, spectral resolution and sensitivity. The first molecule detected in the interstellar medium was the methylidyne radical (CH•) in 1937, through its strong electronic transition at 4300 angstroms (in the optical).<ref name=woon05/> Advances in astronomical instrumentation have led to increasing numbers of new detections. From the 1950s onwards, radio astronomy began to dominate new detections, with sub-mm astronomy also becoming important from the 1990s.<ref name=mcguire_review/>
The inventory of detected molecules is highly biased towards certain types which are easier to detect. For example, radio astronomy is most sensitive to small linear molecules with a high molecular dipole.<ref name=mcguire_review/> The most common molecule in the Universe, H2 (molecular hydrogen), is completely invisible to radio telescopes because it has no dipole;<ref name=mcguire_review/> its electronic transitions are too energetic for optical telescopes, so detection of H2 required ultraviolet observations with a sounding rocket.<ref name=apj161/> Vibrational lines are often not specific to an individual molecule, allowing only the general class to be identified. For example, the vibrational lines of polycyclic aromatic hydrocarbons (PAHs) were identified in 1984,<ref name="leger_puget">Template:Cite journal</ref> showing the class of molecules is very common in space,<ref>Template:Cite journal</ref> but it took until 2021 to identify any specific PAHs through their rotational lines.<ref name=mcguire_pah/><ref name=burkhardt_indene/>
One of the richest sources for detecting interstellar molecules is Sagittarius B2 (Sgr B2), a giant molecular cloud near the centre of the Milky Way. About half of the molecules listed below were first found in Sgr B2, and many of the others have been subsequently detected there.<ref name=ajss60/> Many of the largest molecules were first detected in another molecular cloud, TMC-1. A rich source of circumstellar molecules is CW Leonis (also known as IRC +10216), a nearby carbon star, where about 50 molecules have been identified.<ref name=kaler2002/> There is no clear boundary between interstellar and circumstellar media, so both are included in the tables below.
The discipline of astrochemistry includes understanding how these molecules form and explaining their abundances. The extremely low density of the interstellar medium is not conducive to the formation of molecules, making conventional gas-phase reactions between neutral species (atoms or molecules) inefficient. Many regions also have very low temperatures (typically 10 kelvin inside a molecular cloud), further reducing the reaction rates, or high ultraviolet radiation fields, which destroy molecules through photochemistry.<ref name=brown_pais95/> Explaining the observed abundances of interstellar molecules requires calculating the balance between formation and destruction rates using gas-phase ion chemistry (often driven by cosmic rays), surface chemistry on cosmic dust, radiative transfer including interstellar extinction, and sophisticated reaction networks.<ref name=pnas103d/> The use of molecular lines to determine the physical properties of astronomical objects is known as molecular astrophysics.
MoleculesEdit
The following tables list molecules that have been detected in the interstellar medium or circumstellar matter, grouped by the number of component atoms. Neutral molecules and their molecular ions are listed in separate columns; if there is no entry in the molecule column, only the ionized form has been detected. Designations (names of molecules) are those used in the scientific literature describing the detection; if none was given that field is left empty. Mass is listed in atomic mass units. Deuterated molecules, which contain at least one deuterium (2H) atom, have slightly different masses and are listed in a separate table. The total number of unique species, including distinct ionization states, is indicated in each section header.
Most of the molecules detected so far are organic. The only detected inorganic molecule with five or more atoms is SiH4.<ref name="Klemperer2011"/> Molecules larger than that all have at least one carbon atom, with no N−N or O−O bonds.<ref name="Klemperer2011"/>
Diatomic (45)Edit
Molecule | Designation | Mass | Ions | |
---|---|---|---|---|
AlCl | Aluminium monochloride<ref name="aa183"/> | 62.5 | — | |
AlF | Aluminium monofluoride<ref name=apj433/> | 46 | — | |
AlO | Aluminium monoxide<ref name=apj694/> | 43 | — | |
— | Argonium<ref name="BarlowEtAl2013"/><ref name="NYT-20131213">Template:Cite news</ref> | 37<ref group=note>On Earth, the dominant isotope of argon is 40Ar, so ArH+ would have a mass of 41 amu. However, the interstellar detection was of the 36ArH+ isotopologue, which has a mass of 37 amu.</ref> | ArH+ | |
C2 | Diatomic carbon<ref name=souza1977/><ref name=apj438l/> | 24 | — | |
— | Fluoromethylidynium | 31 | CF+<ref name=aaa454/> | |
CH | Methylidyne radical<ref name="NASA-20161012">{{#invoke:citation/CS1|citation | CitationClass=web
}}</ref><ref name="apj93"/> |
13 | CH+<ref name="ptotrsol324"/> |
CN | Cyano radical<ref name="apj93" /><ref name="apj619f"/><ref name=aaa230/> | 26 | CN+,<ref name="dop03"/> CN−<ref name="AgúndezEtAl2010"/> | |
CO | Carbon monoxide<ref name="LAT-20140308" /><ref name="SCI-20140306" /> | 28 | CO+<ref name=apjl419/> | |
CP | Carbon monophosphide<ref name=aaa230 /> | 43 | — | |
CS | Carbon monosulfide<ref name="Ziurys06" /> | 44 | — | |
FeO | Iron(II) oxide<ref name=aaa409/> | 82 | — | |
— | Helium hydride ion<ref name="EG-20190417">Template:Cite news</ref><ref name="NAT-20190417">Template:Cite journal</ref> | 5 | HeH+ | |
H2 | Molecular hydrogen<ref name=apj161/> | 2 | — | |
HCl | Hydrogen chloride<ref name=apj295/> | 36.5 | HCl+<ref name=deluca2012/> | |
HF | Hydrogen fluoride<ref name=apjl488/> | 20 | — | |
HO | Hydroxyl radical<ref name="Ziurys06" /> | 17 | OH+<ref name="WyrowskiEtAl2009"/> | |
KCl | Potassium chloride<ref name="aa183" /> | 75.5 | — | |
NH | Imidogen radical<ref name=apj376m/><ref name=mnras260_2/> | 15 | — | |
N2 | Molecular nitrogen<ref name=spacedaily20040609/><ref name=Nat429/> | 28 | — | |
NO | Nitric oxide<ref name=apj359/> | 30 | NO+<ref name="dop03"/> | |
NS | Nitrogen sulfide<ref name="Ziurys06" /> | 46 | — | |
NaCl | Sodium chloride<ref name="aa183" /> | 58.5 | — | |
— | Magnesium monohydride cation | 25.3 | MgH+<ref name="dop03"/>Template:Page needed{{ safesubst:#invoke:Unsubst | $B=
Template:Fix }} |
O2 | Molecular oxygen<ref name=omol/> | 32 | — | |
PN | Phosphorus mononitride<ref name=tb_pn/><ref name=apj321/> | 45 | — | |
PO | Phosphorus monoxide<ref name=apj666/> | 47 | — | |
SH | Sulfur monohydride<ref name=apj528/> | 33 | SH+<ref name="MentenEtAl2011"/> | |
SO | Sulfur monoxide<ref name="Ziurys06" /> | 48 | SO+<ref name="ptotrsol324" /> | |
SiC | Carborundum<ref name="aass226" /> | 40 | — | |
SiN | –<ref name=turner1992/> | 42 | — | |
SiO | Silicon monoxide<ref name="Ziurys06" /> | 44 | — | |
NaS | Sodium sulfide<ref name="ReyMontejo24" /> | 55 | — | |
MgS | Magnesium sulfide<ref name="ReyMontejo24" /> | 56 | — | |
SiS | Silicon monosulfide<ref name="Ziurys06" /> | 60 | — | |
TiO | Titanium(II) oxide<ref name="KaminskiEtAl2013" /> | 64<ref group="note">Although titanium has several stable isotopes, only the 48Ti16O isotopologue was detected,<ref name="KaminskiEtAl2013" /> which has a molecular mass of 64 amu.</ref> | — |
Triatomic (45)Edit
Template:Redirect [[File:Trihydrogen-cation-3D-vdW.png|right|thumb|The [[Protonated molecular hydrogen|Template:Chem]] cation is one of the most abundant ions in the universe. It was first detected in 1993.<ref name=pnas103oka/><ref name=nature384/>]] Template:Sticky header
Molecule | Designation | Mass | Ions |
---|---|---|---|
AlNC | Aluminium isocyanide<ref name="Ziurys06" /> | 53 | — |
AlOH | Aluminium hydroxide<ref name=apj712/> | 44 | — |
C3 | Tricarbon<ref name=hinkle1988/><ref name=maier2001/> | 36 | — |
C2H | Ethynyl radical<ref name="apj619f" /> | 25 | — |
CCN | Cyanomethylidyne<ref name="AndersonZiuris2014" /> | 38 | — |
C2O | Dicarbon monoxide<ref name=apjl380/> | 40 | — |
C2S | Thioxoethenylidene<ref name="alac26"/> | 56 | — |
C2P | —<ref name=apj677h/> | 55 | — |
CO2 | Carbon dioxide<ref name=mnras252/> | 44 | — |
CaNC | Calcium(I) isocyanide<ref>Template:Cite journal</ref> | 66 | — |
FeCN | Iron(I) cyanide<ref name=apjl733_2/> | 82 | — |
— | Protonated molecular hydrogen | 3 | Template:Chem<ref name=pnas103oka/><ref name=nature384/> |
H2C | Methylene radical<ref name=apj438h/> | 14 | — |
— | Chloronium | 37.5 | H2Cl+<ref name="LisEtAl2010"/> |
H2O | Water<ref name=es0970429/> | 18 | H2O+<ref name="OssenkopfEtAl"/> |
HO2 | Hydroperoxyl<ref name="PariseEtAl2012"/> | 33 | — |
H2S | Hydrogen sulfide<ref name="Ziurys06" /> | 34 | — |
HCN | Hydrogen cyanide<ref name="apj619f" /><ref name=apj163/> | 27 | — |
HNC | Hydrogen isocyanide<ref name=schilke01/><ref name=apj582/> | 27 | — |
HCO | Formyl radical<ref name="apj303"/> | 29 | HCO+<ref name="ptotrsol324" /><ref name="apj303" /><ref name="apj420"/> |
HCP | Phosphaethyne<ref name=apj662/> | 44 | — |
HCS | Thioformyl<ref name=hcs_hsc/> | 45 | HCS+<ref name="ptotrsol324" /><ref name="apj420" /> |
— | Diazenylium<ref name="apj420" /><ref name="ptotrsol324" /><ref name=apj387/> | 29 | Template:Chem |
HNO | Nitroxyl<ref name=hollis91/> | 31 | — |
— | Isoformyl | 29 | HOC+<ref name="apj619f" /> |
HSC | Isothioformyl<ref name=hcs_hsc/> | 45 | — |
KCN | Potassium cyanide<ref name="Ziurys06" /> | 65 | — |
MgCN | Magnesium(I) cyanide<ref name="Ziurys06" /> | 50 | — |
MgNC | Magnesium(I) isocyanide<ref name="Ziurys06" /> | 50 | — |
NH2 | Amino radical<ref name=apj416/> | 16 | — |
N2O | Nitrous oxide<ref name=apj436/> | 44 | — |
NaCN | Sodium cyanide<ref name="Ziurys06" /> | 49 | — |
NaOH | Sodium hydroxide<ref name=apjle262/> | 40 | — |
OCS | Carbonyl sulfide<ref name=apj245/> | 60 | — |
O3 | Ozone<ref name="PhillipsKnapp1980" /> | 48 | — |
SO2 | Sulfur dioxide<ref name="aa130"/> | 64 | — |
c-SiC2 | c-Silicon dicarbide<ref
name="aass226" /> |
52 | — |
SiCSi | Disilicon carbide<ref name="CernicharoEtAl2015" /> | 68 | — |
SiCN | Silicon carbonitride<ref name=aaa363/> | 54 | — |
SiNC | <ref name=aaa426/> | 54 | — |
CaC2 | Calcium dicarbide<ref name=Gupta24/> | 64 | — |
TiO2 | Titanium dioxide<ref name="KaminskiEtAl2013"/> | 79.9 | — |
Four atoms (31)Edit
Molecule | Designation | Mass | Ions |
---|---|---|---|
CH3 | Methyl radical<ref name=apj535_2/> | 15 | Template:Chem2<ref name="NAT-20230626">Template:Cite journal</ref> |
l-C3H | Propynylidyne<ref name="mnotrs16"/> | 37 | l-C3H+<ref name="PetyEtAl2012"/> |
c-C3H | Cyclopropynylidyne<ref name=aaa239/> | 37 | — |
C3N | Cyanoethynyl<ref name=apj438b/> | 50 | C3N−<ref name=apj677t/> |
C3O | Tricarbon monoxide<ref name="mnotrs16" /> | 52 | — |
C3S | Tricarbon sulfide<ref name="alac26" /> | 68 | — |
— | Hydronium | 19 | H3O+<ref name=apj380/> |
C2H2 | Acetylene<ref name="nat264"/> | 26 | — |
H2CN | Methylene amidogen<ref name=apj427/> | 28 | H2CN+<ref name="ptotrsol324" /> |
H2NC | Aminocarbyne<ref name=Cabezas2021/> | 28 | — |
H2CO | Formaldehyde<ref name=prl61/> | 30 | — |
H2CS | Thioformaldehyde<ref name=aaa244a/> | 46 | — |
HCCN | —<ref name=aaa244b/> | 39 | — |
HCCO | Ketenyl<ref name="AgundezEtAl2015"/> | 41 | — |
— | Protonated hydrogen cyanide | 28 | HCNH+<ref name="apj420" /> |
— | Protonated carbon dioxide | 45 | HOCO+<ref name=apj334m/> |
HCNO | Fulminic acid<ref name=apj690/> | 43 | — |
HOCN | Cyanic acid<ref name="BrünkenEtAl2010"/> | 43 | — |
CNCN | Isocyanogen<ref>Template:Cite journal</ref> | 52 | — |
HOOH | Hydrogen peroxide<ref name="BergmanEtAl2011">Template:Citation</ref> | 34 | — |
HNCO | Isocyanic acid<ref name="aa130" /> | 43 | — |
HNCN | Cyanomidyl radical<ref name=rivilla2021 /> | 41 | — |
HNCS | Isothiocyanic acid<ref name=apj234f/> | 59 | — |
NH3 | Ammonia<ref name="aa138"/> | 17 | — |
HSCN | Thiocyanic acid<ref name=apjl702/> | 59 | — |
HNSO | Thionylimide<ref name=thionylimide/> | 63 | — |
SiC3 | Silicon tricarbide<ref name="Ziurys06" /> | 64 | — |
HMgNC | Hydromagnesium isocyanide<ref name="CabezasEtAl2013" /> | 51.3 | — |
HNO2 | Nitrous acid<ref name=hono/> | 47 | — |
Five atoms (21)Edit
Molecule | Designation | Mass | Ions | |
---|---|---|---|---|
— | Ammonium ion | 18 | Template:Chem<ref>{{#invoke:citation/CS1|citation | CitationClass=web
}}</ref><ref>Template:Cite journal</ref> |
CH4 | Methane<ref name=apj376l/> | 16 | — | |
CH3O | Methoxy radical<ref name="CernicharoEtAl2012"/> | 31 | — | |
c-C3H2 | Cyclopropenylidene<ref name="apj619f" /><ref name="precursors"/><ref name="apj552f"/> | 38 | — | |
l-H2C3 | Propadienylidene<ref name="apj552f" /> | 38 | — | |
H2CCN | Cyanomethyl<ref name=apj334i/> | 40 | — | |
H2C2O | Ketene<ref name="aa130" /> | 42 | — | |
H2CNH | Methylenimine<ref name=apj479/> | 29 | — | |
HNCNH | Carbodiimide<ref name="McGuireEtAl2012"/> | 42 | — | |
— | Protonated formaldehyde | 31 | H2COH+<ref name=apj471/> | |
C4H | Butadiynyl<ref name="Ziurys06" /> | 49 | C4H−<ref name=aaa61/> | |
HC3N | Cyanoacetylene<ref name="apj619f" /><ref name="apj420" /><ref name="apj552l" /><ref name="aaa81"/> | 51 | — | |
HCC-NC | Isocyanoacetylene<ref name=apj386/> | 51 | — | |
HCOOH | Formic acid<ref name=1971ApJ...163L..41Z/><ref name="apj552l"/> | 46 | — | |
NH2CN | Cyanamide<ref name=apj201/><ref name=Ligterink2020/> | 42 | — | |
NH2OH | Hydroxylamine<ref name=hydroxylamine/> | 37 | — | |
— | Protonated cyanogen | 53 | NCCNH+<ref name=aanda579/> | |
HC(O)CN | Cyanoformaldehyde<ref name=apj675/> | 55 | — | |
C5 | Linear C5<ref name=bernath89/> | 60 | — | |
HCS2H | dithioformic acid<ref name=manna25/> | 78 | — | |
SiC4 | Silicon-carbide cluster<ref name="aass226" /> | 92 | — | |
SiH4 | Silane<ref name=apj279/> | 32 | — |
Six atoms (16)Edit
Molecule | Designation | Mass | Ions |
---|---|---|---|
c-H2C3O | Cyclopropenone<ref name=apj643hr/> | 54 | — |
E-HNCHCN | E-Cyanomethanimine<ref name="ZaleskiEtAl2013"/> | 54 | — |
C2H4 | Ethylene<ref name="apj244" /> | 28 | — |
CH3CN | Acetonitrile<ref name="aa130" /><ref name="apj632"/><ref name="Alma 2015">Template:Cite news</ref> | 40 | — |
CH3NC | Methyl isocyanide<ref name="apj632" /> | 40 | — |
CH3OH | Methanol<ref name="aa130" /><ref>First Detection of Methyl Alcohol in a Planet-forming Disc. 15 June 2016.</ref> | 32 | — |
CH3SH | Methanethiol<ref name=apj234l/> | 48 | — |
l-H2C4 | Diacetylene<ref name="Cernicharo_546"/> | 50 | — |
— | Protonated cyanoacetylene | 52 | HC3NH+<ref name="apj420" /> |
HCONH2 | Formamide<ref name="apj643hl" /> | 44 | — |
HOCOOH | Carbonic acid<ref>Template:Cite journal</ref> | — | |
C5H | Pentynylidyne<ref name="alac26" /> | 61 | — |
C5N | Cyanobutadiynyl radical<ref name="GuelinEtAl98"/> | 74 | — |
HC2CHO | Propynal<ref name=apj335/> | 54 | — |
HC4N | —<ref name="Ziurys06" /> | 63 | — |
CH2CNH | Ketenimine<ref name="precursors" /> | 40 | — |
C5S | —<ref name="Agundez+2014" /> | 92 | — |
Seven atoms (16)Edit
Molecule | Designation | Mass | Ions |
---|---|---|---|
c-C2H4O | Ethylene oxide<ref name="boaas29"/> | 44 | — |
CH3C2H | Methylacetylene<ref name="apj619f" /> | 40 | — |
H3CNH2 | Methylamine<ref name=apj198/> | 31 | — |
CH2CHCN | Acrylonitrile<ref name="aa130" /><ref name="apj632" /> | 53 | — |
HCCCHNH | Propargylimine<ref>Template:Cite journal</ref> | 53 | — |
H2CHCOH | Vinyl alcohol<ref name="rnao011001" /> | 44 | — |
C6H | Hexatriynyl radical<ref name="alac26" /> | 73 | C6H−<ref name="apj552f" /><ref name=apj652/> |
HC4CN | Cyanodiacetylene<ref name="aa130" /><ref name="aaa81" /><ref name="apj632" /> | 75 | — |
HC4NC | Isocyanodiacetylene<ref name=hc4nc/> | 75 | — |
HC5O | —<ref name=hc5o/> | 77 | — |
CH3CHO | Acetaldehyde<ref name="boaas29" /> | 44 | — |
CH3CHS | Thioacetaldehyde<ref name="thioacetaldehyde" /> | 60 | — |
CH3NCO | Methyl isocyanate<ref name="apj812" /> | 57 | — |
HOCH2CN | Glycolonitrile<ref name=glyconitrile/> | 57 | — |
HC3HCN | 1-cyano propargyl radical<ref name=1cyanopropargyl/> | 64 | — |
CH2C3N | 3-cyano propargyl radical<ref name=3cyanopropargyl/> | 64 | — |
Eight atoms (14)Edit
Molecule | Designation | Mass |
---|---|---|
H3CC2CN | Methylcyanoacetylene<ref name="aj637" /> | 65 |
HC3H2CN | Propargyl cyanide<ref name=propargyl_cyanide/> | 65 |
H2COHCHO | Glycolaldehyde<ref name=hollis2000/> | 60 |
(CHOH)2 | 1,2-ethenediol<ref name="ethenediol"/> | 60 |
HCOOCH3 | Methyl formate<ref name="aa130" /><ref name="apj552l" /> | 60 |
CH3COOH | Acetic acid<ref name="acetic_acid" /> | 60 |
H2C6 | Hexapentaenylidene<ref name="Cernicharo_546" /> | 74 |
CH2CHCHO | Propenal<ref name="precursors" /> | 56 |
CH2CCHCN | Cyanoallene<ref name="precursors" /><ref name="aj637"/> | 65 |
CH3CHNH | Ethanimine<ref name="LoomisEtAl13" /> | 43 |
C2H3NH2 | Vinylamine<ref name=Zeng2021/> | 43 |
C7H | Heptatrienyl radical<ref name=aaa317/> | 85 |
NH2CH2CN | Aminoacetonitrile<ref name=aaa482/> | 56 |
(NH2)2CO | Urea<ref name="RemijanEtAl2014"/> | 60 |
Nine atoms (11)Edit
Molecule | Designation | Mass | Ions |
---|---|---|---|
CH3C4H | Methyldiacetylene<ref name="aj643"/> | 64 | — |
CH3OCH3 | Dimethyl ether<ref name=apj191/> | 46 | — |
CH3CH2CN | Propionitrile<ref name="aa130" /><ref name="apj632" /> | 55 | — |
CH3CONH2 | Acetamide<ref name="precursors" /><ref name="apj643hl" /><ref name=Ligterink2020/> | 59 | — |
CH3CH2OH | Ethanol<ref name=apj196/> | 46 | — |
C8H | Octatetraynyl radical<ref name=aaa309/> | 97 | C8H−<ref name=apj664b/><ref name=apj664r/> |
HC7N | Cyanohexatriyne or Cyanotriacetylene<ref name="aa138" /><ref name="bell_483"/><ref name=apj219/> | 99 | — |
CH3CHCH2 | Propylene (propene)<ref name=apj665/> | 42 | — |
CH3CH2SH | Ethyl mercaptan<ref name="KolesnikovaEtAl2014"/> | 62 | — |
CH3SCH3 | Dimethyl sulfide<ref name=DMS/> | 62 | — |
CH3NHCHO | N-methylformamide<ref name=Ligterink2020/> | 59 | — |
Ten or more atoms (24)Edit
Template:Multiple image Template:Sticky header
Atoms | Molecule | Designation | Mass | Ions |
---|---|---|---|---|
10 | (CH3)2CO | Acetone<ref name="aa130" /><ref name=apj578/> | 58 | — |
10 | (CH2OH)2 | Ethylene glycol<ref name="HollisEtAl2002"/><ref name="Hollis"/> | 62 | — |
10 | CH3CH2CHO | Propanal<ref name="precursors" /> | 58 | — |
10 | CH3OCH2OH | Methoxymethanol<ref name=methoxymethanol/> | 62 | — |
10 | CH3C5N | Methylcyanodiacetylene<ref name="precursors" /> | 89 | — |
10 | CH3CHCH2O | Propylene oxide<ref name=science352/> | 58 | — |
11 | NH2CH2CH2OH | Ethanolamine<ref>Template:Cite journal</ref> | 61 | — |
11 | HC8CN | Cyanotetraacetylene<ref name="bell_483" /> | 123 | — |
11 | C2H5OCHO | Ethyl formate<ref name="arxiv4694"/> | 74 | — |
11 | CH3COOCH3 | Methyl acetate<ref name="TerceroEtAl2013"/> | 74 | — |
11 | CH3C6H | Methyltriacetylene<ref name="precursors" /><ref name="aj643" /> | 88 | — |
12 | C6H6 | Benzene<ref name="Cernicharo_546" /> | 78 | — |
12 | C3H7CN | n-Propyl cyanide<ref name="arxiv4694" /> | 69 | — |
12 | (CH3)2CHCN | iso-Propyl cyanide<ref>Template:Cite news</ref><ref>Template:Cite journal</ref> | 69 | — |
13 | CH3OCH2CH2OH | 2-methoxyethanol<ref name="fried2024" /> | 76 | — |
13 | Template:Chem | Benzonitrile<ref name=benzonitrile/> | 104 | — |
13 | HC10CN | Cyanopentaacetylene<ref name="bell_483" /> | 147 | — |
17 | C9H8 | Indene<ref name=burkhardt_indene /> | 116 | — |
19 | C10H7CN | 1-cyanonaphthalene<ref name=mcguire_pah /> | 153 | — |
19 | C10H7CN | 2-cyanonaphthalene<ref name=mcguire_pah /> | 153 | — |
21 | C12H7CN | 1-cyanoacenaphtylene<ref name=cyanoacenaphtylene /> | 177 | — |
21 | C12H7CN | 5-cyanoacenaphtylene<ref name=cyanoacenaphtylene /> | 177 | — |
27 | C16H9CN | 1-cyanopyrene<ref name=1cyanopyrene /> | 227 | — |
27 | C16H9CN | 2-cyanopyrene<ref name=24cyanopyrene /> | 227 | — |
27 | C16H9CN | 4-cyanopyrene<ref name=24cyanopyrene /> | 227 | — |
37 | C24H11CN | cyanocoronene<ref name=cyanocoronene /> | 325 | — |
60 | C60 | Buckminsterfullerene (C60 fullerene)<ref name=science20100722/> |
720 | Template:Chem<ref name=Foing1994/><ref name=cam15/><ref name=Berne2012/> |
70 | C70 | C70 fullerene<ref name=science20100722/> | 840 | — |
Deuterated molecules (22)Edit
These molecules all contain one or more deuterium atoms, a heavier isotope of hydrogen. Template:Sticky header
Atoms | Molecule | Designation |
---|---|---|
2 | HD | Hydrogen deuteride<ref name=aaa430/><ref name="pass50"/> |
3 | H2D+, Template:Chem | Trihydrogen cation<ref name=aaa430/><ref name="pass50"/> |
3 | HDO, D2O | Heavy water<ref name=ajss70/><ref name=apj659/> |
3 | DCN | Hydrogen cyanide<ref name="apj225"/> |
3 | DCO | Formyl radical<ref name="apj225" /> |
3 | DNC | Hydrogen isocyanide<ref name="apj225" /> |
3 | N2D+ | —<ref name="apj225" /> |
3 | NHD, ND2 | Amidogen<ref name=melosso2020 /> |
4 | NH2D, NHD2, ND3 | Ammonia<ref name="pass50" /><ref name=apj571/><ref name=aaa403/> |
4 | HDCO, D2CO | Formaldehyde<ref name="pass50" /><ref name=apj362/> |
4 | DNCO | Isocyanic acid<ref name="formamide">Template:Cite journal</ref> |
5 | NH3D+ | Ammonium ion<ref name="CernicharoEtAl2013" /><ref name="DomenechEtAl2013"/> |
6 | Template:Chem; NHDCHO | Formamide<ref name="formamide"/> |
7 | CH2DCCH, CH3CCD | Methylacetylene<ref name=aaa253/><ref name=apj627/> |
Unconfirmed (16)Edit
Evidence for the existence of the following molecules has been reported in the scientific literature, but the detections either are described as tentative by the authors, or have been challenged by other researchers. They await independent confirmation.
Atoms | Molecule | Designation |
---|---|---|
2 | SiH | Silylidine<ref name=schilke01/> |
2 | CaO | Calcium oxide<ref name=ReyMontejo24/> |
4 | PH3 | Phosphine<ref name="AgúndezEtAl2008"/> |
4 | MgCCH | Magnesium monoacetylide<ref name="Agundez+2014" /> |
4 | NCCP | Cyanophosphaethyne<ref name="Agundez+2014" /> |
5 | H2NCO+ | —<ref name="GuptaEtAl2013"/> |
6 | SiH3CN | Silyl cyanide<ref name="Agundez+2014"/> |
10 | H2NCH2COOH | Glycine<ref name=apj619s/><ref name=apj593/> |
10 | C2H5NH2 | Ethylamine<ref name=Zeng2021/> |
12 | CO(CH2OH)2 | Dihydroxyacetone<ref name=apjl624/><ref name=apponi2006/> |
12 | C2H5OCH3 | Ethyl methyl ether<ref name="FuchsEtAl2005"/> |
18 | Template:Chem | Naphthalene cation<ref name=apjl685/> |
24 | C24 | Graphene<ref name="García-HernándezEtAl2011"/> |
24 | C14H10 | Anthracene<ref name="Battersby">Template:Cite news</ref><ref name=arxiv1005.4388/> |
26 | C16H10 | Pyrene<ref name="Battersby" /> |
27 | C11H12N2O2 | Tryptophan<ref name=IglesiasGroth2023/><ref name=Hudson2023/><ref name=Dhariwal2024/> |
See alsoEdit
- Astrochemistry
- Cosmic dust
- Diffuse interstellar band
- Lists of molecules
- Molecular astrophysics
- Molecular spectroscopy
- Molecules in stars
- Polycyclic aromatic hydrocarbon (PAH)
- Tholin
NotesEdit
ReferencesEdit
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